As of 2024, the United States, the Soviet Union, Japan, and the European Space Agency have conducted missions to comets.
Spacecraft | Launch date [1] | Operator | Comet | Mission | Outcome | Remarks | Carrier rocket [2] |
---|---|---|---|---|---|---|---|
ICE (ISEE-3) | 12 August 1978 | NASA United States / ESA | 21P/Giacobini–Zinner | Flyby | Successful | Extended mission; Closest approach of 7,862 kilometres (4,885 mi) at 11:02 UTC on 11 September 1985. Also made distant observations of 1P/Halley in May 1986. [3] | Delta 2914 |
Vega 1 (5VK No.901) | 15 December 1984 | Soviet Union | 1P/Halley | Flyby | Successful | Flew past Halley after visiting Venus; closest approach 8,889 kilometres (5,523 mi) at 07:20:06 UTC on 6 March 1986. [4] | Proton-K/D-1 |
Vega 2 (5VK No.902) | 21 December 1984 | Soviet Union | 1P/Halley | Flyby | Successful | Flew past Halley after visiting Venus; closest approach at 07:20 UTC on 9 March 1986. [5] | Proton-K/D-1 |
Sakigake (MS-T5) | 7 January 1985 | ISAS Japan | 1P/Halley | Flyby | Successful | Closest approach of 6.99 million kilometres (4.34 million miles) at 04:18 UTC on 11 March 1986. [6] | Mu-3S-II |
Giotto | 2 July 1985 | ESA | 1P/Halley | Flyby | Successful | Closest approach of 605 kilometres (376 mi) at 00:03:02 UTC on 14 March 1986. [7] | Ariane 1 |
26P/Grigg–Skjellerup | Flyby | Successful | Extended mission. Closest approach of 200 kilometres (120 mi) at 15:30 UTC on 10 July 1992. [7] | ||||
Suisei (PLANET-A) | 19 August 1985 | ISAS Japan | 1P/Halley | Flyby | Successful | Closest approach of 152,400 kilometres (94,700 mi) at 13:06 UTC on 8 March 1986 [8] | Mu-3S-II |
21P/Giacobini–Zinner | Flyby | Spacecraft failure (Extended mission) | Extended mission, spacecraft ran out of fuel en route; flyby had been scheduled for 24 November 1998 [8] | ||||
Deep Space 1 | 24 October 1998 | NASA United States | 107P/Wilson–Harrington [9] | Flyby | Spacecraft failure | Spacecraft was unable to reach Wilson–Harrington due to ion engine operation being suspended while a problem with the probe's star tracker was investigated. [10] | Delta II 7326 |
19P/Borrelly | Flyby | Successful | Extended mission | ||||
Stardust (Discovery 4) | 7 February 1999 | NASA United States | 81P/Wild | Flyby | Successful | Delta II 7426 | |
Sample return | Successful | ||||||
9P/Tempel | Flyby | Successful | Extended mission, Stardust-NExT, to survey crater caused by Deep Impact | ||||
CONTOUR (Discovery 6) | 3 July 2002 | NASA United States | 2P/Encke | Flyby | Spacecraft failure | Delta II 7425 | |
73P/Schwassmann–Wachmann | Flyby | Spacecraft failure | |||||
6P/d'Arrest | Flyby | Spacecraft failure | Flyby provisionally scheduled at time of spacecraft's failure | ||||
Rosetta | 2 March 2004 | ESA | 67P/Churyumov–Gerasimenko | Orbiter | Successful | Entered orbit around 67P at 09:06 UTC on 6 August 2014. On 30 September 2016 mission ended in an attempt to slow land on the comet's surface near a 130 m (425 ft) wide pit called Deir el-Medina. | Ariane 5G+ |
Philae | 2 March 2004 | ESA / DLR Germany | 67P/Churyumov–Gerasimenko | Lander | Successful | Carried by Rosetta. Came to rest on the surface of 67P at 17:32 UTC on 12 November 2014. Communications ceased with the loss of battery power at 00:36 UTC on 15 November 2014 and the lander began hibernating. Reactivated on solar power and briefly established contact with ground control again at 20:28 UTC on 13 June 2015, and sporadically until 9 July 2015 when the last communication was received. [11] [12] | Ariane 5G+ |
Deep Impact (Discovery 7) | 12 January 2005 | NASA United States | 9P/Tempel | Flyby | Successful | Delta II 7925 | |
Impactor | Successful | Impact occurred at 05:52 UTC on 4 July 2005. | |||||
103P/Hartley | Flyby | Successful | Extended mission (EPOXI) |
A comet is an icy, small Solar System body that warms and begins to release gases when passing close to the Sun, a process called outgassing. This produces an extended, gravitationally unbound atmosphere or coma surrounding the nucleus, and sometimes a tail of gas and dust gas blown out from the coma. These phenomena are due to the effects of solar radiation and the outstreaming solar wind plasma acting upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small rocky particles. The coma may be up to 15 times Earth's diameter, while the tail may stretch beyond one astronomical unit. If sufficiently close and bright, a comet may be seen from Earth without the aid of a telescope and can subtend an arc of up to 30° across the sky. Comets have been observed and recorded since ancient times by many cultures and religions.
