timelines science

                                              SCIENCE’S TIMELINE

HISTORY OF MATHEMATICS

Ca. 70,000 BC- south african ochre rocks adorned with scratches of geometric patterns.

C. 20,000 BC-1st reference to prime numbers.

2500 bc-multiplication tables

C. 2,000 BC-1st known approximation of the value of pi.

C. 1,800 BC-berlin papyrus 6619 contains the quadratic equation and its solution.

1,650 BC- attempt to square a circle and solutions to linear equations, 1st use of

cotangent, solving linear equations

ANCIENT BABYLON-practical arithmetic, and geometry, use both duodecimal and

decimal systems, composite and prime numbers, arithmetic, geometric, and

harmonic means, sieve of eratosthenes, perfect number theory (number 6), linear

equations, arithmetic and geometric series, solving 2nd order equations

ANCIENT EGYPT- arithmetic and cadastral surveys, use of decimal system

C. 2000-1800 bc-pythagorean triples and pythagorean theorem

1,046 BC-256 BC-arithmetic and geometric algorithms and proofs.

C. 8th century BC-earliest concept of infinity.

800 BC-use of quadratic equation

C. 600 BC-calculation of pythagorean triples, quadratic equations

CLASSICAL GREECE-

key people: thales, pythagoras, euclid

main accomplishments: geometry, logical reasoning

thales-pure geometry, Pythagoras-deductive geometry, special

numbers and ratios, eudoxus-method of exhaustion,

Mathematical rigor, conics, spherical geometry summation of

infinite series

C. 530 BC- discovery of irrational numbers

C. 400 BC-recognition of 5 kinds of infinity

300 BC-earliest information on combinations, fundamental theorem of arithmetic

HELLENISTIC-

Key people: archimedes, apollonius, diophantus

Key accomplishments: algebra

euclid- systematization of deductive geometry, archimedes-applied

math, apollonius-conics, hero-algebraic method, archimedes-rational approximation

of irrational numbers, Diophantus-algebraic notation

300 BC-proof of infinitely many prime numbers; proof of the fundamental theorem of

arithmetic, 1st use of fibonacci numbers and pascal’s triangle

300 BC-abacus

C. 300 BC-1st use of fibonacci numbers and pascal’s triangle

150 BC-knowledge of the theory of numbers, arithmetic operations, geometry,

operations with fractions, simple equations, cubic equations, quartic equations,

permutations, and combinations

150 BC-gaussian elimination, horner’s method, negative numbers, negative numbers

190-120 BC- development of trigonometry

1st century-earliest reference to the square root of a negative number

70-140-menelaus of alexandria on spherical trigonometry

250-350- diophantus- diophantine analysis, diophantine approximations, solutions of

indeterminate equations

179- china- mathematical formula for gaussian elimination

300-earliest use of zero

300-500-chinese remainder theorem

3rd century- cavalier’s principle to find volume of sphere

C. 400-understanding of logarithms to base 2 and computes square roots of numbers

as large as a million correct to 11 decimal places

C. 340-hexagon theorem and centroid theorem

MIDDLE AGES-

key people: khwarizmi

Key accomplishments: algebra

Khwarizmi- development and name of algebra

4th century-hexagon theorem and centroid theorem

500-aryabhata introduces the trigonometry of functions and how to calculate them

628-brahagupta sums series, Brahmagupta identity, brahamguptl theorem

8th century-virasena gives explicit rules for the fibonacci sequence, derivation of the

volume of a frustum using an infinite procedure, knows the laws for base 2

logarithm; shridhara-volume of sphere and formula for solving quadratic equations

9th century-govindsvamin-newton-gauss interpolation formula

C. 850—mahavira rules for expressing a fraction as sum of unit fractions; alkindi-

Frequency analysis

895-thabit Ibn qurra-solution and properties of cubic equations, and theorem of how

amicable numbers can be found

953-al-karaji-algebra replaces geometric operations with arithmetic operations, and

discovered the binomial theorem

975-al-batani-inverse of trigonometric functions

895-solutions and properties of cubic equations

10th to 15 centuries-

Key people: fibonacci

Key accomplishment: trigonometry

rediscovery of ancient knowledge, arabic-hindu numerals to west,

fibonacci-rediscovery of arabic (greek) mathematics

9th century- algebra of irrational numbers with square roots of 4th roots as solutions and

coefficients to quadratic equations, solving 3 nonlinear equations with 3 unknowns

C. 1000-abu-mahmud al-khujandi-special case of fermat’s last theorem, law of sines,al-

karaji-1st known proof by induction and proof of binomial theorem, pascal’s

triangle, and sum of integral cubes, and was 1st to introduce integral calculus

C. 1000-solving equations higher than degree 2

1000-1st proof by mathematical induction and used to prove binomial theorem, pascal’s

triangle, and the sum of integral cubes

1020-adul waft-formula for sin(a+b) and quadrature of parabola and volume of

paraboloid

1100-omar khayyam-general geometric solutions to cubic equations using intersecting

conic sections and laid foundations for development of analytic geometry and non-

euclidean geometry

12th century- bhaskara recognizes that a positive number has 2 square roots,

conceives differential calculus, develops rolle’s theorem, pell’s equation, a proof of

the pythagorean theorem, proves division by zero is infinity, and calculated time

which the earth orbits sun to 9 decimal places

1135-sharafeddin tush-uses algebra to study curves by means of equations-beginning

of analytic geometry

C. 1250-nasir al-din-tusi-attempt to develop non-euclidean geometry

1280-1303-china-solution to simultaneous higher order algebraic equations using

method similar to horner’s method

1303-zhu shijie-method of arranging binomial coefficients in a triangle

14th century-madhava-father of mathematical analysis, worked on power series for pi,

sine, and cosine, and founded important concepts of calculus, parameshvara-

series form of sine function equivalent to Taylor series expansion, and states mean

value theorem of differential calculus, bhaskara-2-mathematical objects equivalent

or approximately equivalent to infinitesimals, derivatives, mean value theorem, and

derivative of sine

1400-madhava-series expansion of inverse-tangent function, infinite series for arctan

and sin

15th century-symbolic algebra and for mathematics in general; nilakantha somayaji-

infinite series expansion

1424-ghiyath al-kashi-computes pi to 16 decimal places using inscribed and

circumscribed polygons

16th centuries-

Key people: tartaglia, cardano, napier, kepler

Key accomplishment: logarithms, infinitesimal, solving cubic and quartic equations

Tartaglia, cardano, bombelli-solution of cubic equations, vieta-

algebraic problems solved trigonometrically, Napier- logarithms, briggs-log tables

1639-cardono solves cubic equations

1540-ferrari solves quartic equations

1545-cardano conceives complex numbers

1572-bombelli uses imaginary numbers to solve cubic equations

17th century-

Key people: newton, Leibniz, Jakob and john Bernoulli, Descartes, fermat

Key accomplishments: calculus, analytic geometry, probability, number

theory, codification algebra development of calculus, kepler-conics as modified

circles, Wallis-mathematics of infinitesimal, limits, Newton and Leibniz-calculus,

Bernoulli’s Jacques and jean-application of calculus, Descartes-coordinate

geometry, desargues- projective geometry, pascal and format-statistical probability

1618- napier uses e in logarithmic work

1619-descartes and fermat- analytic geometry

1629-fermat- rudimentary differential calculus

1637-fermat claims to have proven fermat’s last theorem, 1st use of imaginary numbers

1654-pascal and fermat create theory of probability

1665-newton-fundamental theorem of calculus and infinitesimal calculus

1668-mercator and brouncker discover infinite series for the logarithm while attempting

to calculate area under hyperbolic segment

1671-gregory develops series expansion for inverse-tangent function

1673-leibniz-infintesimal calculus

1675-newton-computation of functional roots

1680s-leibniz-symbolic logic

1683-seki-resultant, determinant, elimination theory

1691-leibniz-separation of variables for ordinary differential equations

1696-l’hospital-rule for computing certain limits

1696-jakob and Johann bernoulli solve brachistochrone problem, the first result in

calculus of variations

18th century-

Key people: euler, Laplace, Lagrange, de moivre, Daniel bernoulli

Key accomplishment: analysis, topology, mathematical physics, complex numbers,

Metric system

cotes,de moivre, maupertius-complex numbers and trigonometry, Euler-

development of analysis, and foundation of topography, Lagrange-calculus of

variations, laplace-mathematical physics

1706-john machin develops a quickly converging inverse-tangent series for pi and computes pi to 100 decimal places

1708-seki-bernoulli numbers

1712-taylor series

1722-de moire formula stated connecting trigonometric functions and complex numbers

1733-de moire introduces normal distribution to approximate binomial distribution in probability

1734-euler’s integrating factor technique to solve 1st-order ordinary differential

equations

1735-euler solves Basel problem relating an infinite series to pi.

