Discovery [1] | |
---|---|
Discovered by | J. Robinson |
Discovery site | ATLAS–HKO (T05) |
Discovery date | 16 December 2019 |
Designations | |
A10iMHA [2] CK19Y010 | |
Orbital characteristics [3] | |
Epoch | 12 April 2020 (JD 2458951.5) |
Observation arc | 208 days |
Number of observations | 1,010 |
Aphelion | 669.1457±3.3432 AU |
Perihelion | 0.838 AU |
Semi-major axis | ~240 AU |
Eccentricity | 0.99651 |
Orbital period | ~3,720 years |
Inclination | 73.348° |
31.366° | |
Argument of periapsis | 57.498° |
Mean anomaly | 0.007° |
Last perihelion | 15 March 2020 |
Earth MOID | 0.083 AU |
Jupiter MOID | 1.026 AU |
Physical characteristics [4] | |
Dimensions | 1.2 km (0.75 mi) |
Comet total magnitude (M1) | 11.9±1.0 |
Comet nuclear magnitude (M2) | 13.8±0.5 |
C/2019 Y1 (ATLAS) is a comet with a near-parabolic orbit discovered by the ATLAS survey on 16 December 2019. It passed perihelion on 15 March 2020 at 0.84 AU from the Sun. [3] Its orbit is very similar to C/1988 A1 (Liller), C/1996 Q1 (Tabur), C/2015 F3 (SWAN) and C/2023 V5 (Leonard), suggesting they may be fragments of a larger ancient comet. [5]
The comet passed close to Earth in early May 2020. It was visible in the northern hemisphere sky in the spring of 2020.
Comet Giacobini–Zinner is a periodic comet in the Solar System. It was discovered by Michel Giacobini, who observed it in the constellation of Aquarius on 20 December 1900. It was recovered two orbits later by Ernst Zinner, while he was observing variable stars near Beta Scuti on 23 October 1913.
The Great Comet of 1882, formally designated as C/1882 R1, 1882 II, and 1882b, was a comet which became very bright in September 1882. It was a member of the Kreutz Sungrazers, a family of comets which pass within 1 R☉ of the Sun's photosphere at perihelion.
Comet Skorichenko–George, formally designated as C/1989 Y1, 1990 VI, and 1989e1, is a non-periodic comet co-discovered by astronomers Boris Skorichenko and Doug George on December 17, 1989. It has a hyperbolic trajectory around the Sun, but still weakly bound to it by its barycenter.
Comet IRAS–Araki–Alcock is a long-period comet that, in 1983, made the closest known approach to Earth of any comet in the last 200 years, at a distance of about 0.0312 AU.
Comet 96P/Machholz or 96P/Machholz 1 is a short-period sungrazing comet discovered on May 12, 1986, by amateur astronomer Donald Machholz on Loma Prieta peak, in central California using 130 millimetres (5.1 in) binoculars. On June 6, 1986, 96P/Machholz passed 0.404 AU from the Earth. 96P/Machholz last came to perihelion on January 31, 2023. The comet has an estimated diameter of around 6.4 km (4.0 mi).
Comet McNaught–Russell, formally designated as C/1993 Y1, is a long-period comet that reached a maximum magnitude of 6.5 in early 1994. It was discovered by Robert H. McNaught and Kenneth S. Russell using the U.K. Schmidt Telescope in Australia. McNaught and Russell worked at Siding Spring Observatory and together discovered five comets between 1991 and 1995.
C/2007 W1 (Boattini) is a non-periodic comet discovered on 20 November 2007, by Andrea Boattini at the Mt. Lemmon Survey. At the peak the comet had an apparent magnitude around 5.
D/1770 L1, popularly known as Lexell's Comet after its orbit computer Anders Johan Lexell, was a comet discovered by astronomer Charles Messier in June 1770. It is notable for having passed closer to Earth than any other comet in recorded history, approaching to a distance of only 0.015 astronomical units, or six times the distance from the Earth to the Moon. The comet has not been seen since 1770 and is considered a lost comet.
