67P/Churyumov–Gerasimenko (abbreviated 67P or 67P/C–G and nicknamed "Chury") 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 . Churyumov–Gerasimenko is approximately 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 (closest approach to the Sun) on 2 November 2021, and will next come to perihelion on 9 April 2028.
Churyumov–Gerasimenko was the destination of the European Space Agency's Rosetta mission, launched on 2 March 2004. Rosetta rendezvoused with Churyumov–Gerasimenko on 6 August 2014 and entered orbit on 10 September 2014. Rosetta lander, Philae, landed on the comet's surface on 12 November 2014, becoming the first spacecraft to land on a comet nucleus. On 30 September 2016, the Rosetta spacecraft ended its mission by landing on the comet in its Maat region.
Discovery Churyumov–Gerasimenko was discovered in 1969 by Klim Ivanovich Churyumov of Kyiv University's Astronomical Observatory, who examined a photograph that had been exposed for comet Comas Solà by Svetlana Ivanovna Gerasimenko on 11 September 1969 at the Alma-Ata Astrophysical Institute, near Alma-Ata, the then-capital city of Kazakh Soviet Socialist Republic, Soviet Union. Churyumov found a cometary object near the edge of the plate, but assumed that this was comet Comas Solà.
After returning to his home institute in Kyiv, Churyumov examined all the photographic plates more closely. On 22 October, about a month after the photograph was taken, he discovered that the object could not be Comas Solà, because it was about 1.8 degrees off the expected position. Further scrutiny produced a faint image of Comas Solà at its expected position on the plate, thus proving the other object to be a different body.
Shape
The comet consists of two lobes connected by a narrower neck, with the larger lobe measuring about and the smaller one about . With each orbit the comet loses matter, as gas and dust are evaporated away by the Sun. It is estimated that a layer with an average thickness of about is lost per orbit as of 2015. The comet has a mass of approximately 10 billion tonnes.
The two-lobe shape of the comet is the result of a gentle, low-velocity collision of two objects, and is called a contact binary. The "terraces", layers of the interior of the comet that have been exposed by partial stripping of outer layers during its existence, are oriented in different directions in the two lobes, indicating that two objects fused to form Churyumov–Gerasimenko.
A high-resolution photogrammetric shape model of the nucleus, featuring 132.1 million facets, was reconstructed using 7,682 NAC and 1,504 WAC images from the OSIRIS cameras taken post-perihelion. This model enabled the first detailed description and thermal modeling of Subsurface Access Points (SAPs)—cavities ranging from 20 to 47 meters in depth that provide direct access to the comet's subsurface. The study established a correlation between the energy threshold received at the bottom of these SAPs and the onset of transient sublimation jets. These sites are considered primary targets for future sample-return missions seeking pristine material beneath the surface crust.. Video visualization: 3D stereoscopic and 2D version via YouTube.
Surface
There are 26 distinct regions on Churyumov–Gerasimenko, with each named after an Egyptian deity; regions on the large lobe are named after gods, whereas those on the small lobe are named after goddesses. Nineteen regions were defined in the northern hemisphere prior to equinox. Later, when the southern hemisphere became illuminated, seven more regions were identified using the same naming convention.
Region Terrain Region Terrain Region Terrain Maat Dust covered Ash Dust covered Babi Dust covered Seth Pitted and brittle material Hatmehit Large-scale depression Nut Large-scale depression Aten Large-scale depression Hapi Smooth Imhotep Smooth Anubis Smooth Maftet Rock-like Bastet Rock-like Serqet Rock-like Hathor Rock-like Anuket Rock-like Khepry Rock-like Aker Rock-like Atum Rock-like Apis Rock-like Khonsu Rock-like Bes Rock-like Anhur Rock-like, rather friable Geb Rock-like Sobek Rock-like Neith Rock-like Wosret Rock-like
Gates Features described as gates, twin prominences on the surface so named for their appearance, were named after deceased members of the Rosetta team. Name Named after C. Alexander Gate Claudia Alexander A. Coradini Gate Angioletta Coradini
Surface changes During Rosetta lifetime, many changes were observed on the comet's surface, particularly when the comet was close to perihelion. These changes included evolving patterns of circular shapes in smooth terrains that at some point grew in size by a few meters per day. A fracture in the neck region was also observed to grow in size; boulders tens of meters wide were displaced, sometimes travelling more than 100 meters; and patches of the ground were removed to expose new features. A number of collapsing cliffs have also been observed. One notable example in December 2015 was captured by Rosetta NAVCAM as a bright patch of light shining from the comet. Rosetta scientists determined that a large cliff had collapsed, making it the first landslide on a comet known to be associated with an outburst of activity. An apparent outburst of the comet was observed on 14 November 2021. According to the researchers, "At the time of the outburst discovery with ZTF, the comet was 1.23 au from the Sun and 0.42 au from the Earth. The comet's last perihelion passage was on 2021 Nov 2.".