1736-euler-7 bridges of konigsberg, graph theory

1739-euler-solves general homogeneous linear ordinary differential equations with

constant coefficients

1742-goldbach’s conjecture

1761-proof of bake’s theorem, lambert-pi irrational

1762-lagrange-divergence theorem

1796-gauss-regular 17-gon constructed with compass and straightedge

1796-legrendre-prime number theorem conjectured

1797-wessel-associates vectors with complex numbers and studies complex numbers

in geometric terms

1799-gauss-fundamental theorem of algebra; ruffini partial proof (abel-ruffini theorem)

quintic or higher equation cannot be solved by general formula

19th century-

Key people- legendre, gauss, Riemann, Hamilton, abel, galois, Cauchy, Jacobi,

dirichlet, labochevski, weierstrauss, lie, klein, Hausdorff, Fourier

Key accomplishments- non-euclidean geometry, vector calculus, matrices, set

theory, group theory, boolean algebra, n-dimestions, theory of infinite

gauss-number theory and method of least squares, fundamental theorem of

algebra, quadratic law of reciprocity, bolyais (fracas and janos), lobachevski,

Riemann-noneuclidean geometry, dedikind-dedikind cuts and

number theory, cantor-theory of infinite sets, mobiles-topology, babage-

calculatikng engine, hamilton-quanternions, grassmann-vector analysis,

Boole-boolean algebra, cayley-matrices, Venn-graphic solutions of set theory

19th century-hermann grassmann-vector spaces, galois-group theory, cantor-set theory

1805-legendre-methods of least squares for fitting a curve to given set of observations

1806-argand diagram

1807-fourier-trigonometric decomposition of functions

1811-gauss-integrals with complex limits

1815-poisson-integration along paths of complex plane

1817-bolzano-intermediate value theorem

1822-cauchy-cauchy integral theorem-integrate around boundary of rectangle in

complex plane

1823-sophie germain theorem

1824-abel partial proof abel-ruffini theorem

1825-cauchy integral theorem for general integration paths, and theory of residues in

complex analysis; dirichlet and legendre-proof Fermat last theorem n=5, ampere-

stoke’s theorem

1828-proof green’s theorem

1829-bolyai, gauss, labochevsky-hyperbolic non-euclidean geometry

Early 1800s-elliptical geometry

1831-ostrogradsky-proof divergence theorem and founding group and galois theory

1832-dirichlet-proof n=14 format’s last theorem, galois general condition for solving of

algebraic equations, thereby founding group theory and galois theory

1835-proof dirichlet theorem about primes in arithmetic progressions

1837-wantzel-proof impossibility double cube and trisect angle with compass and

straight edge, and constructability of regular polygon; dirchlet-analytic number

theory

1841-1843-weierstrauss and laurent-laurent expansion theorem

1843-hamilton-quanternions

1847-boole-symbolic logic/boolean algebra

1850-stoke’s theorem proved

1854-riemann geometry

1854-cayley-quanternions in 4-dimensional space

1858-mobius strip

1859-riemann hypothesis

1870-klein-analytic geometry for labochevskian geometry

1872-dedikind cut

1873-hermite- e transcendental; frobenius-series solutions to linear differential

equations with regular singular points

1874-cantor-real numbers uncountably infinite, but all algebraic numbers countably

infinite

1882-lindemann-pi transcendental and circle cannot be squared with compass and

straightedge; klein bottle

1895-cantor-set theory containing arithmetic of infinite cardinal numbers and continuum

hypothesis

1896-hadamard and vallée poussin prove prime number theorem

1899-cantor-contadiction in set theory

20th century-

Key people: poincare, von neuman, godel, Russell, hilbert, lebesgue, manelbrot

Key accomplishments: game theory, mathematical logic, chaos theory, statistics

einstein-theories of relativities, von neuman-game theory, Russell-math

logic, model- yodel’s theorem, measure theory, qualitative study of dynamical

systems, axiomatization of probability theory, development of functional analysis,

distribution theory, fixed point theory, knot theory, ergodic theory, singularity theory,

catastrophe theory, lie theory, non-standard analysis, information theory, control

theory

1900-hilbert problems

1901-lebesgue integration

1903-runge-fast fourier transform algorithm

1903-landau-much simpler proof prime number theorem

1908-zermelo-axiometization of set theory avoiding cantor’s condradiction; plemelj-

solves reman problem about existence of differential equation with given

monochromic group and uses sokhotsky-plemelj formula

1912-brouwer fixed-point theorem

1915-noether-proves her symmetry theorem which shows symmetry in physics has a corresponding conservation law

1916-ramanujan conjecture

1919-brun’s constant b2 for twin primes

1921-noether-commutative ring

1930-church-lambda calculus

1931-godel imcompleteness theorem

1931-de rham-theorems in cohomology and characteristic classes

1933-boruk-ulam antipodal-point; kolmogorov-axiomatization of probability based on

measure theory

1940-gode-neither continuum hypothesis nor axiom of choice can be disproven from standard axioms of set theory

1942-fast fourier transform algorithm

1945-mac lane and eilenbery-category theory

1949-shannon-information theory

1950-ulam and von neumann-cellular automata dynamical systems

1957-ito calculus

1958-grothendieck-riemann-roch theorem

1959-iwasawa theory

1961-qr algorithm to calculate eigenvalues and eigenvectors of a matrix; smale-proof

dimensions >=5 for poincare conjecture

1963-cohen-neither continuum hypothesis nor axiom choice can be proven with

standard axioms of set theory; butterfly effect

1965-zadeh-fuzzy mathematics

1966-robinson-non-standard analysis

1967-langlands program of conjectures relating number theory and representation

theory

1968-proof of atiyah-singer-index theorem about index of elliptical operators

1975-mandelbrot-fractal

1976-proof 4-color theorem

1973-zadeh-fuzzy logic

1983-falting proves morsel conjecture-only infinite many whole number solutions for

each exponent fermat last theorem

1985-branges proves biererbach conjecture

1986-proof rib’s theorem

1991-connes and lott-non-commutative geometry

1994-shor’s algorithm, a quantum algorithm for

integer factorization

1995-wiles-proof format’s last theorem

1995-baily-borwein-plouffe formula to find nth binary digit of pi

1998-hales-almost certainly proof kepler conjecture

1999- proof taniyama-shimura conjecture

2000-clay mathematics institute millenium prize problems

21st century—

2002-mihailescu proof Catalan’s conjecture

2003-perelman-proof poincare conjecture

2009-ngo baa-proof fundamental lemma (langlands program)

2005-green and tao prove the green-tao theorem

2009-fundamental lemma (langlands program) proved by ego ban Chau

2014-complete kepler’s conjecture proof, calculation of pi to 13.3 trillion digits

2015-tao-solves erdos discrepancy problem, lassie babai found that a quasi polynomial
complexity algorithm would solve the graph isomorphism problem

PHYSICS

ANCIENT GREEKS AND ROMANS
C. 570-490 bc-pythagorean theorem: a^2+b^2=c^2 for a triangle

Early 5th century bc-leucippus opposed the idea of direct intervention in the universe. he and his student democritus were the first to develop a theory of atomism, a theoretical approach that regards something as interpretable through analysis into Distinct and separable, and independent elementary components.

424-347 bc-plato is said to have disliked democritus so much, that he wished his books Burned. Nowadays, many consider democritus to be the father of modern science.

384-322 bc-Aristotle, a student of plato, promoted the concept of natural laws for physical phenomena, which he attempted to explain with the theory of the 4 elements, earth, air, fire, and water. he had a geocentric view of the universe. Aristotelian physics became enormously popular in Europe with the scientific and scholastic developments of the middle ages and remained the mainstream scientific paradigm until the time of Galilei and newton.

310-ca. 230 bc-in contract to Aristotle’s geocentric view, aristarchus of Samos proposed a heliocentric model of the solar system, but received little support from ancient astronomers, although his student seleucus was according to Plutarch, the first to prove the heliocentric system through reasoning. But the argument got lost.

287-212 bc-archimedes- he was responsible for: the foundations of statics and hydrostatics Mathematics of the lever
The archimedes screw/pump

archimede’s principle-law of buoyance
His hypotheses are that the fixed stars and the sun remain unmoved, that the earth revolves about the sun on the circumference of a circle.

90-168-based on previous work by Hipparchus (190-120 bc), ptolemy one of the leading minds of the roman empire, perfected the geocentric system, so that accurate predictions of the planetary movements became possible.

DARK AGES
destruction of the library of alexandria in 48 bc. Most of the direct work of the ancient world got lost (about 40,000), including all 14 books of Hipparchus.
Hindu-arabic numeral system (0,1,2,3…)

MIDDLE AGES
awareness of ancient works re-entered the west through translations from arabic to latin.

C. 1270-roger bacon-conducted studies in optics

SCIENTIFIC REVOLUTION
systematic theory and observation conducted to analyze nature in order to understand how the universe behaves.

1473-1543- Nicolaus copernicus-heliocentism

1546-1601-tycho brace-precise planetary data

1571-1630-johannes kepler-three laws of planetary motion

1564-1642-galilei galileo-birth of modern science. Use of telescope to see 4 of Jupiter’s moons, inertial frames (galileo relativity)

1642-1727-isaac newton-three laws of motion. priincipia mathematic. law of universal gravitation. Calculus.

1690-christian huygen-published a wave theory of light
1738-daniel Bernoulli-hydrodynamics
1788-lagrange-analytical mechanics
1798-count rumford-stated that the motion of particles in a substance produces heat. 1799-1825-laplace-celestial mechanics

THERMODYNAMICS
1650-otto von guerricke-vacuum pump

1662-boyle’s law 1698,1711-savory,newcomen-theory of steam engine 1763-watt-steam engine

1802-joseph gay-lussac-pv=nrt
1824-carnot engine
1831-robert brown-brownian movement
1840-1850-mayer, joule, thomphson-1st law of thermodynamics (energy conserved) 1851-kelvin, 1854-clausius-2nd law of thermodynamics

ELECTRODYNAMICS 1824-alexandra Volta-battery

1820-orsted, ampere-current-magnetic force, current-current force 1821-michael faraday-electric motor
1831-faraday, henry-induction
1850-hippolyte fizeau, león foucault-accurate measurement of speed of light 1864-james clerk maxell-maxwell equations: c=1/sqrt(u(0)e(0) 1890-electromagnetic waves, ether (false), radio

1887-michaelson-morley, 1905-einstein-c is independent of the motion of its source

BIRTH OF MODERN PHYSICS 1895-wilhelm rontgen-x-rays

1896-henri becquerel-natural radioactivity
1897-j.j. thomson-electron, isotopes
Curies-isolate radioactive radium and polonium
1905-einstein-special theory of relativity (electrodynamics of moving bodies) 1906-einstein- e=mc^2

1911-rutherford-rutherford scattering-atomic structure 1916-einstein-general relativity (gravity)

QUANTUM MECHANICS 1900-max planck

1913-bohr- bohr model

1925-heisenberg-uncertainty principle

1926-schrodinger-schrodinger equations

(with contributions from einstein, de Broglie, born, jordan, Pauli, dirac, bose)

1928-dirac-relativistic dirac equation-antimatter

1932-sir john Cockcroft and Ernest watson-bulit first particle accelerator

1932-carl anderson-positron

1938-otto Hahn and fritz strassman-achieved fission of uranium atom

1942-enrico fermi-first controlled nuclear chain reaction

1947-bardeen, Shockley, brattain-invented transistor

BIRTH OF QUANTUM FIELD THEORY 1950-quantum electrodynamics

1964-murray gell-mann-proposed quark as a fundamental particle 1973-quantum chromodynamics

