Timeline of solar system astronomy
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Timeline of solar system astronomy
Contents |
[edit] Antiquity
- 2137 BC, October 22 - Chinese astronomers record a solar eclipse
- ca. 2000 BC - Chinese determine that Jupiter needs 12 years to complete one revolution of its orbit.
- 2nd millennium BC - earliest possible date for the composition of the Babylonian Venus tablet of Ammisaduqa, a 7th 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 the Sun 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 and lunar eclipses and the earliest known Solar prominence
- ca. 1100 BC - Chinese first determine the spring equinox.
- 776 BC - Chinese make the earliest reliable record of solar eclipse.
- 600s BC - Egyptian astronomers alleged to have predicted a solar eclipse
- 613 BC, July - A Comet, possibly Comet Halley, is recorded in Spring and Autumn Annals by the Chinese
- 586 BC - Thales of Miletus alleged to have predicted a solar eclipse
- 350 BC - Aristotle argues for a spherical Earth using lunar eclipses and other observations
- 280 BC - Aristarchus of Samos uses the size of the Earth's shadow on the Moon 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 uses parallax to determine that the distance to the Moon is roughly 380,000 km
- 134 BC - Hipparchus discovers the precession of the equinoxes
- 28 BC - Chinese history book Book of Han makes earliest known dated record of sunspot.
- c. 150 CE - Claudius Ptolemy completes his Almagest that codifies the astronomical knowledge of his time and cements the geocentric model in the West
[edit] Middle Ages
- 499 CE - The Indian astronomer-mathematician, Aryabhata, in his Aryabhatiya, propounds a possibly heliocentric solar system of gravitation, 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's circumference, the solar and lunar eclipses, and the length of Earth's revolution around the Sun
- 620s - Indian mathematician-astronomer Brahmagupta recognizes gravity as a force of attraction, and briefly describes a law of gravitation
- 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 of meteor shower
- 800s - The eldest Banū Mūsā brother, Ja'far Muhammad ibn Mūsā ibn Shākir, hypothesizes that the heavenly bodies and celestial spheres are subject to the same laws of physics as Earth, and proposes that there is a force 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 the ecliptic, the precessional movement of the apogees of the Sun
- 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 the Earth moving in an elliptic orbit around the Sun
- 900s - Ibn Yunus observes more than 10,000 entries for the Sun's position for many years using a large astrolabe with a diameter of nearly 1.4 metres
- 1019 - Abū Rayhān al-Bīrūnī observes and describes the solar eclipse on April 8 and the lunar 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 the celestial spheres do not consist of solid 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-astronomer Bhaskara, in the 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
- 1150s - Bhaskara 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.
- 1150s - Gerard of Cremona translates Ptolemy's Almagest from Arabic into Latin, eventually leading to its adoption by the Catholic Church as an approved text.
- ~1350 - Ibn al-Shatir anticipates Copernicus by abandoning the equant of Ptolemy in his calculations of planetary motion, and he provides the first empirical model of lunar motion which accurately match observations
[edit] Renaissance
- 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 that comets 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, sees Saturn's planetary rings (but does not recognize that they are rings), and observes the phases of Venus, disproving the Ptolemaic system, though not the geocentric model
- 1619 - Johannes Kepler states his third empirical law of planetary motion
- 1655 - Giovanni Domenico Cassini discovers Jupiter's Great Red Spot
- 1656 - Christiaan Huygens identifies Saturn's rings as rings and discovers Titan
- 1665 - Cassini determines the rotational speeds of Jupiter, Mars, and Venus
- 1672 - Cassini discovers Rhea
- 1672 - Jean Richer and Cassini measure the astronomical unit to be about 138,370,000 km
- 1675 - Ole Rømer uses the orbital mechanics of Jupiter's moons to estimate that the speed of light is about 227,000 km/s
[edit] Eighteenth century
- 1705 - Edmund Halley publicly predicts the periodicity of Halley's Comet and computes its expected path of return in 1757
- 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 the transit of Venus
- 1729 - James Bradley determines the cause of the aberration of starlight, providing the first direct evidence of the Earth's motion
- 1755 - Immanuel Kant first formulates the nebular 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 astronomer La Caille suggests it should be named Halley'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 discovers Uranus 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 spinning nebula of gas and dust
[edit] Nineteenth century
- 1801 - Giuseppe Piazzi discovers the asteroid Ceres
- 1802 - Heinrich Wilhelm Olbers discovers the asteroid Pallas
- 1821 - Alexis Bouvard detects irregularities in the orbit of Uranus
- 1825 - Pierre Laplace completes his study of gravitation, the stability of the solar system, tides, the precession of the equinoxes, the libration of the Moon, and Saturn's rings in Mécanique Celeste
- 1838 - Friedrich Wilhelm Bessel measures the parallax of the star 61 Cygni, refuting one of the oldest arguments against heliocentrism.
- 1843 - John Adams predicts the existence and location of Neptune 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 the Roche 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 the spectroscopic signature of the Sun and comparing it to those of other stars, Father Angelo Secchi determines that the Sun is itself a star.
- 1866 - Giovanni Schiaparelli realizes that meteor streams occur when the Earth passes through the orbit of a comet that has left debris along its path
[edit] Twentieth century
- 1906 - Max Wolf discovers the Trojan asteroid Achilles
- 1930 - Clyde Tombaugh discovers Pluto
- 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 cometary Oort cloud
- 1951 - Gerard Kuiper argues for an annular reservoir of comets between 40-100 astronomical units from the Sun, the Kuiper belt
- 1959 - Luna 3 sends a picture of the far side of the Moon
- 1977 - James Elliot discovers the rings of Uranus during a stellar occultation experiment on the Kuiper Airborne Observatory
- 1978 - James Christy discovers Charon
- 1978 - Peter Goldreich and Scott Tremaine present a Boltzmann 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
- 1979 - Voyager 1 discovers Jupiter's faint ring system, and the volcanoes on Io.
- 1980 - Voyager 1 discovers two new satellites of Jupiter, and six new satellites of Saturn.
- 1986 - Voyager 2 Uranus flyby; first closeup images of surface features, rings and moons, plus ten new satellites discovered.
- 1988 - Martin Duncan, Thomas Quinn, and Scott Tremaine demonstrate that short-period comets come primarily from the Kuiper Belt and not the Oort cloud
- 1989 - Voyager 2 Neptune flyby: first observations of surface features; arclike nature of rings determined; Triton imaged for the first time; five new satellites discovered.
- 1992 - First planetary system beyond our own Solar System detected, around the pulsar PSR B1257+12
- 1992 - David Jewitt and Jane Luu of the University of Hawaii discover (15760) 1992 QB1, the first object deemed to be a member of the Kuiper belt
- 1995 - The first planet around a Sun-like star is discovered, in orbit around the star 51 Pegasi.
[edit] Twenty-first century
- 2004 - Sedna, a large object with an unprecedented 12,000 year orbit, is discovered by Michael E. Brown, Chad Trujillo, and David L. Rabinowitz.
- 2005 - The Cassini spacecraft and Huygens probe provide the first images of the surface of Saturn's moon Titan. Cassini also reveals cryovolcanism on Saturn's moon Enceladus and a strange equatorial ridge on the smaller moon Iapetus
- 2005 - Michael E. Brown et al. discover Eris, a Trans-Neptunian object larger than Pluto, and later also its moon, Dysnomia. Eris was first imaged in 2003
