Discovery [1] | |
---|---|
Discovered by | Hideo Nishimura (Kakegawa, Japan) |
Discovery date | 12 August 2023 |
Designations | |
C/2023 P1 | |
HN00003 | |
Orbital characteristics [2] | |
Observation arc | 232 days (7.7 months) |
Earliest precovery date | 19 January 2023 |
Number of observations | 477 |
Aphelion | 114 AU (1800) [3] 110 AU (2200) |
Perihelion | 0.225 AU (33.7 million km; 87.6 LD) [4] (73% of Mercury's perihelion) |
Semi-major axis | 57 AU (comparable to Eris) [2] |
Eccentricity | 0.9961 (1800) [3] 0.9959 (2200) |
Orbital period | ≈431 years (inbound) [3] ≈406 years (outbound) |
Max. orbital speed | 88.7 km/s @ perihelion [4] |
Inclination | 132.5° |
66.8° | |
Argument of periapsis | 116.3° |
Last perihelion | 17 September 2023 15:24 [4] [2] ≈1588–1592 [5] [3] |
Next perihelion | ≈2430 Feb [6] |
Earth MOID | 0.078 AU (11.7 million km; 30 LD) [2] |
Jupiter MOID | 2.3 AU (340 million km) |
Comet total magnitude (M1) | 12.7 [2] |
C/2023 P1 (Nishimura) is a long-period comet discovered by Hideo Nishimura on 12 August 2023. [7] The comet passed perihelion on 17 September 2023 and reached an apparent magnitude of about 2.5. [8]
Japanese amateur astronomer Hideo Nishimura discovered the comet in images he obtained using a 200-mm f/3 telephoto lens mounted on a Canon EOS 6D on 12 August 2023, when the comet was 1.0 AU from the Sun. He also found it in images he exposed the previous night. [1] The comet upon discovery was located in the dawn sky and moving closer to the Sun and has been less than 50 degrees from the Sun since April 2023. Its apparent magnitude was estimated to be around 10–11. [1] Pre-discovery images from 19, 24, and 25 January 2023 from PanSTARRS were identified by Robert Weryk extending the observation arc to seven months. The comet appeared in them as a stellar object with an apparent magnitude of about 22. [5]
The comet brightened rapidly and by 27 August its apparent magnitude was estimated to be 7.3 and its coma to have a diameter of 5 arcminutes, while a thin ion tail 1.5–2 degrees long is visible in photographs. [9] The comet was spotted with the naked eye by Piotr Guzik on 8 September at an estimated magnitude of 4.7. [10] The comet tail was up to 7.5 degrees long when imaged with CCD. [10] On 12 September 2023 the comet passed 0.84 AU (126 million km ; 78 million mi ; 330 LD ) from Earth but was only 15 degrees from the glare of the Sun. [11]
On 17 September 2023 the comet came to perihelion 0.22 AU from the Sun. [4] [2] The comet appeared briefly in the evening sky in mid September, being 5 degrees over the horizon 30 minutes after sunset at 35° north latitude. [12] Even though the comet reached a naked eye apparent magnitude of around +2, it was difficult to locate against the glare of the Sun. [13] [14] After perihelion, the comet became visible in the coronograph of STEREO, without showing signs of disintegration. [15] The comet was also observed by Parker Solar Probe on 27-28 September 2023, during encounter 17. [16]
With an observation arc of seven months, the outbound orbital period of the comet is estimated to be about 406 years. [3] An eccentricity of 0.996 gives the comet a semi-major axis of about 57 AU, [2] which is comparable to the average distance of Eris at 68 AU. The comet will not leave the Solar System, will come to aphelion (farthest distance from the Sun) in 2227, [17] and return around the year 2430. [6]
Perihelion passages [5] | |||||||
302 | |||||||
723 | |||||||
1169 | |||||||
1588–1592 [3] | |||||||
2023-09-17 | |||||||
2430 Feb [6] |
Date and time of closest approach | Earth distance (AU) | Sun distance (AU) | Velocity relative to Earth (km/s) | Velocity relative to Sun (km/s) | Uncertainty region (3-sigma) | Solar elongation |
---|---|---|---|---|---|---|
12 September 2023 ≈09:20 | 0.838 AU (125.4 million km ; 77.9 million mi ; 326 LD ) | 0.292 AU (43.7 million km; 27.1 million mi; 114 LD) | 107.0 | 77.9 | ± 300 km | 14.9° |
It is possible that Comet C/2023 P1 (Nishimura) may be related to the Sigma Hydrids meteor shower that is active November 22 to January 18 (peaking around November 30). [9]
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Comet Crommelin, also known as Comet Pons-Coggia-Winnecke-Forbes, is a periodic comet with an orbital period of almost 28 years. It fits the classical definition of a Halley-type comet with. It is named after the British astronomer Andrew C. D. Crommelin who calculated its orbit in 1930. It is one of only four comets not named after their discoverer(s), the other three being Comets Halley, Encke, and Lexell. It next comes to perihelion around May 27, 2039 when it will be near a maximum near-perihelion distance from Earth.
94P/Russell 4 is a periodic comet in the Solar System. It fits the definition of an Encke-type comet with. It was discovered by Ken Rusell on photographic plates taken by M. Hawkins on March 7, 1984. In the discovery images, Russell estimated that the comet had an apparent magnitude of 13 and a noticeable tail of 5 arc minutes. In the year of discovery, the comet had come to perihelion in January 1984.
C/2000 W1 (Utsunomiya–Jones) is a long-period comet from the Oort cloud discovered on November 18, 2000, by Syogo Utsunomiya and Albert F. A. L. Jones. The comet reached up to apparent magnitude 5.5, but was only 27 degrees from the Sun in mid-December 2000.
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C/2014 UN271 (Bernardinelli–Bernstein), simply known as C/2014 UN271 or Comet Bernardinelli–Bernstein (nicknamed BB), is a large Oort cloud comet discovered by astronomers Pedro Bernardinelli and Gary Bernstein in archival images from the Dark Energy Survey. When first imaged in October 2014, the object was 29 AU (4.3 billion km; 2.7 billion mi) from the Sun, almost as far as Neptune's orbit and the greatest distance at which a comet has been discovered. With a nucleus diameter of at least 120 km (75 mi), it is the largest Oort cloud comet known. It is approaching the Sun and will reach its perihelion of 10.9 AU (just outside of Saturn's orbit) in January 2031. It will not be visible to the naked eye because it will not enter the inner Solar System.
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