STANDARD MODEL OF PARTICLE PHYSICS
1975-(fermi, be the, Feynman, schwinger, tomonaga, gell-mann, higgs, brout, Sangler, kibble, guralnik, hagen, kibble, Glashow, salam, Weinberg, gross, wilczek, Politzer)

COSMOLOGY 2011-perlmutter, schmidt, ries

HISTORY OF CHEMISTRY

1 1/2 million years ago-  used fire

35,000 bc- bronze (melting copper and tin together)

c. 3000 BC

Egyptians formulate the theory of the Ogdoad, or the “primordial forces”, from which all was formed. These were the elements of chaos, numbered in eight, that existed before the creation of the sun.[2]

c. 1200 BC

Tapputi-Belatikallim, a perfume-maker and early chemist, was mentioned in a cuneiform tablet in Mesopotamia.[3]

c. 450 BC

Empedocles asserts that all things are composed of four primal elements: earth, air, fire, and water, whereby two active and opposing forces, love and hate, or affinity and antipathy, act upon these elements, combining and separating them into infinitely varied forms.[4]

c. 440 BC

Leucippus and Democritus propose the idea of the atom, an indivisible particle that all matter is made of. This idea is largely rejected by natural philosophers in favor of the Aristotlean view (see below).[5][6]

c. 360 BC

Plato coins term ‘elements’ (stoicheia) and in his dialogue Timaeus, which includes a discussion of the composition of inorganic and organic bodies and is a rudimentary treatise on chemistry, assumes that the minute particle of each element had a special geometric shape: tetrahedron (fire), octahedron (air), icosahedron (water), and cube (earth).[7]

c. 350 BC

Aristotle, expanding on Empedocles, proposes idea of a substance as a combination of matter and form. Describes theory of the Five Elements, fire, water, earth, air, and aether. This theory is largely accepted throughout the western world for over 1000 years.[8]

c. 50 BC

Lucretius publishes De Rerum Natura, a poetic description of the ideas of atomism.[9]

c. 300

Zosimos of Panopolis writes some of the oldest known books on alchemy, which he defines as the study of the composition of waters, movement, growth, embodying and disembodying, drawing the spirits from bodies and bonding the spirits within bodies.[10]

c. 770

Abu Musa Jabir ibn Hayyan (aka Geber), an Arab/Persian alchemist who is “considered by many to be the father of chemistry”,[11][12][13] develops an early experimental method for chemistry, and isolates numerous acids, including hydrochloric acid, nitric acid, citric acid, acetic acid, tartaric acid, and aqua regia.[14]

c. 1000

Abū al-Rayhān al-Bīrūnī[15] and Avicenna,[16] both Persian chemists, refute the practice of alchemy and the theory of the transmutation of metals.

c. 1167

Magister Salernus of the School of Salerno makes the first references to the distillation of wine.[17]

c. 1220

Robert Grosseteste publishes several Aristotelian commentaries where he lays out an early framework for the scientific method.[18]

c 1250

Tadeo Alderotti develops fractional distillation, which is much more effective than its predecessors.[19]

c 1260

St Albertus Magnus discovers arsenic[20] and silver nitrate.[21] He also made one of the first references to sulfuric acid.[22]

c. 1267

Roger Bacon publishes Opus Maius, which among other things, proposes an early form of the scientific method, and contains results of his experiments with gunpowder.[23]

c. 1310

Pseudo-Geber, an anonymous Spanish alchemist who wrote under the name of Geber, publishes several books that establish the long-held theory that all metals were composed of various proportions of sulfur and mercury.[24] He is one of the first to describe nitric acid, aqua regia, and aqua fortis.[25]

c. 1530

Paracelsus develops the study of iatrochemistry, a subdiscipline of alchemy dedicated to extending life, thus being the roots of the modern pharmaceutical industry. It is also claimed that he is the first to use the word “chemistry”.[10]

1597

Andreas Libavius publishes Alchemia, a prototype chemistry textbook.[26]

17th and 18th centuries

1605

Sir Francis Bacon publishes The Proficience and Advancement of Learning, which contains a description of what would later be known as the scientific method.[27]

1605

Michal Sedziwój publishes the alchemical treatise A New Light of Alchemy which proposed the existence of the “food of life” within air, much later recognized as oxygen.[28]

1615

Jean Beguin publishes the Tyrocinium Chymicum, an early chemistry textbook, and in it draws the first-ever chemical equation.[29]

1637

René Descartes publishes Discours de la méthode, which contains an outline of the scientific method.[30]

1648

Posthumous publication of the book Ortus medicinae by Jan Baptist van Helmont, which is cited by some as a major transitional work between alchemy and chemistry, and as an important influence on Robert Boyle. The book contains the results of numerous experiments and establishes an early version of the law of conservation of mass.[31]

1661

Robert Boyle publishes The Sceptical Chymist, a treatise on the distinction between chemistry and alchemy. It contains some of the earliest modern ideas of atoms, molecules, and chemical reaction, and marks the beginning of the history of modern chemistry.[32]

1662

Robert Boyle proposes Boyle’s law, an experimentally based description of the behavior of gases, specifically the relationship between pressure and volume.[32]

1735

Swedish chemist Georg Brandt analyzes a dark blue pigment found in copper ore. Brandt demonstrated that the pigment contained a new element, later named cobalt.[33][34]

1754

Joseph Black isolates carbon dioxide, which he called “fixed air”.[35]

1757

Louis Claude Cadet de Gassicourt, while investigating arsenic compounds, creates Cadet’s fuming liquid, later discovered to be cacodyl oxide, considered to be the first synthetic organometallic compound.[36]

1758

Joseph Black formulates the concept of latent heat to explain the thermochemistry of phase changes.[37]

1766

Henry Cavendish discovers hydrogen as a colorless, odourless gas that burns and can form an explosive mixture with air.[38]

1773–1774

Carl Wilhelm Scheele and Joseph Priestley independently isolate oxygen, called by Priestley “dephlogisticated air” and Scheele “fire air”.[39][40]

1778

Antoine Lavoisier, considered “The father of modern chemistry”,[41] recognizes and names oxygen, and recognizes its importance and role in combustion.[42]

1787

Antoine Lavoisier publishes Méthode de nomenclature chimique, the first modern system of chemical nomenclature.[42]

1787

Jacques Charles proposes Charles’s law, a corollary of Boyle’s law, describes relationship between temperature and volume of a gas.[43]

1789

Antoine Lavoisier publishes Traité Élémentaire de Chimie, the first modern chemistry textbook. It is a complete survey of (at that time) modern chemistry, including the first concise definition of the law of conservation of mass, and thus also represents the founding of the discipline of stoichiometry or quantitative chemical analysis.[42][44]

1797

Joseph Proust proposes the law of definite proportions, which states that elements always combine in small, whole number ratios to form compounds.[45]

1800

Alessandro Volta devises the first chemical battery, thereby founding the discipline of electrochemistry.[46]

19th century

1801

John Dalton proposes Dalton’s law, which describes relationship between the components in a mixture of gases and the relative pressure each contributes to that of the overall mixture.[47]

1805

Joseph Louis Gay-Lussac discovers that water is composed of two parts hydrogen and one part oxygen by volume.[48]

1808

Joseph Louis Gay-Lussac collects and discovers several chemical and physical properties of air and of other gases, including experimental proofs of Boyle’s and Charles’s laws, and of relationships between density and composition of gases.[49]

1808

John Dalton publishes New System of Chemical Philosophy, which contains first modern scientific description of the atomic theory, and clear description of the law of multiple proportions.[47]

1808

Jöns Jakob Berzelius publishes Lärbok i Kemien in which he proposes modern chemical symbols and notation, and of the concept of relative atomic weight.[50]

1811

Amedeo Avogadro proposes Avogadro’s law, that equal volumes of gases under constant temperature and pressure contain equal number of molecules.[51]

1825

Friedrich Wöhler and Justus von Liebig perform the first confirmed discovery and explanation of isomers, earlier named by Berzelius. Working with cyanic acid and fulminic acid, they correctly deduce that isomerism was caused by differing arrangements of atoms within a molecular structure.[52]

1827

William Prout classifies biomolecules into their modern groupings: carbohydrates, proteins and lipids.[53]

1828

Friedrich Wöhler synthesizes urea, thereby establishing that organic compounds could be produced from inorganic starting materials, disproving the theory of vitalism.[52]

1832

Friedrich Wöhler and Justus von Liebig discover and explain functional groups and radicals in relation to organic chemistry.[52]

1840

Germain Hess proposes Hess’s law, an early statement of the law of conservation of energy, which establishes that energy changes in a chemical process depend only on the states of the starting and product materials and not on the specific pathway taken between the two states.[54]

1847

Hermann Kolbe obtains acetic acid from completely inorganic sources, further disproving vitalism.[55]

1848

Lord Kelvin establishes concept of absolute zero, the temperature at which all molecular motion ceases.[56]

1849

Louis Pasteur discovers that the racemic form of tartaric acid is a mixture of the levorotatory and dextrotatory forms, thus clarifying the nature of optical rotation and advancing the field of stereochemistry.[57]

1852

August Beer proposes Beer’s law, which explains the relationship between the composition of a mixture and the amount of light it will absorb. Based partly on earlier work by Pierre Bouguer and Johann Heinrich Lambert, it establishes the analytical technique known as spectrophotometry.[58]

1855

Benjamin Silliman, Jr. pioneers methods of petroleum cracking, which makes the entire modern petrochemical industry possible.[59]

1856

William Henry Perkin synthesizes Perkin’s mauve, the first synthetic dye. Created as an accidental byproduct of an attempt to create quinine from coal tar. This discovery is the foundation of the dye synthesis industry, one of the earliest successful chemical industries.[60]

1857

Friedrich August Kekulé von Stradonitz proposes that carbon is tetravalent, or forms exactly four chemical bonds.[61]

1859–1860

Gustav Kirchhoff and Robert Bunsen lay the foundations of spectroscopy as a means of chemical analysis, which lead them to the discovery of caesium and rubidium. Other workers soon used the same technique to discover indium, thallium, and helium.[62]