Cheops boulder Cheops is the largest boulder on the surface of the comet, measuring up to 45 meters. It is located in the comet's larger lobe. It was named for the pyramid in Giza because its shape is similar to that of a pyramid.
Orbit and rotation Perihelion distanceat different epochs Epoch Perihelion(AU) 1821 2.44 1882 2.94 1956 2.74 1963 1.28 2021 1.21 2101 1.35 2223 ≈ 0.8
Like the other comets of the Jupiter family, Churyumov–Gerasimenko probably originated in the Kuiper belt and was ejected towards the interior of the Solar System, where later encounters with Jupiter successively changed its orbit. These interactions will continue until the comet is eventually thrown out of the Solar System or collides with the Sun or a planet.
On 4 February 1959, a close encounter with Jupiter of moved Churyumov–Gerasimenko's perihelion inward from to , where it basically remains today. In November 2220 the comet will pass about from Jupiter which will move perihelion inwards to about from the Sun.
Before Churyumov–Gerasimenko's perihelion passage in 2009, its rotational period was 12.76 hours. During this perihelion passage, it decreased to 12.4 hours, which likely happened because of sublimation-induced torque.
2015 perihelion , Churyumov–Gerasimenko's nucleus had an apparent magnitude of roughly 20. It came to perihelion on 13 August 2015. From December 2014 until September 2015, it had an elongation less than 45 degrees from the Sun. On 10 February 2015, it went through solar conjunction when it was 5 degrees from the Sun and was from Earth. It crossed the celestial equator on 5 May 2015 and became easiest to see from the Northern Hemisphere. Even right after perihelion when it was in the constellation of Gemini, it only brightened to about apparent magnitude 12, and required a telescope to be seen. , the comet had a total magnitude of about 20.
2021 perihelion
The 2021 apparition marked the closest approach to Earth since 1982. The comet reached perihelion on 2 November 2021 and the closest approach to Earth was on November 12, 2021, at 00:50 UTC, at a distance of 38 million miles (61 million km). The comet brightened to an apparent magnitude of 9, meaning it was visible with amateur telescopes. Two outbursts were observed during the apparition, on 2021 October 29.940 and November 17.864 UTC, −3.12 days and +15.81 days, respectively, from the perihelion date. During the first outburst the comet brightened by 0.26 ± 0.03 mag in the outburst, with a 27% increase in the effective geometric cross-section and total outburst dust mass of . The second outburst caused a brightening of 0.49 ± 0.08 mag with effective geometric cross-section and total outburst dust mass 2.5 times larger than the first event. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.
Exploration Rosetta mission
The Rosetta mission was the first mission to include an orbiter that accompanied a comet for several years, as well as a lander that collected close-up data from the comet's surface. The mission launched in 2004, arrived at comet 67P in 2014, and concluded with a touchdown on the comet's surface in 2016.
Advance work
As preparation for the Rosetta mission, Hubble Space Telescope pictures taken on 12 March 2003 were closely analysed. An overall 3D model was constructed and computer-generated images were created.
On 25 April 2012, the most detailed observations until that time were taken with the 2-meter Faulkes Telescope by N. Howes, G. Sostero and E. Guido while it was at its aphelion.
On 6 June 2014, water vapor was detected being released at a rate of roughly when Rosetta was from Churyumov–Gerasimenko and from the Sun. On 14 July 2014, images taken by Rosetta showed that its nucleus is irregular in shape with two distinct lobes. The size of the nucleus was estimated to be . Two explanations for its shape were proposed at the time: that it was a contact binary, or that its shape may have resulted from asymmetric erosion due to ice sublimating from its surface to leave behind its lobed shape. By September 2015, mission scientists had determined that the contact binary hypothesis was unambiguously correct.
Rendezvous and orbit
Beginning in May 2014, Rosetta velocity was reduced by with a series of thruster firings. Ground controllers rendezvoused Rosetta with Churyumov–Gerasimenko on 6 August 2014. This was done by reducing Rosetta relative velocity to . Rosetta entered orbit on 10 September, at about from the nucleus.
Landing
Descent of a small lander occurred on 12 November 2014. Philae is a robotic probe that set down on the surface with landing gear. The landing site has been christened Agilkia in honor of Agilkia Island, where the temples of Philae Island were relocated after the construction of the Aswan Dam flooded the island. The acceleration due to gravity on the surface of Churyumov–Gerasimenko has been estimated for simulation purposes at 10−3 m/s, or about 1/10,000 of that on Earth.
Because of its low relative mass, landing on the comet relied on tools to anchor Philae to the surface. The probe had an array of mechanisms designed to manage Churyumov–Gerasimenko's low gravity, including a cold gas thruster, harpoons, landing-leg-mounted ice screws, and a flywheel to keep it oriented during its descent. During the event, the thruster and the harpoons failed to operate, and the ice screws did not gain a grip. The lander bounced twice and only came to rest when it made contact with the surface for the third time, two hours after first contact.