C/2002 T7 (LINEAR) is a hyperbolic comet discovered in 2002 by the LINEAR project. The comet brightened to a magnitude of 2.2 in 2004.
The Great Comet of 1823, also designated C/1823 Y1 or Comet De Bréauté-Pons, was a bright comet visible from December 1823 to April 1824.
C/1490 Y1 is a comet that was recorded and observed across East Asia, particularly China and Korea, from December 1490 to February 1491. It is the parent body of the Quadrantids meteor shower.
C/2015 ER61 (PanSTARRS) is a comet and inner Oort cloud object. When classified as a minor planet, it had the fourth-largest aphelion of any known minor planet in the Solar System, after 2005 VX3, 2012 DR30, and 2013 BL76. It additionally had the most eccentric orbit of any known minor planet, with its distance from the Sun varying by about 99.9% during the course of its orbit, followed by 2005 VX3 with an eccentricity of 0.9973. On 30 January 2016, it was classified as a comet when it was 5.7 AU from the Sun. It comes close to Jupiter, and a close approach in the past threw it on the distant orbit it is on now.
Candy's Comet, also known as C/1960 Y1 by its modern nomenclature, is a non-periodic comet in retrograde orbit around the Sun. It is the first comet to have its orbit calculated by its own discoverer.
C/2017 T1 (Heinze) is a hyperbolic comet that passed closest to Earth on 4 January 2018 at a distance of 0.22 AU (33 million km).
C/2018 Y1 (Iwamoto) is a long period comet with a retrograde orbit discovered on 18 December 2018, by Japanese amateur astronomer Masayuki Iwamoto. Its period is estimated to be 1,733 years. It passed closest to Earth on 13 February 2019. It was expected to reach a magnitude of between 6.5 and 7.5, visible in binoculars or a small telescope and was reported to reach a magnitude of 5.5 by Juan Jose Gonzalez on February 13, before fading to 7.6 two weeks later.
C/2019 Y4 (ATLAS) was a comet with a near-parabolic orbit discovered by the ATLAS survey on December 28, 2019. Early predictions based on the brightening rate suggested that the comet could become as bright as magnitude 0 matching the brightness of Vega. It received widespread media coverage due to its dramatic increase in brightness and orbit similar to the Great Comet of 1844, but on 22 March 2020, the comet started disintegrating. Such fragmentation events are very common for Kreutz Sungrazers. The comet continues to fade and did not reach naked eye visibility. By mid-May, comet ATLAS appeared very diffuse even in a telescope. C/2019 Y4 (ATLAS) has not been seen since 21 May 2020.
C/2020 F8 (SWAN), or Comet SWAN, is an Oort cloud comet that was discovered in images taken by the Solar Wind Anisotropies (SWAN) camera on 25 March 2020, aboard the Solar and Heliospheric Observatory (SOHO) spacecraft. In the glare of twilight, Comet SWAN is difficult to find with 50mm binoculars even though it is still near the theoretical range of naked eye visibility. The comet has dimmed since May 3. As of perihelion, the comet is very diffuse, does not have a visible nucleus and is not a comet that will be noticed by inexperienced observers. It is likely that the comet disintegrated.
Comet Ikeya-Seki, formally designated as C/1967 Y1, is a retrograde non-periodic comet discovered by Kaoru Ikeya and Tsutomu Seki on 1967. It is the second comet discovered together by the two Japanese astronomers after C/1965 S1.
Comet Erasmus, formally designated as C/2020 S3, is a non-periodic comet that became barely visible to the naked eye during the later months of 2020. Its maximum brightness peaked as a 3rd-magnitude object in the night sky, however its proximity to the Sun made it a difficult object to view from the ground.
Comet PanSTARRS, formal designation C/2022 A2, is a faint hyperbolic comet that passed through the inner Solar System in February 2023. It is one of many comets discovered by the Pan-STARRS survey.