1860

Stanislao Cannizzaro, resurrecting Avogadro’s ideas regarding diatomic molecules, compiles a table of atomic weights and presents it at the 1860 Karlsruhe Congress, ending decades of conflicting atomic weights and molecular formulas, and leading to Mendeleev’s discovery of the periodic law.[63]

1862

Alexander Parkes exhibits Parkesine, one of the earliest synthetic polymers, at the International Exhibition in London. This discovery formed the foundation of the modern plastics industry.[64]

1862

Alexandre-Emile Béguyer de Chancourtois publishes the telluric helix, an early, three-dimensional version of the periodic table of the elements.[65]

1864

John Newlands proposes the law of octaves, a precursor to the periodic law.[65]

1864

Lothar Meyer develops an early version of the periodic table, with 28 elements organized by valence.[66]

1864

Cato Maximilian Guldberg and Peter Waage, building on Claude Louis Berthollet‘s ideas, proposed the law of mass action.[67][68][69]

1865

Johann Josef Loschmidt determines exact number of molecules in a mole, later named Avogadro’s number.[70]

1865

Friedrich August Kekulé von Stradonitz, based partially on the work of Loschmidt and others, establishes structure of benzene as a six carbon ring with alternating single and double bonds.[61]

1865

Adolf von Baeyer begins work on indigo dye, a milestone in modern industrial organic chemistry which revolutionizes the dye industry.[71]

1869

Dmitri Mendeleev publishes the first modern periodic table, with the 66 known elements organized by atomic weights. The strength of his table was its ability to accurately predict the properties of as-yet unknown elements.[65][66]

1873

Jacobus Henricus van ‘t Hoff and Joseph Achille Le Bel, working independently, develop a model of chemical bonding that explains the chirality experiments of Pasteur and provides a physical cause for optical activity in chiral compounds.[72]

1876

Josiah Willard Gibbs publishes On the Equilibrium of Heterogeneous Substances, a compilation of his work on thermodynamics and physical chemistry which lays out the concept of free energy to explain the physical basis of chemical equilibria.[73]

1877

Ludwig Boltzmann establishes statistical derivations of many important physical and chemical concepts, including entropy, and distributions of molecular velocities in the gas phase.[74]

1883

Svante Arrhenius develops ion theory to explain conductivity in electrolytes.[75]

1884

Jacobus Henricus van ‘t Hoff publishes Études de Dynamique chimique, a seminal study on chemical kinetics.[76]

1884

Hermann Emil Fischer proposes structure of purine, a key structure in many biomolecules, which he later synthesized in 1898. Also begins work on the chemistry of glucose and related sugars.[77]

1884

Henry Louis Le Chatelier develops Le Chatelier’s principle, which explains the response of dynamic chemical equilibria to external stresses.[78]

1885

Eugene Goldstein names the cathode ray, later discovered to be composed of electrons, and the canal ray, later discovered to be positive hydrogen ions that had been stripped of their electrons in a cathode ray tube. These would later be named protons.[79]

1893

Alfred Werner discovers the octahedral structure of cobalt complexes, thus establishing the field of coordination chemistry.[80]

1894–1898

William Ramsay discovers the noble gases, which fill a large and unexpected gap in the periodic table and led to models of chemical bonding.[81]

1897

J. J. Thomson discovers the electron using the cathode ray tube.[82]

1898

Wilhelm Wien demonstrates that canal rays (streams of positive ions) can be deflected by magnetic fields, and that the amount of deflection is proportional to the mass-to-charge ratio. This discovery would lead to the analytical technique known as mass spectrometry.[83]

1898

Maria Sklodowska-Curie and Pierre Curie isolate radium and polonium from pitchblende.[84]

c. 1900

Ernest Rutherford discovers the source of radioactivity as decaying atoms; coins terms for various types of radiation.[85]

20th century

1903

Mikhail Semyonovich Tsvet invents chromatography, an important analytic technique.[86]

1904

Hantaro Nagaoka proposes an early nuclear model of the atom, where electrons orbit a dense massive nucleus.[87]

1905

Fritz Haber and Carl Bosch develop the Haber process for making ammonia from its elements, a milestone in industrial chemistry with deep consequences in agriculture.[88]

1905

Albert Einstein explains Brownian motion in a way that definitively proves atomic theory.[89]

1907

Leo Hendrik Baekeland invents bakelite, one of the first commercially successful plastics.[90]

1909

Robert Millikan measures the charge of individual electrons with unprecedented accuracy through the oil drop experiment, confirming that all electrons have the same charge and mass.[91]

1909

S. P. L. Sørensen invents the pH concept and develops methods for measuring acidity.[92]

1911

Antonius van den Broek proposes the idea that the elements on the periodic table are more properly organized by positive nuclear charge rather than atomic weight.[93]

1911

The first Solvay Conference is held in Brussels, bringing together most of the most prominent scientists of the day. Conferences in physics and chemistry continue to be held periodically to this day.[94]

1911

Ernest Rutherford, Hans Geiger, and Ernest Marsden perform the gold foil experiment, which proves the nuclear model of the atom, with a small, dense, positive nucleus surrounded by a diffuse electron cloud.[85]

1912

William Henry Bragg and William Lawrence Bragg propose Bragg’s law and establish the field of X-ray crystallography, an important tool for elucidating the crystal structure of substances.[95]

1912

Peter Debye develops the concept of molecular dipole to describe asymmetric charge distribution in some molecules.[96]

1913

Niels Bohr introduces concepts of quantum mechanics to atomic structure by proposing what is now known as the Bohr model of the atom, where electrons exist only in strictly defined orbitals.[97]

1913

Henry Moseley, working from Van den Broek’s earlier idea, introduces concept of atomic number to fix inadequacies of Mendeleev’s periodic table, which had been based on atomic weight.[98]

1913

Frederick Soddy proposes the concept of isotopes, that elements with the same chemical properties may have differing atomic weights.[99]

1913

J. J. Thomson expanding on the work of Wien, shows that charged subatomic particles can be separated by their mass-to-charge ratio, a technique known as mass spectrometry.[100]

1916

Gilbert N. Lewis publishes “The Atom and the Molecule”, the foundation of valence bond theory.[101]

1921

Otto Stern and Walther Gerlach establish concept of quantum mechanical spin in subatomic particles.[102]

1923

Gilbert N. Lewis and Merle Randall publish Thermodynamics and the Free Energy of Chemical Substances, first modern treatise on chemical thermodynamics.[103]

1923

Gilbert N. Lewis develops the electron pair theory of acid/base reactions.[101]

1924

Louis de Broglie introduces the wave-model of atomic structure, based on the ideas of wave–particle duality.[104]

1925

Wolfgang Pauli develops the exclusion principle, which states that no two electrons around a single nucleus may have the same quantum state, as described by four quantum numbers.[105]

1926

Erwin Schrödinger proposes the Schrödinger equation, which provides a mathematical basis for the wave model of atomic structure.[106]

1927

Werner Heisenberg develops the uncertainty principle which, among other things, explains the mechanics of electron motion around the nucleus.[107]

1927

Fritz London and Walter Heitler apply quantum mechanics to explain covalent bonding in the hydrogen molecule,[108] which marked the birth of quantum chemistry.[109]

1929

Linus Pauling publishes Pauling’s rules, which are key principles for the use of X-ray crystallography to deduce molecular structure.[110]

1931

Erich Hückel proposes Hückel’s rule, which explains when a planar ring molecule will have aromatic properties.[111]

1931

Harold Urey discovers deuterium by fractionally distilling liquid hydrogen.[112]

1932

James Chadwick discovers the neutron.[113]

1932–1934

Linus Pauling and Robert Mulliken quantify electronegativity, devising the scales that now bear their names.[114]

1935

Wallace Carothers leads a team of chemists at DuPont who invent nylon, one of the most commercially successful synthetic polymers in history.[115]

1937

Carlo Perrier and Emilio Segrè perform the first confirmed synthesis of technetium-97, the first artificially produced element, filling a gap in the periodic table. Though disputed, the element may have been synthesized as early as 1925 by Walter Noddack and others.[116]

1937

Eugene Houdry develops a method of industrial scale catalytic cracking of petroleum, leading to the development of the first modern oil refinery.[117]

1937

Pyotr Kapitsa, John Allen and Don Misener produce supercooled helium-4, the first zero-viscosity superfluid, a substance that displays quantum mechanical properties on a macroscopic scale.[118]

1938

Otto Hahn discovers the process of nuclear fission in uranium and thorium.[119]

1939

Linus Pauling publishes The Nature of the Chemical Bond, a compilation of a decades worth of work on chemical bonding. It is one of the most important modern chemical texts. It explains hybridization theory, covalent bonding and ionic bonding as explained through electronegativity, and resonance as a means to explain, among other things, the structure of benzene.[110]

1940

Edwin McMillan and Philip H. Abelson identify neptunium, the lightest and first synthesized transuranium element, found in the products of uranium fission. McMillan would found a lab at Berkeley that would be involved in the discovery of many new elements and isotopes.[120]

1941

Glenn T. Seaborg takes over McMillan’s work creating new atomic nuclei. Pioneers method of neutron capture and later through other nuclear reactions. Would become the principal or co-discoverer of nine new chemical elements, and dozens of new isotopes of existing elements.[120]

1945

Jacob A. Marinsky, Lawrence E. Glendenin, and Charles D. Coryell perform the first confirmed synthesis of Promethium, filling in the last “gap” in the periodic table.[121]

1945–1946

Felix Bloch and Edward Mills Purcell develop the process of nuclear magnetic resonance, an analytical technique important in elucidating structures of molecules, especially in organic chemistry.[122]

1951

Linus Pauling uses X-ray crystallography to deduce the secondary structure of proteins.[110]

1952

Alan Walsh pioneers the field of atomic absorption spectroscopy, an important quantitative spectroscopy method that allows one to measure specific concentrations of a material in a mixture.[123]

1952

Robert Burns Woodward, Geoffrey Wilkinson, and Ernst Otto Fischer discover the structure of ferrocene, one of the founding discoveries of the field of organometallic chemistry.[124]

1953

James D. Watson and Francis Crick propose the structure of DNA, opening the door to the field of molecular biology.[125]

1957

Jens Skou discovers Na⁺/K⁺-ATPase, the first ion-transporting enzyme.[126]

