- Timeline of solar system astronomy
Timeline ofsolar system astronomy Antiquity
* 2137 BC,
October 22 - Chinese astronomers record asolar eclipse
*ca.2000 BC - Chinese determine thatJupiter needs 12 years to complete one revolution of its orbit.
* 2nd millennium BC - earliest possible date for the composition of the BabylonianVenus tablet of Ammisaduqa , a7th century BC copy of a list of observations of the motions of the planet Venus, and the oldest planetary table currently known.
* 1000s BC - The idea of a heliocentric solar system, with theSun at the center, is possibly first suggested in the Vedic literature of ancient India, which often refer to the Sun as the "centre of spheres".
*ca.1400 BC - Chinese record the regularity of solar andlunar eclipse s and the earliest knownSolar prominence
*ca.1100 BC - Chinese first determine thespring equinox .
*776 BC - Chinese make the earliest reliable record ofsolar eclipse .
* 600s BC - Egyptian astronomers alleged to have predicted a solar eclipse
*613 BC , July - AComet , possiblyComet Halley , is recorded inSpring and Autumn Annals by the Chinese
*586 BC - Thales of Miletus alleged to have predicted a solar eclipse
*350 BC -Aristotle argues for a sphericalEarth usinglunar eclipse s and other observations
*280 BC -Aristarchus of Samos uses the size of the Earth'sshadow on theMoon to estimate that the Moon's radius is one-third that of the Earth, and to estimate sizes and distances for the Moon and Sun
*200 BC -Eratosthenes uses shadows to determine that the radius of the Earth is roughly 6,400 km
*150 BC -Hipparchus usesparallax to determine that the distance to the Moon is roughly 380,000 km
*134 BC - Hipparchus discovers theprecession of theequinox es
*28 BC - Chinese history bookBook of Han makes earliest known dated record ofsunspot .
*c. 150 CE -Claudius Ptolemy completes hisAlmagest that codifies the astronomical knowledge of his time and cements the geocentric model in the WestMiddle Ages
* 499 CE - The Indian astronomer-mathematician,
Aryabhata , in his "Aryabhatiya ", propounds a possibly heliocentric solar system ofgravitation , and an eccentric epicyclic model of the planets, where the planets follow elliptical orbits around the Sun, and the Moon and planets shine by reflected sunlight
*500 - Aryabhata accurately computes the Earth'scircumference , the solar and lunar eclipses, and the length of Earth's revolution around the Sun
*620s - Indian mathematician-astronomerBrahmagupta recognizes gravity as a force of attraction, and briefly describes a law ofgravitation
*628 - Brahmagupta 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
*687 - Chinese make earliest known record ofmeteor shower
* 800s - The eldestBanū Mūsā brother,Ja'far Muhammad ibn Mūsā ibn Shākir , hypothesizes that the heavenly bodies andcelestial spheres are subject to the same laws of physics asEarth , and proposes that there is aforce of attraction between heavenly bodies
*820 -Muhammad ibn Musa al-Khwarizmi composes his astronomical tables, utilising Hindu-Arabic numerals in his calculations
*850 -Ahmad ibn Muhammad ibn Kathīr al-Farghānī (Alfraganus) gives values for the obliquity of theecliptic , the precessional movement of the apogees of theSun
* 900s -Muhammad ibn Jābir al-Harrānī al-Battānī (Albatenius) discovers that the direction of the Sun's eccentricity is changing, which in modern astronomy is equivalent to theEarth moving in anelliptic orbit around the Sun
* 900s -Ibn Yunus observes more than 10,000 entries for the Sun's position for many years using a largeastrolabe with a diameter of nearly 1.4 metres
*1019 -Abū Rayhān al-Bīrūnī observes and describes thesolar eclipse on April 8 and thelunar eclipse on September 17 in detail, and gives the exact latitudes of the stars during the lunar eclipse
*1021 -Ibn al-Haytham (Alhacen), in his "Book of Optics ", discovers that thecelestial spheres do not consist ofsolid matter, and he also discovers that the heavens are less dense than the air
*1031 -Abū al-Rayhān al-Bīrūnī calculates the distance between the Earth and the Sun in his "Canon Mas’udicus"
*1150 - Indian mathematician-astronomerBhaskara , in the "Siddhanta Shiromani", calculates thelongitude s andlatitude s of the planets, lunar and solar eclipses,rising s and settings, the Moon'slunar crescent , syzygies, and conjunctions of the planets with each other and with the fixedstars , and explains the three problems of diurnal rotation
*1150s - Bhaskara calculates the planetarymean motion , ellipses, first visibilities of the planets, the lunar crescent, theseasons , and the length of the Earth's revolution around the Sun to 9 decimal places.
*1150s -Gerard of Cremona translates Ptolemy's "Almagest " fromArabic intoLatin , eventually leading to its adoption by the Catholic Church as an approved text.
* ~1350 -Ibn al-Shatir anticipates Copernicus by abandoning theequant of Ptolemy in his calculations of planetary motion, and he provides the firstempirical model of lunar motion which accurately matchobservation sRenaissance
* a.
1514 -Nicolaus Copernicus states his heliocentric theory in "Commentariolus "
*1543 - Nicolaus Copernicus publishes his heliocentric theory in "De revolutionibus orbium coelestium "
*1577 -Tycho Brahe uses parallax to prove thatcomet s are distant entities and not atmospheric phenomena
*1609 -Johannes Kepler states his first two empirical laws of planetary motion, stating that the orbits of the planets are elliptical rather than circular, and thus resolving many ancient problems with planetary models.
