An asteroid is a minor planet orbiting within the inner Solar System or co-orbital with Jupiter, larger than a meteoroid but not a planet or identified comet. Asteroids are atmosphere-less, rocky, metallic, or icy bodies, classified as C-type (carbonaceous), M-type (metallic), or S-type (silicaceous). Their sizes and shapes vary considerably, from small rubble piles to Ceres, a dwarf planet nearly 1000 km in diameter. An object is classified as a comet if it exhibits a coma (tail) when warmed by solar radiation, blurring the lines between the two.
In 1914, asteroid designations included year plus a Greek letter.
In 1918, Kiyotsugu Hirayama first recognized Main belt families and are often called Hirayama families in his honor.
In 1925, a simple chronological numbering system for asteroids was established.
In 1937, asteroid 69230 Hermes approached within 0.005 AU of Earth, leading astronomers to realize the potential for Earth impacts.
In 1967, "Project Icarus" was designed as a contingency plan in case of collision with asteroid 1566 Icarus, using Saturn V rockets with nuclear warheads to deflect or destroy the asteroid.
In 1975, Chapman, Morrison, and Zellner developed an asteroid taxonomic system based on color, albedo, and spectral shape.
In 1977, astronomers discovered 2060 Chiron, the first small body that permanently resided further out than Jupiter.
In 1979, the first active asteroid, 7968 Elst–Pizarro, was initially discovered as an asteroid.
In 1984, David J. Tholen proposed the Tholen classification of asteroids, based on data collected from an eight-color asteroid survey performed in the 1980s, resulting in 14 asteroid categories.
In 1990, the Acfer 049 meteorite was discovered in Algeria.
In 1991, 951 Gaspra became the first asteroid to be photographed in close-up by the Galileo probe.
In 1992, 15760 Albion was discovered, it was the first object found beyond the orbit of Neptune, excluding Pluto.
In 1993, the Galileo probe imaged 243 Ida and its moon Dactyl.
In 1996, Eric Elst and Guido Pizarro found that 7968 Elst-Pizarro had a tail and gave it the cometary designation 133P/Elst-Pizarro.
In 1997, NASA's NEAR Shoemaker probe photographed asteroid 253 Mathilde.
In 1998, it was defined that when an observer finds an apparition, it gets a provisional designation, made up of the year of discovery, a letter representing the half-month of discovery, and finally a letter and a number indicating the discovery's sequential number (example: 1998 FJ74).
In 1999, the Deep Space 1 spacecraft performed a flyby of asteroid 9969 Braille.
In 2001, the NEAR Shoemaker spacecraft successfully landed on the surface of asteroid 433 Eros, marking the first successful landing on an asteroid.
In 2002, Asteroid 2002 AA29 was discovered and found to have an unusual horseshoe orbit that is co-orbital with Earth.
In 2002, an example provisional designation was given as 2002 AT4, which includes the year of discovery and an alphanumeric code.
In 2002, the Small Main-Belt Asteroid Spectroscopic Survey resulted in a modified version of the Tholen taxonomy with 24 different types.
In 2002, the Stardust spacecraft flew by asteroid 5535 Annefrank.
From September to November 2005, the Japanese Hayabusa probe studied asteroid 25143 Itokawa in detail.
In 2006, astronomers David Jewitt and Henry Hsieh originally designated active asteroids as main-belt comets (MBCs).
In 2006, the IAU created the class of dwarf planets for the largest minor planets. Ceres was placed in this category.
In 2006, the International Astronomical Union (IAU) introduced the term 'small Solar System body' to broadly categorize objects in the Solar System that are neither planets, dwarf planets, nor natural satellites, including asteroids and comets.
In 2007, NASA launched the Dawn spacecraft, which subsequently orbited 4 Vesta for a year and observed the dwarf planet Ceres for three years.
In 2008, the Rosetta probe briefly visited asteroids 2867 Šteins and 21 Lutetia while en route to its primary destination.