1958

Max Perutz and John Kendrew use X-ray crystallography to elucidate a protein structure, specifically sperm whale myoglobin.[127]

1962

Neil Bartlett synthesizes xenon hexafluoroplatinate, showing for the first time that the noble gases can form chemical compounds.[128]

1962

George Olah observes carbocations via superacid reactions.[129]

1964

Richard R. Ernst performs experiments that will lead to the development of the technique of Fourier transform NMR. This would greatly increase the sensitivity of the technique, and open the door for magnetic resonance imaging or MRI.[130]

1965

Robert Burns Woodward and Roald Hoffmann propose the Woodward–Hoffmann rules, which use the symmetry of molecular orbitals to explain the stereochemistry of chemical reactions.[124]

1966

Hitoshi Nozaki and Ryōji Noyori discovered the first example of asymmetric catalysis (hydrogenation) using a structurally well-defined chiral transition metal complex.[131][132]

1970

John Pople develops the Gaussian program greatly easing computational chemistry calculations.[133]

1971

Yves Chauvin offered an explanation of the reaction mechanism of olefin metathesis reactions.[134]

1975

Karl Barry Sharpless and group discover a stereoselective oxidation reactions including Sharpless epoxidation,[135][136] Sharpless asymmetric dihydroxylation,[137][138][139] and Sharpless oxyamination.[140][141][142]

1985

Harold Kroto, Robert Curl and Richard Smalley discover fullerenes, a class of large carbon molecules superficially resembling the geodesic dome designed by architect R. Buckminster Fuller.[143]

1991

Sumio Iijima uses electron microscopy to discover a type of cylindrical fullerene known as a carbon nanotube, though earlier work had been done in the field as early as 1951. This material is an important component in the field of nanotechnology.[144]

1994

First total synthesis of Taxol by Robert A. Holton and his group.[145][146][147]

1995

Eric Cornell and Carl Wieman produce the first Bose–Einstein condensate, a substance that displays quantum mechanical properties on the macroscopic scale.[148]

Alchemists learned ways to make acids

HISTORY OF ASTRONOMY

750 BC

Babylonian astronomers discover an 18.6-year cycle in the rising and setting of the Moon. From this they created the first almanacs – tables of the movements of the Sun, Moon and planets for the use in astrology. In 6th century BC Greece, this knowledge is used to predict eclipses.

585 BC
Thales predicts a solar eclipse. 467 BC

Anaxagoras produced a correct explanation for eclipses and then described the sun as a fiery mass larger than the Peloponnese , as well as attempting to explain rainbows and meteors . He was the first to explain that the moon shines due to reflected light from the sun.[1][2][3]

388 BC

Plato, a Greek philosopher, founds a school (the Platonic Academy) that will influence the next 2000 years. It promotes the idea that everything in the universe moves in harmony and that the Sun, Moon, and planets move around Earth in perfect circles.

270 BC

Aristarchus of Samos proposes heliocentrism as an alternative to the Earth-centered universe. His heliocentric model places the Sun at its center, with Earth as just one planet orbiting it. However, there were only a few people who took the theory seriously.

164 BC

The earliest recorded sighting of Halley’s Comet is made by Babylonian astronomers. Their records of the comet’s

movement allow astronomers today to predict accurately how the comet’s orbit changes over the centuries.

4 BC

The astronomer Shi Shen is believed to have cataloged 809 stars in 122 constellations, and he also made the earliest known observation of sunspots.

140 AD

Ptolemy publishes his star catalogue, listing 48 constellations and endorses the geocentric (Earth- centered) view of the universe. His views go unquestioned for nearly 1500 years in Europe, and are passed down to Arabic and medieval European astronomers in his book the Almagest.

400

The Hindu cosmological time cycles explained in the Surya Siddhanta, give the average length of the sidereal year (the length of the Earth’s revolution around the Sun) as 365.2563627 days, which is only 1.4 seconds longer than the modern value of 365.256363004 days.[4] This remains the most accurate estimate for the length of the sidereal year anywhere in the world for over a thousand years.

499 CE

 

Indian mathematician-astronomer Aryabhata, in his Aryabhatiya first identifies the force gravity to explain why objects do not fall when the earth rotates.[5] propounds a geocentric solar system of gravitation, and an eccentric elliptical model of the planets, where the planets spin on their axes and follow elliptical orbits,the Sun and the moon revolve around the earth in epicycles. He also writes that the planets and the Moon do not have their own light but reflect the light of the Sun, and that the Earth rotates on its axis causing day and night and also sun around the earth causing years.

628

Indian mathematician-astronomer Brahmagupta, in his Brahma-Sphuta- Siddhanta, first recognizes gravity as a force of attraction, and briefly describes the second law of Newton’s law of universal gravitation. He gives methods for calculations of the motions and places of various planets, their rising and setting, conjunctions, and calculations of the solar and lunar eclipses.

773

The Sanskrit works of Aryabhata and Brahmagupta, along with the Sanskrit text Surya Siddhanta, are translated into Arabic, introducing Arabic astronomers to Indian astronomy.

777

Muhammad al-Fazari and Yaqub ibn Tariq translate the Surya Siddhanta and Brahmasphutasiddhanta, and

compile them as the Zij al-Sindhind, the first Zij treatise. [6]

830

The first major Arabic work of astronomy is the Zij al- Sindh by al- Khwarizimi. The work contains tables for the movements of the sun, the moon and the five planets known at the time. The work is significant as it introduced Ptolemaic concepts into Islamic sciences. This work also marks the turning point in Arabic astronomy. Hitherto, Arabic astronomers had adopted a primarily research approach to the field, translating works of others and learning already discovered knowledge. Al-Khwarizmi’s work marked the beginning of nontraditional methods of study and calculations.[7]

850

al-Farghani wrote Kitab fi Jawani (“A compendium of the science of stars“). The book primarily gave a summary of Ptolemic cosmography. However, it also corrected Ptolemy based on findings of earlier Arab astronomers. Al- Farghani gave revised values for the obliquity of the ecliptic, the precessional movement of the apogees of the sun and the moon, and the circumference of the earth. The books were widely circulated through the Muslim world, and even translated into Latin.[8]

928

The earliest surviving astrolabe is constructed by Islamic mathematician- astronomer Mohammad al-Fazari. Astrolabes are the most advanced instruments of their time. The precise measurement of the positions of stars and planets allows Islamic astronomers to compile the most detailed almanacs and star atlases yet.

1030

Abū Rayḥān al-Bīrūnī discussed the Indian heliocentric theories of Aryabhata, Brahmagupta and Varahamihira in his Ta’rikh al-Hind (Indica in Latin). Biruni stated that the followers of Aryabhata consider the Earth to be

at the center. In fact, Biruni casually stated that this does not create any mathematical problems.[9]

1031

Abu Said Sinjari, a contemporary of Abu Rayhan Biruni, suggested the possible heliocentric movement of the Earth around the Sun.[10]

1054

Chinese astronomers record the sudden appearance of a bright star. Native-American rock carvings also show the brilliant star close to the Moon. This star is the Crab supernova exploding.

1070

Abu Ubayd al-Juzjani published the Tarik al-Aflak. In his work, he indicated the so-called “equant” problem of the Ptolemic model. Al-Juzjani even proposed a solution for the problem. In al-Andalus, the anonymous work al- Istidrak ala Batlamyus (meaning “Recapitulation regarding Ptolemy”), included a list of objections to the Ptolemic astronomy.

One of the most important works in the period was Al- Shuku ala Batlamyus (“Doubts on Ptolemy“). In this, the author summed up the inconsistencies of the Ptolemic models. Many astronomers took up the challenge posed in this work, namely to develop alternate models that evaded such errors.

1126

Islamic and Indian astronomical works (including Aryabhatiya and Brahma- Sphuta-Siddhanta) are translated into Latin in Córdoba, Spain in 1126, introducing European astronomers to Islamic and Indian astronomy.

1150

Indian mathematician-astronomer Bhāskara II, in his Siddhanta Shiromani, calculates the longitudes and latitudes of the planets, lunar and solar eclipses, risings

and settings, the Moon’s lunar crescent, syzygies, and conjunctions of the planets with each other and with the fixed stars, and explains the three problems of diurnal rotation. He also calculates the planetary mean motion, ellipses, first visibilities of the planets, the lunar crescent, the seasons, and the length of the Earth’s revolution around the Sun to 9 decimal places.

1250

Mo’ayyeduddin Urdi develops the Urdi lemma, which is later used in the Copernican heliocentric model.

Nasir al-Din al-Tusi resolved significant problems in the Ptolemaic system by developing the Tusi-couple as an alternative to the physically problematic equant introduced by Ptolemy.[11] His Tusi-couple is later used in the Copernican model.

Tusi’s student Qutb al-Din al-Shirazi, in his The Limit of Accomplishment concerning Knowledge of the Heavens, discusses the possibility of heliocentrism.
Najm al-Din al-Qazwini al-Katibi, who also worked at the Maraghah observatory, in his Hikmat al-‘Ain, wrote an argument for a heliocentric model, though he later abandoned the idea.[10]

1350

Ibn al-Shatir (1304–1375), in his A Final Inquiry Concerning the Rectification of Planetary Theory,

eliminated the need for an equant by introducing an extra epicycle, departing from the Ptolemaic system in a way very similar to what Copernicus later also did. Ibn al-Shatir proposed a system that was only approximately geocentric, rather than exactly so, having demonstrated trigonometrically that the Earth was not the exact center of the universe. His rectification is later used in the Copernican model.

1543

Nicolaus Copernicus publishes De revolutionibus orbium coelestium containing his theory that Earth travels around the Sun. However, he complicates his theory by retaining Plato’s perfect circular orbits of the planets.

1573

A brilliant supernova (SN 1572 – thought, at the time, to be a comet) is observed by Tycho Brahe, who proves that it is traveling beyond Earth’s atmosphere and therefore provides the first evidence that the heavens can change.

1608

Dutch eyeglass maker Hans Lippershey invents the refracting telescope. The invention spreads rapidly across Europe, as scientists make their own

instruments. Their discoveries begin a revolution in astronomy.

1609

Johannes Kepler publishes his New Astronomy. In this and later works, he announces his three laws of planetary motion, replacing the circular orbits

of Plato with elliptical ones. Almanacs based on his laws prove to be highly accurate.