*1610 -Galileo Galilei discovers Callisto, Europa, Ganymede, and Io, seesSaturn 'splanetary ring s (but does not recognize that they are rings), and observes thephases of Venus , disproving the Ptolemaic system, though not thegeocentric model
*1619 - Johannes Kepler states his third empirical law of planetary motion
*1655 -Giovanni Domenico Cassini discoversJupiter 'sGreat Red Spot
*1656 -Christiaan Huygens identifies Saturn's rings as rings and discovers Titan
*1665 - Cassini determines the rotational speeds of Jupiter,Mars , andVenus
*1672 - Cassini discovers Rhea
*1672 -Jean Richer and Cassini measure theastronomical unit to be about 138,370,000 km
*1675 -Ole Rømer uses the orbital mechanics of Jupiter's moons to estimate that thespeed of light is about 227,000 km/sEighteenth century
*
1705 -Edmund Halley publicly predicts the periodicity ofHalley's Comet and computes its expected path of return in1757
*1715 - Edmund Halley calculates the shadow path of a solar eclipse
*1716 - Edmund Halley suggests a high-precision measurement of the Sun-Earth distance by timing thetransit of Venus
*1729 -James Bradley determines the cause of theaberration of starlight , providing the first direct evidence of the Earth's motion
*1755 -Immanuel Kant first formulates thenebular hypothesis of solar system formation.
*1758 -Johann Palitzsch observes the return of Halley's comet. The interference of Jupiter's orbit had slowed the return by 618 days. Parisian astronomerLa Caille suggests it should be namedHalley's comet .
*1766 -Johann Titius finds the Titius-Bode rule for planetary distances
*1772 -Johann Bode publicizes the Titius-Bode rule for planetary distances
*1781 -William Herschel discoversUranus during a telescopic survey of the northern sky
*1796 -Pierre Laplace re-states the nebular hypothesis for the formation of the solar system from a spinningnebula of gas and dustNineteenth century
*
1801 -Giuseppe Piazzi discovers theasteroid Ceres
*1802 -Heinrich Wilhelm Olbers discovers the asteroid Pallas
*1821 -Alexis Bouvard detects irregularities in theorbit of Uranus
*1825 - Pierre Laplace completes his study ofgravitation , thestability of the solar system , tides, the precession of the equinoxes, thelibration of the Moon, and Saturn's rings in "Mécanique Celeste "
*1838 -Friedrich Wilhelm Bessel measures theparallax of the star61 Cygni , refuting one of the oldest arguments againstheliocentrism .
*1843 - John Adams predicts the existence and location ofNeptune from irregularities in the orbit of Uranus
*1846 -Urbain Le Verrier predicts the existence and location of Neptune from irregularities in the orbit of Uranus
*1846 -Johann Galle discovers Neptune
*1846 -William Lassell discovers Triton
*1849 -Édouard Roche finds the limiting radius of tidal destruction and tidal creation for a body held together only by its self gravity, called theRoche limit , and uses it to explain why Saturn's rings do not condense into a satellite
*1856 -James Clerk Maxwell demonstrates that a solid ring around Saturn would be torn apart by gravitational forces and argues that Saturn's rings consist of a multitude of tiny satellites
*1862 - By analysing thespectroscopic signature of the Sun and comparing it to those of other stars, FatherAngelo Secchi determines that the Sun is itself a star.
*1866 -Giovanni Schiaparelli realizes thatmeteor streams occur when the Earth passes through the orbit of a comet that has left debris along its pathTwentieth century
*
1906 -Max Wolf discovers theTrojan asteroid Achilles
*1930 -Clyde Tombaugh discoversPluto
*1930 -Seth Nicholson measures the surface temperature of the Moon
*1944 -Gerard Kuiper discovers that the satellite Titan has a substantial atmosphere
*1950 -Jan Oort suggests the presence of a cometaryOort cloud
*1951 -Gerard Kuiper argues for an annular reservoir of comets between 40-100 astronomical units from the Sun, theKuiper belt
*1959 -Luna 3 sends a picture of the far side of theMoon
*1977 -James Elliot discovers the rings of Uranus during a stellar occultation experiment on theKuiper Airborne Observatory
*1978 -James Christy discovers Charon
*1978 -Peter Goldreich andScott Tremaine present aBoltzmann equation model of planetary-ring dynamics for indestructible spherical ring particles that do not self-gravitate and find a stability requirement relation between ring optical depth and particle normal restitution coefficient
*1988 -Martin Duncan ,Thomas Quinn , andScott Tremaine demonstrate that short-period comets come primarily from the Kuiper Belt and not the Oort cloud
*1992 - Firstplanetary system beyond our own Solar System detected, around thepulsar PSR B1257+12
*1992 -David Jewitt andJane Luu of theUniversity of Hawaii discover mpl|(15760) 1992 QB|1, the first object deemed to be a member of theKuiper belt
*1995 - The first planet around a Sun-like star is discovered, in orbit around the star51 Pegasi .Twenty-first century
*
2004 - Sedna, a large object with an unprecedented 12,000 year orbit, is discovered byMichael E. Brown ,Chad Trujillo , andDavid L. Rabinowitz .
*2005 -Michael E. Brown "et al." discover Eris, aTrans-Neptunian object larger thanPluto , and later also its moon, Dysnomia. Eris was first imaged in2003 See also
*
Timeline of Solar System exploration
*Timeline of Solar System object discoveries
*Timeline of Chinese astronomy
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