On June 13, 2010, the Japanese Hayabusa probe returned samples from the surface of asteroid 25143 Itokawa to Earth, marking the first asteroid sample-return mission.
As of 2011, it was estimated that 89% to 96% of near-Earth asteroids one kilometer or larger in diameter had been discovered.
In 2012, China's lunar orbiter Chang'e 2 flew within 3.2 km of asteroid 4179 Toutatis.
In October 2013, water was detected on an extrasolar body for the first time, specifically on an asteroid orbiting the white dwarf GD 61.
According to expert testimony in the United States Congress in 2013, NASA would require at least five years of preparation before a mission to intercept an asteroid could be launched.
On 22 January 2014, ESA scientists reported the detection of water vapor on Ceres, the largest object in the asteroid belt, using the Herschel Space Observatory.
In 2014, JAXA launched the Hayabusa2 probe to asteroid 162173 Ryugu.
In 2016, NASA launched the OSIRIS-REx mission to asteroid 101955 Bennu for sample return.
In 2017, observations were taken with the Very Large Telescope's SPHERE imager.
In 2017, radar imaging discovered that the asteroid 3122 Florence has two moons.
In June 2018, the National Science and Technology Council warned that the United States is unprepared for an asteroid impact event and released the "National Near-Earth Object Preparedness Strategy Action Plan" to improve preparedness.
As of 29 October 2018, the LINEAR system alone had discovered 147,132 asteroids, including almost 900 near-Earth asteroids larger than 1 km.
In 2018, observations were taken with the Very Large Telescope's SPHERE imager.
In November 2019, scientists reported detecting sugar molecules, including ribose, in meteorites, suggesting that chemical processes on asteroids can produce bio-ingredients important to life.
In 2019, it was shown that the Acfer 049 meteorite has an ultraporous lithology (UPL), suggesting that UPL represents fossils of primordial ice.
In 2020, samples collected by Hayabusa2 from asteroid 162173 Ryugu were delivered to Earth.
In 2020, the OSIRIS-REx mission studied the asteroid Bennu and collected a sample.
As of October 2021, there were 85 NEAs known to have at least one moon, including three known to have two moons.
In 2021, the OSIRIS-REx probe departed from asteroid 101955 Bennu with a sample from its surface.
As of April 2022, a total of 28,772 near-Earth asteroids were known; 878 have a diameter of one kilometer or larger.
In September 2022, the DART spacecraft deliberately crashed into Dimorphos, the minor-planet moon of the double asteroid Didymos, as part of the asteroid deflection experiment.
In September 2022, the Double Asteroid Redirection Test spacecraft successfully altered the orbit of the non-threatening asteroid Dimorphos by crashing into it, as an experiment to meet the danger of Near-Earth asteroids.
In September 2023, the OSIRIS-REx mission delivered a sample from asteroid 101955 Bennu to Earth.
In October 2023, NASA launched the Psyche mission to study the large metallic asteroid Psyche.
ESA launched the Hera mission in October 2024 to study the results of the DART impact on Dimorphos.
In October 2024, ESA's Hera mission was launched to study the results of the DART impact.
In 2024, dark comets, asteroids exhibiting non-gravitational acceleration without a coma or tail, were first identified, revealing two distinct families: the Outer Family and the Inner Family.
CNSA's Tianwen-2 was launched in May 2025 and will explore the near-Earth asteroid 469219 Kamoʻoalewa and active asteroid 311P/PanSTARRS, collecting samples from Kamo'oalewa's regolith.
As of May 2025, the Minor Planet Center had data on 1,460,356 minor planets in the inner and outer Solar System, of which about 826,864 had enough information to be given numbered designations.
NASA's Lucy probe is not set to reach its first main target, 3548 Eurybates, until 2027.
In 2029, the OSIRIS-REx spacecraft, in its extended mission designated OSIRIS-APEX, will explore the near-Earth asteroid Apophis.
The Hayabusa2 spacecraft, on an extended mission, is expected to arrive at a new target in 2031.
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