1610

Galileo Galilei publishes Sidereus Nuncius describing the findings of his observations with the telescope he built. These include spots on the Sun, craters on the Moon, and four satellites of Jupiter. Proving that not everything orbits Earth, he promotes the Copernican view of a Sun- centered universe.

1655

As the power and the quality of the telescopes increase, Christiaan Huygens studies Saturn and discovers its largest satellite, Titan. He also explains Saturn’s appearance, suggesting the planet is surrounded by a thin ring.

1663

Scottish astronomer James Gregory describes his “gregorian” reflecting telescope, using parabolic mirrors instead of lenses to reduce chromatic aberration and spherical aberration, but is unable to build one.

1668

Isaac Newton builds the first reflecting telescope, his Newtonian telescope. 1687

Isaac Newton publishes his first copy of the book Philosophiae Naturalis Principia Mathematica, establishing the theory of gravitation and laws of motion. The Principia explains Kepler’s laws of planetary motion and allows astronomers to understand the forces acting between the Sun, the planets, and their moons.

1705

Edmond Halley calculates that the comets recorded at 76-year intervals from 1456 to 1682 are one and the same. He predicts that the comet will return again in 1758. When it reappears as expected, the comet is named in his honor.

1750

French astronomer Nicolas de Lacaille sails to southern oceans and begins work compiling a catalog of more than 10000 stars in the southern sky. Although Halley

and others have observed from the Southern Hemisphere

before, Lacaille’s star catalog is the first comprehensive one of the southern sky.

1781

Amateur astronomer William Herschel discovers the planet Uranus, although he at first mistakes it for a comet. Uranus is the first planet to be discovered beyond Saturn, which was thought to be the most distant planet in ancient times.

1784

Charles Messier publishes his catalog of star clusters and nebulas. Messier draws up the list to prevent these objects from being identified as comets. However, it soon becomes a standard reference for the study of star clusters and nebulars and is still in use today.

1800

William Herschel splits sunlight through a prism and with a thermometer, measures the energy given out by different colours. He notices a sudden increase in energy beyond the red end of the spectrum, discovering invisible infrared and laying the foundations of spectroscopy.

1801

Italian astronomer Giuseppe Piazzi discovers what appears to be a new planet orbiting between Mars and Jupiter, and names it Ceres. William Herschel proves it is a very small object, calculating it to be only 320 km in diameter, and not a planet. He proposes the name asteroid, and soon other similar bodies are being found. We now know that Ceres is 932 km in diameter, and is now considered to be a dwarf planet.

1814

Joseph von Fraunhofer builds the first accurate spectrometer and uses it to study the spectrum of the Sun’s light. He discovers and maps hundreds of fine dark lines crossing the solar spectrum. In 1859 these lines are linked to chemical elements in the Sun’s atmosphere. Spectroscopy becomes a method for studying what stars are made of.

1838

Friedrich Bessel successfully uses the method of stellar parallax, the effect of Earth’s annual movement around the Sun, to calculate the distance to 61 Cygni, the first star other than the Sun to have its distance from Earth measured. Bessel’s is a truly accurate measurement of stellar positions,

and the parallax technique establishes a framework for measuring the scale of the universe.

1843

German Amateur astronomer Heinrich Schwabe, who has been studying the Sun for the past 17 years, announces his discovery of a regular cycle in sunspot numbers – the first clue to the Sun’s internal structure.

1845

Irish astronomer William Parsons, 3rd Earl of Rosse completes the first of the world’s great telescopes, with a 180-cm mirror. He uses it to study and draw the structure of nebulas, and within a few months discovers the spiral structure of the Whirlpool Galaxy.

French physicists Jean Foucault and Armand Fizeau take the first detailed photographs of the Sun’s surface through a telescope – the birth of scientific astrophotography. Within five years, astronomers produce the first detailed photographs of the Moon. Early film is not sensitive enough to image stars.

1846

A new planet, Neptune, is identified by German astronomer Johann Gottfried Galle while searching in the position suggested by Urbain Le Verrier. Le Verrier has calculated the position and size of the planet from

the effects of its gravitational pull on the orbit of Uranus. An English mathematician, John Couch Adams, also made a similar calculation a year earlier.

1868

Astronomers notice a new bright emission line in the spectrum of the Sun’s atmosphere during an eclipse. The emission line is caused by an element’s giving out light, and British astronomer Norman Lockyer concludes that it is an element unknown on Earth. He calls it helium, from the Greek word for the Sun. Nearly 30 years later, helium is found on Earth.

1872

An American astronomer Henry Draper takes the first photograph of the spectrum of a star (Vega), showing absorption lines that reveal its chemical makeup. Astronomers begin to see that spectroscopy is the key to understanding how stars evolve. William Huggins uses absorption lines to measure the redshifts of stars, which give the first indication of how fast stars are moving.

1895

Konstantin Tsiolkovsky publishes his first article on the possibility of space flight. His greatest discovery is that a rocket, unlike other forms of propulsion, will work in a vacuum. He also outlines the principle of a multistage launch vehicle.

1901

A comprehensive survey of stars, the Henry Draper Catalog, is published. In the catalog, Annie Jump Cannon proposes a sequence of classifying stars by the absorption waves in their spectra, which is still in use today.

1906

Ejnar Hertzsprung establishes the standard for measuring the true brightness of a star. He shows that there is a relationship between color and absolute magnitude for 90% of the stars in the Milky Way Galaxy. In 1913, Henry Norris Russell publishes a diagram that shows this relationship. Although astronomers agree that the diagram shows the sequence in which stars evolve, they argue about which way the sequence progresses. Arthur Eddington finally settles the controversy in 1924.

1916

German physicist Karl Schwarzschild uses Albert Einstein’s theory of general relativity to lay the groundwork for black hole theory. He suggests that if any star collapse to a certain size or smaller, its gravity

will be so strong that no form of radiation will escape from it.

1923

Edwin Hubble discovers a Cepheid variable star in the “Andromeda Nebula” and proves that Andromeda and other nebulas are galaxies far beyond our own. By 1925, he produces a classification system for galaxies.

1926

Robert Goddard launches the first rocket powered by liquid fuel. He also demonstrates that a rocket can work in a vacuum. His later rockets break the sound barrier for the first time.

1929

Edwin Hubble discovered that the universe is expanding and that the farther away a galaxy is, the faster it is moving away from us. Two years

later, Georges Lemaître suggests that the expansion can be traced to an initial “Big Bang”.

1930

By applying new ideas from subatomic physics, Subrahmanyan Chandrasekhar predicts that the atoms in a white dwarf star of more than 1.44 solar masses will

disintegrate, causing the star to collapse violently. In 1933, Walter Baade and Fritz Zwicky describe the neutron star that results from this collapse, causing a supernova explosion.

Clyde Tombaugh discovers the dwarf planet Pluto at the Lowell Observatory in Flagstaff, Arizona. The object is so faint and moving so slowly that he has to compare photos taken several nights apart.

1932

Karl Jansky detects the first radio waves coming from space. In 1942, radio waves from the Sun are detected. Seven years later radio astronomers identify the first distant source – the Crab Nebula, and the galaxies Centaurus A and M87.

1938

German physicist Hans Bethe explains how stars generate energy. He outlines a series of nuclear fusion reactions that turn hydrogen into helium and release enormous amounts of energy in a star’s core. These reactions use the star’s hydrogen very slowly, allowing it to burn for billions of years.

1944

A team of German scientists led by Wernher von Braun develops the V-2, the first rocket-powered ballistic

missile. Scientists and engineers from Braun’s team were captured at the end of World War II and drafted into the American and Russian rocket programs.

1948

The largest telescope in the world, with a 5.08m (200 in) mirror, is completed at Palomar Mountain in California. At the time, the telescope pushes single-mirror telescope technology to its limits – large mirrors tend to bend under their own weight.

1957

Russia launches the first artificial satellite, Sputnik 1, into orbit, beginning the space age. The US launches its first satellite, Explorer 1, four months later.

1958

(July 29) Beginning of the NASA (National Aeronautics and Space Administration), agency newly created by the United States to catch up with Soviet space technologies. It absorbs all research centers and staffs of the NACA (National Advisory Committee for Aeronautics), an organization founded in 1915.

1959

Russia and the US both launch probes to the Moon, but NASA’s Pioneer probes all failed. The Russian Luna program was more successful. Luna 2 crash-lands on the Moon’s surface in September, and Luna 3 returns the first pictures of the Moon’s farside in October.

1961

Russia takes the lead in the space race as Yuri Gagarin becomes the first person to orbit Earth in April. NASA astronaut Alan Shepard becomes the first American in space a month later, but does not go into orbit, although he is the first person to land with himself still inside his spacecraft and thus technically achieving the first complete human spaceflight by FAI definitions.[12] John Glenn achieves orbit in early 1962.

1962

Mariner 2 becomes the first probe to reach another planet, flying past Venus in December. NASA follows this with the successful Mariner 4 mission to Mars in 1965, both the US and Russia send many more probes to planets through the rest of the 1960s and 1970s.

1963

Dutch-American astronomer Maarten Schmidt measures the spectra of quasars, the mysterious star-like radio sources discovered in 1960. He establishes that quasars are active galaxies, and among the most distant objects in the universe.

1965

Arno Penzias and Robert Wilson announce the discovery of a weak radio signal coming from all parts of the sky. Scientists figure out that this must be emitted by an object at a temperature of -270 °C. Soon it is recognized as the remnant of the very hot radiation from the Big Bang that created the universe 13 billion years ago, see Cosmic microwave background. This

radio signal is emitted by the electron in hydrogen flipping from pointing up or down and is approximated to happen once in a million years for every particle. Hydrogen is present in interstellar space gas throughout the entire universe and most dense in nebulae which is where the signals originate. Even though the electron of hydrogen only flips once every million years the mere quantity of hydrogen in space gas makes the presence of these radio waves prominent.

1966

Russian Luna 9 probe makes the first successful soft landing on the Moon in January, while the US lands the far more complex Surveyor missions, which follows up to NASA’s Ranger series of crash-landers, scout sites for possible manned landings.