Rosetta was a space probe built by the European Space Agency launched on 2 March 2004. Along with Philae, its lander module, Rosetta performed a detailed study of comet 67P/Churyumov–Gerasimenko (67P). During its journey to the comet, the spacecraft performed flybys of Earth, Mars, and the asteroids 21 Lutetia and 2867 Šteins. It was launched as the third cornerstone mission of the ESA's Horizon 2000 programme, after SOHO / Cluster and XMM-Newton.
A lander is a spacecraft that descends towards, then comes to rest on the surface of an astronomical body other than Earth. In contrast to an impact probe, which makes a hard landing that damages or destroys the probe upon reaching the surface, a lander makes a soft landing after which the probe remains functional.
67P/Churyumov–Gerasimenko is a Jupiter-family comet. It is originally from the Kuiper belt and has an orbital period of 6.45 years as of 2012, a rotation period of approximately 12.4 hours, and a maximum velocity of 135,000 km/h. Churyumov–Gerasimenko is approximately 4.3 by 4.1 km at its longest and widest dimensions. It was first observed on photographic plates in 1969 by Soviet astronomers Klim Ivanovych Churyumov and Svetlana Ivanovna Gerasimenko, after whom it is named. It most recently came to perihelion on 2 November 2021, and will next come to perihelion on 9 April 2028.
Philae was a robotic European Space Agency lander that accompanied the Rosetta spacecraft until it separated to land on comet 67P/Churyumov–Gerasimenko, ten years and eight months after departing Earth. On 12 November 2014, Philae touched down on the comet, but it bounced when its anchoring harpoons failed to deploy and a thruster designed to hold the probe to the surface did not fire. After bouncing off the surface twice, Philae achieved the first-ever "soft" (nondestructive) landing on a comet nucleus, although the lander's final, uncontrolled touchdown left it in a non-optimal location and orientation.
Rosetta is a space probe designed to rendezvous with the comet 67P/Churyumov–Gerasimenko, perform flybys of two asteroids, and carry lander Philae until its landing on 67P. This page records a detailed timeline of this mission.
The Italian Space Agency is a government agency established in 1988 to fund, regulate and coordinate space exploration activities in Italy. The agency cooperates with numerous national and international entities who are active in aerospace research and technology.
The Comet Rendezvous Asteroid Flyby (CRAF) was a cancelled plan for a NASA-led exploratory mission designed by the Jet Propulsion Laboratory during the mid-to-late 1980s and early 1990s, that planned to send a spacecraft to encounter an asteroid, and then to rendezvous with a comet and fly alongside it for nearly three years. The project was eventually canceled when it went over budget; most of the money still left was redirected to its twin spacecraft, Cassini–Huygens, destined for Saturn, so it could survive Congressional budget cutbacks. Most of CRAF's scientific objectives were later accomplished by the smaller NASA spacecraft Stardust and Deep Impact, and by ESA's flagship Rosetta mission.
The nucleus is the solid, central part of a comet, formerly termed a dirty snowball or an icy dirtball. A cometary nucleus is composed of rock, dust, and frozen gases. When heated by the Sun, the gases sublime and produce an atmosphere surrounding the nucleus known as the coma. The force exerted on the coma by the Sun's radiation pressure and solar wind cause an enormous tail to form, which points away from the Sun. A typical comet nucleus has an albedo of 0.04. This is blacker than coal, and may be caused by a covering of dust.
This is a timeline of space exploration which includes notable achievements, first accomplishments and milestones in humanity's exploration of outer space.
The Max Planck Institute for Solar System Research is a research institute in astronomy and astrophysics located in Göttingen, Germany, where it relocated in February 2014 from the nearby village of Lindau. The exploration of the Solar System is the central theme for research done at this institute.
Discovery and exploration of the Solar System is observation, visitation, and increase in knowledge and understanding of Earth's "cosmic neighborhood". This includes the Sun, Earth and the Moon, the major planets Mercury, Venus, Mars, Jupiter, Saturn, Uranus, and Neptune, their satellites, as well as smaller bodies including comets, asteroids, and dust.
A flyby is a spaceflight operation in which a spacecraft passes in proximity to another body, usually a target of its space exploration mission and/or a source of a gravity assist to impel it towards another target. Spacecraft which are specifically designed for this purpose are known as flyby spacecraft, although the term has also been used in regard to asteroid flybys of Earth for example. Important parameters are the time and distance of closest approach.
CAESAR is a sample-return mission concept to comet 67P/Churyumov–Gerasimenko. The mission was proposed in 2017 to NASA's New Frontiers program mission 4, and on 20 December 2017 it was one of two finalists selected for further concept development. On 27 June 2019, the other finalist, the Dragonfly mission, was chosen instead.
Stephan Ulamec is an Austrian geophysicist, born in Salzburg on January 27, 1966, with more than 100 articles in peer-reviewed journals and several participations in space missions and payloads operated by diverse space agencies. He is working at the German Aerospace Center in Cologne. He is regularly giving lectures about his publications in aerospace engineering at the University of Applied Sciences: Fachhochschule FH-Aachen. Main aspects of his work are related to the exploration of small bodies in the solar system.