1967

Jocelyn Bell Burnell and Antony Hewish detected the first pulsar, an object emitting regular pulses of radio waves. Pulsars are eventually recognized as rapidly spinning neutron stars with intense magnetic fields – the remains of a supernova explosion.

1968

NASA’s Apollo 8 mission becomes the first human spaceflight mission to travel beyond Earth’s gravitational influence and to orbit another celestial body.

1969

The US wins the race for the Moon, as Neil Armstrong steps onto the lunar surface on July 20. Apollo 11 is followed by five further landing missions, three carrying a sophisticated lunar rover vehicle.

1970

The Uhuru satellite, designed to map the sky at X-ray wavelengths, is launched by NASA. The existence of X rays from the Sun and a few other stars has already been found using rocket-launched experiments, but Uhuru charts more than 300 X-ray sources, including several possible black holes.

1971

Russia launches its first space station, Salyut 1, into orbit. It is followed by a series of stations, culminating with Mir in 1986. A permanent platform in

orbit allows cosmonauts to carry out serious research and to set a series of new duration records for spaceflight.

1972

Charles Thomas Bolton was the first astronomer to present irrefutable evidence of the existence of a black hole.

1975

The Russian probe Venera 9 lands on the surface of Venus and sends back the first picture of its surface. The first probe to land on another planet, Venera 7 in 1970, had no camera. Both break down within an hour in the hostile atmosphere.

1976

Two NASA probes arrive at Mars. Each Viking mission consists of an orbiter, which photographs the planet from above, and a lander, which touches down on the surface, analyzes the rocks, and searches unsuccessfully for life.

1977

(August 20) The Voyager 2 space probe launched by NASA to study the Jovian system, Saturnian system, Uranian system, Neptunian system, the Kuiper belt, the heliosphere and the interstellar space. (September 5) The Voyager 1 space probe launched by NASA to study the Jovian system, Saturnian system and the interstellar medium.

1981

Columbia, the first of NASA’s reusable space shuttles, makes its maiden flight, ten years in development, the shuttle will make space travel routine and eventually open the path for a new International Space Station.

1983

The first infrared astronomy satellite, IRAS, is launched. It must be cooled to extremely low temperatures with liquid helium, and it operates for only 300 days before the supply of helium is exhausted. During this time it completes an infrared survey of 98% of the sky.

1986

NASA’s spaceflight program comes to a halt when Space Shuttle Challenger explodes shortly after launch. A thorough inquiry and modifications to the rest of the fleet kept the shuttles on the ground for nearly three years.

The returning Halley’s comet is met by a fleet of five probes from Russia, Japan, and Europe. The most ambitious is the European Space Agency’s Giotto spacecraft, which flies through the comet’s coma and photographs the nucleus.

1990

The Magellan probe, launched by NASA, arrives at Venus and spends three years mapping the planet with radar. Magellan is the first in a new wave of probes that include Galileo, which arrives at Jupiter in 1995, and Cassini which arrives at Saturn in 2004.

The Hubble Space Telescope, the first large optical telescope in orbit, is launched using the Space Shuttle, but astronomers soon discovered that it is crippled by a problem with its mirror. A complex repair mission in 1993 allows the telescope to start producing spectacular images of distant stars, nebulae, and galaxies.

1992

The Cosmic Background Explorer satellite produces a detailed map of the background radiation remaining from the Big Bang. The map shows “ripples”, caused by slight variations in the density of the early universe – the seeds of galaxies and galaxy clusters.

The 10 meter Keck telescope on Mauna Kea, Hawaii, is completed. The first revolutionary new wave of

telescopes, the Keck’s main mirror is made of 36 six- sided segments, with computers to control their alignment. New optical telescopes also make use of interferometry – improving resolution by combining images from separate telescopes.

1998

Construction work on a huge new space station named ISS has begun. A joint venture between many countries, including former space rivals Russia and the US.

2005

Mike Brown and his team discovered a large body in the outer solar system.[13] It was temporarily named as (2003) UB313. Initially, it appeared larger than Pluto, and was called tenth planet.[14]

2006

International Astronomical Union (IAU) adopted a new definition of planet. A new distinct class of objects called dwarf planets was also decided. Pluto was redefined as a dwarf planet along with Ceres and Eris, formerly known

as (2003) UB313. Eris was named after the IAU General Assembly in 2006.

[15][16]

2012

(May 2) First visual proof of existence of black holes is published. Suvi Gezari’s team in Johns Hopkins University, using the Hawaiian telescope Pan-STARRS 1, record images of a supermassive black hole 2.7 million light-years away that is swallowing a red giant.[17]

2013

In October 2013, the first extrasolar asteroid is detected around white dwarf star GD 61. It is also the first

detected extrasolar body which contains water in liquid or solid form.[18][19][20]

2015

In July 14, with the successful encounter of Pluto by NASA’s New Horizons spacecraft, the United States became the first nation to explore all of 9 major planets recognized in 1981. Later in September 14, LIGO was the first to directly detect gravitational waves.

                                TIMELINE OF SPACE EXPLORATION 

This is for a timeline of space exploration including notable achievements and first accomplishments in humanity’s exploration of outer space.

1610-1951

Date
Event leading to space exploration
Country
Researcher(s)
1610
First telescopic observation of the night sky: Discovery of Jupiter’s moons, lunar craters and the phases of Venus.

Republic of Venice

Galileo Galilei

1687
Publication of the Philosophiæ Naturalis Principia Mathematica 

England
Sir Isaac Newton

1813
First exposition of the rocket equation based on Newton’s third law of motion: Treatise on the Motion of Rockets 

UK William Moore

1840
First clear telescopic photograph of another world: the Moon.

United States John William Draper

1865
From the Earth to the Moon published.

France Jules Verne

1898
The War of the Worlds published. This inspired Robert Goddard to investigate rocketry.

UK
H. G. Wells

1903
Inspired by the writings of Jules Verne, first serious work published that showed physical space exploration was theoretically possible: Исследование мировых пространств реактивными приборами (The Exploration of Cosmic Space by Means of Reaction Devices)

Russia
Konstantin Tsiolkovsky
1914
Goddard files for and is subsequently awarded U.S. patents on multistage and liquid-fueled rockets

United States

Robert H. Goddard

1919
Goddard’s widely influential paper “A Method of Reaching Extreme Altitudes” discussed solid- and liquid-fueled rocketry

United States

Robert H. Goddard

15 December 1923
Die Rakete zu den Planetenräumen (“By Rocket into Planetary Space”) self-published after its rejection as a doctoral thesis.

Germany Hermann Oberth

1924
Society for Studies of Interplanetary Travel founded

USSR
Members include Konstantin Tsiolkovsky, Friedrich Zander, Yuri Kondratyuk
16 March 1926
Goddard launches the first liquid-fueled rocket

United States

Robert H. Goddard

1927
Verein für Raumschiffahrt (Society for Space Travel) formed; it includes many top European rocket scientists.

Germany

1927

The Conquest of Interplanetary Space discusses rocket mechanics and orbital effects including the gravitational slingshot

USSR

Yuri Kondratyuk

1928

Das Problem der Befahrung des Weltraums – der Raketen-Motor (The Problem of Space Travel – The Rocket Motor) discusses space travel and its potential uses for scientific experiments.

Germany
Herman Potočnik
1929
Oberth, with students including Wernher von Braun, launches his first liquid-fueled rocket

Germany

Hermann Oberth

1931
First German military liquid-fueled rocket engines developed

Germany

Walter Riedel

1933
Work begins on the Aggregate series of rockets which leads to the V-2 rocket.

Nazi Germany

Wernher von Braun

17 August 1933
Group for the Study of Reactive Motion (GIRD) launches the first Soviet liquid-fueled rocket

USSR
Sergey Korolev (group leader), Friedrich Zander (designer)

1935
Graduate student Frank Malina under his professor Theodore von Kármán begins work on a sounding rocket

United States

Frank Malina

20 June 1944
V-2 Rocket (MW 18014): First man-made object to cross what would later be defined as the Kármán line and hence first spaceflight in history.

Nazi Germany

Wehrmacht

10 May 1946
First space research flight (cosmic radiation experiments)

United States
captured and improved V-2 rocket

22 May 1946
First U.S.-designed rocket to reach edge of space (80 km (49 mi))

United States

WAC Corporal

24 October 1946
First pictures of Earth from 105 km (65 mi) [1][2]

United States

V-2

20 February 1947
First animals in space (fruit flies) [1][3]

United States

V-2

22 July 1951
First dogs in space (Dezik and Tsygan) [4]

USSR

R-1

1957–1959

Date
Mission Achievements Country/Organization
Mission Name
21 August 1957
First intercontinental ballistic missile (ICBM)

USSR
R-7 Semyorka/SS-6 Sapwood

4 October 1957
First artificial satellite
First signals from space

USSR

Sputnik 1

3 November 1957
First animal in orbit, the dog Laika

USSR

Sputnik 2

31 January 1958
Confirmed the existence of the Van Allen belts

USA (ABMA) Explorer 1

2 January 1959
First firing of a rocket in Earth orbit
First reaching Earth escape velocity or Trans Lunar Injection
First detection of solar wind

USSR

Luna 1

4 January 1959
First artificial satellite to reach the Moon vicinity and first artificial satellite in heliocentric orbit

USSR

Luna 1

7 August 1959
First photograph of Earth from orbit

USA (NASA) Explorer 6

13 September 1959
First impact into another world (the Moon)
First delivery of national (USSR) pennants to a celestial body

USSR

Luna 2

4 October 1959
First photos of another world from space: The far side of the Moon

USSR

Luna 3

1960–1969

Date
Mission Success Country/Organization Mission Name
March 1960
First solar probe.

USA (NASA)

Pioneer 5

19 August 1960
First plants and animals to return alive from Earth orbit

USSR

Sputnik 5

10 October 1960
First probe launched to Mars (failed to reach target)

USSR

Mars 1M

31 January 1961
First Hominidae in space, first tasks performed in space; Ham (chimpanzee).

USA (NASA)

M-R 2

12 February 1961
First launch from Earth orbit of upper stage into a heliocentric orbit
First mid-course corrections
First spin-stabilisation

USSR

Venera 1

12 April 1961
First human spaceflight–(Yuri Gagarin) First human-crewed orbital flight

USSR

Vostok 1

5 May 1961
First human-piloted space flight–(Alan Shepard)
First human-crewed suborbital flight
First human space mission that landed with pilot still in spacecraft, thus the first complete human spaceflight by FAI definitions.[5]

USA

Freedom 7 

19 May 1961
First planetary flyby (within 100,000 km of Venus – no data returned)

USSR

Venera 1

7 March 1962
First orbital solar observatory

USA (NASA)

OSO-1

26 April 1962
First spacecraft to impact the far side of the Moon[6]

USA (NASA)

Ranger 4

November 1962
First Mars flyby (11,000 km) but contact was lost

USSR

Mars 1

14 December 1962
First successful planetary flyby (Venus closest approach 34,773 kilometers)

USA (NASA)

Mariner 2

16 June 1963
First woman in space (Valentina Tereshkova)

USSR

Vostok 6

19 July 1963
First reusable crewed spacecraft (suborbital)

USA (NASA)

X-15 Flight 90

18 March 1965
First extra-vehicular activity-(Alexei Leonov)

USSR

Voskhod 2

March 1965
First crewed spacecraft to change orbit

USA (NASA)

Gemini 3

14 July 1965
First Mars flyby (closest approach 9,846 kilometers; returned pictures)

USA (NASA)

Mariner 4

14 July 1965
First close-up photographs of another planet: Mars

USA (NASA)

Mariner 4

15 December 1965
First orbital rendezvous (parallel flight, no docking)

USA (NASA)
Gemini 6A/Gemini 7
3 February 1966
First soft landing on another world (the Moon) First photos from another world

USSR

Luna 9

1 March 1966
First impact into another planet (Venus)

USSR

Venera 3

16 March 1966
First orbital docking between two spacecraft

USA (NASA)
Gemini 8/Agena target vehicle

3 April 1966
First artificial satellite around another world (the Moon)

USSR

Luna 10

August 1966
First probe to map the Moon

USA

Lunar Orbiter 1

30 October 1967
First automated (crewless) docking

USSR
Cosmos 186/Cosmos 188

September 1968
First animals and plants to orbit moon, and the first to return safely to Earth

USSR

Zond 5

7 December 1968
First orbital ultraviolet observatory

USA (NASA)

OAO-2

21 December 1968
First piloted orbital mission of another celestial body (Moon),
First-ever Trans-Earth injection
First human space mission to escape Earth’s influence(25 December)

USA (NASA)

Apollo 8

January 1969
First docking between two crewed spacecraft in Earth orbit, also the first crew exchange in space

USSR
Soyuz 4 and Soyuz 5

January 1969
First to parachute in Venus’s atmosphere, lost contact before landing.

USSR

Venera 5

20 July 1969
First human on the Moon, and first space launch from a celestial body other than the Earth
First sample return from the Moon

USA (NASA)

Apollo 11

August 4, 1969
First photograph of Phobos from Space

USA (NASA)

Mariner 7

19 November 1969
First rendezvous on the surface of a celestial body

USA (NASA) Apollo 12/Surveyor 3

1970–1980

Date
Mission Success
Country/Organization
Mission Name
24 September 1970
First automatic sample return from the Moon

USSR

Luna 16

17 November 1970 First lunar rover

USSR

Lunokhod 1 

12 December 1970
First X-ray orbital observatory

USA (NASA)

Uhuru (satellite)

15 December 1970
First soft landing on another planet (Venus) First signals from another planet

USSR

Venera 7

19 April 1971
First space station

USSR

Salyut 1

June 1971
First Manned orbital observatory

USSR

Orion 1

14 November 1971
First to maintain orbit around another planet (Mars)

USA (NASA)

Mariner 9

27 November 1971 First impact into Mars

USSR

Mars 2

2 December 1971
First soft Mars landing
First signals from Mars surface

USSR

Mars 3

3 March 1972
First human made object sent on escape trajectory away from the Sun

USA (NASA)

Pioneer 10 

15 July 1972
First mission to enter the asteroid belt and leave inner Solar System

USA (NASA)

Pioneer 10 

15 November 1972
First orbital gamma ray observatory

USA (NASA)

SAS 2

3 December 1973
First Jupiter flyby (at 130,000 km)

USA (NASA)

Pioneer 10 

5 February 1974
Venus flyby at 5768 kilometers, first gravitational assist manoeuvre
First photograph of Venus from Space

USA (NASA)

Mariner 10

29 March 1974
First Mercury flyby at 703 kilometers

USA (NASA)

Mariner 10

15 July 1975
First multinational manned mission

USSR USA (NASA)

Apollo-Soyuz Test Project

20 October 1975
First orbit around Venus

USSR

Venera 9

22 October 1975
First photos from the surface of another planet (Venus)

USSR

Venera 9

17 April 1976
Closest flyby of the Sun (43.432 million kilometers) Maximum speed record among spacecraft (252,792 km/h)

USA (NASA) West Germany (DFVLR) Helios 2 

20 July 1976
First photos and soil samples from the surface of Mars

USA (NASA)

Viking Lander

26 January 1978
First real time remotely operated ultraviolet orbital observatory

USA (NASA) ESA UK (SERC) International Ultraviolet Explorer

4 December 1978
First extended (multi-year) orbital exploration of Venus from 1978 to 1992

USA (NASA)

Pioneer Venus Orbiter

5 March 1979
Jupiter flyby (closest approach 349,000 km) encounters with Five Jovian moons, discovery of volcanism on Io

USA (NASA)

Voyager 1 

1 September 1979
First Saturn flyby at 21,000 km, first photographs of Titan from Space

USA (NASA)

Pioneer 11 

12 November 1980
Saturn flyby (closest approach 124,000 kilometers), close encounter of Titan and encounters with a dozen others.

USA (NASA)

Voyager 1 

1981–Present

Date
Mission Success
Country/Organization
Mission Name
12 April 1981
First Reusable manned spacecraft (orbital)

USA (NASA)

STS-1

1 March 1982
First Venus soil samples and sound recording of another world

USSR

Venera 13

25 January 1983
First Infrared orbital observatory

USA (NASA) UK (SERC) Netherlands (NIVR) IRAS

13 June 1983
First spacecraft beyond the orbit of Neptune (first spacecraft to pass beyond all Solar System planets)

USA (NASA)

Pioneer 10 

7 February 1984
First untethered spacewalk, Bruce McCandless II

USA (NASA)

STS-41-B

24 January 1986
First Uranus flyby (closest approach 81,500 kilometers (44,000 nmi)

USA (NASA)

Voyager 2 

28 January 1986
Challenger explosion with Christa McAuliffe (teacher at high school in Concord, New Hampshire)

USA (NASA)

STS-51-L

19 February 1986
First consistently inhabited long-term research space station

USSR

Mir

8 August 1989
First astrometric satellite

ESA

Hipparcos

25 August 1989
First Neptune flyby (closest approach at 29,240 km)

USA (NASA)

Voyager 2 

18 November 1989
First orbital cosmic microwave observatory

USA (NASA)

COBE

14 February 1990

First photograph of the whole Solar System

USA (NASA)

Voyager 1 

24 April 1990
Optical orbital observatory

USA (NASA) ESA

Hubble Space Telescope

15 September 1990
Extended (multi-year) orbital exploration of Venus

USA (NASA)

Magellan 

21 October 1991
First asteroid flyby (951 Gaspra closest approach 1,600 kilometers)

USA (NASA)

Galileo 

8 February 1992
First polar orbit around the Sun

USA (NASA) ESA

Ulysses 

22 March 1995
Record longest duration spaceflight (437.7 days) set by Valeri Polyakov

Russia (FKA) Mir

7 December 1995 First orbit of Jupiter

USA (NASA)

Galileo 

7 December 1995
First mission into the atmosphere of a gas giant (Jupiter)

USA (NASA)

Galileo‘s atmospheric entry probe 12 February 1997
First orbital radio observatory

Japan (ISAS) HALCA

4 July 1997
First operational rover on another planet (Mars)

USA (NASA)

Mars Pathfinder

20 November 1998
First multinational space station,
Largest man-made object built in space to date

Russia(FKA) USA (NASA) Europe (ESA) Japan (JAXA) Canada (CSA)
International Space Station

14 February 2000
First orbiting of an asteroid (433 Eros)

USA (NASA) ESA

NEAR Shoemaker 

12 February 2001
First landing on an asteroid (433 Eros)

USA (NASA)

NEAR Shoemaker 

1 July 2004
First orbit of Saturn

USA (NASA)

Cassini–Huygens 

ESA Italy (ASI)

8 September 2004
First sample return beyond lunar orbit (solar wind)

USA (NASA)

Genesis 

14 January 2005
First soft landing on Titan

ESA USA (NASA) Italy (ASI)

Cassini–Huygens 

19 November 2005
First asteroid ascent (25143 Itokawa)
First interplanetary escape without undercarriage cutoff

Japan (JAXA) Hayabusa 

15 January 2006
First sample return from comet (81P/Wild)

USA (NASA)

Stardust 

6 March 2009
Kepler Mission is launched, first space telescope designated to search for Earth-like exoplanets[8]

USA (NASA)

Kepler Mission

13 June 2010
First sample return from asteroid (25143 Itokawa)

Japan (JAXA)

Hayabusa 

18 March 2011
First orbit of Mercury

USA (NASA)

MESSENGER 

16 July 2011
First orbit of giant asteroid Vesta

USA (NASA)

Dawn 

25 August 2012
First manmade probe in interstellar space.

USA (NASA)

Voyager 1 

12 November 2014
First man-made probe to make a planned and soft landing on a comet (67P/Churyumov–Gerasimenko).

ESA

Rosetta 

6 March 2015
First orbit of dwarf planet (Ceres).
First spacecraft to orbit two separate celestial bodies.

USA (NASA)

Dawn 

July 2015
First flyby of dwarf planet (Pluto).
Last original encounter with one of the nine major planets recognized in 1981.

USA (NASA)

New Horizons 

10 August 2015
Lettuce was the first food eaten that was grown in space.

USA (NASA) Japan (JAXA)

1 March 2016
Astronaut Scott Kelly and Cosmonaut Mikhail Kornienko return to Earth after their 340-day space mission, longest recorded time in space for ISS crew members.

USA (NASA) Russia(FKA)

ISS year long mission

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