Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

169P/NEAT

From Wikipedia, the free encyclopedia
Periodic comet
For other comets discovered by the Near-Earth Asteroid Tracking survey, seeComet NEAT (disambiguation).
169P/NEAT
Discovery
Discovered byNEAT
Discovery dateMarch 15, 2002
Designations
P/2002 EX12
Orbital characteristics[1][2]
Epoch2022-08-09 (2459800.5)
Aphelion4.6014 AU
Perihelion0.60282 AU
Semi-major axis2.6021AU
Eccentricity0.76833
Orbital period4.1975yr
Inclination11.2985°
Last perihelion9 July 2022
Physical characteristics[3]
Mean radius
2.5 km (1.6 mi)
8.4 hours

169/NEAT is aperiodic comet in theSolar System. It is the parent body of thealpha Capricornids meteor shower in late July. 169/NEAT may be related to cometP/2003 T12 (SOHO).[4][5]

Physical characteristics

[edit]

169P is a low activity comet roughly about 5.0 km (3.1 mi) in diameter,[3][6] with a rotation period lasting about 8.4 hours.[3] It could have originated from the mainasteroid belt.[5]

Orbit

[edit]

It last came toperihelion (closest approach to the Sun) on 9 July 2022.[2] On 13 July 2022 passed 0.1395 AU (20.87 million km) fromVenus.[1] On 11 August 2026, it will pass 0.1672 AU (25.01 million km) fromEarth and then come to perihelion on 21 September 2026.

169P has a similar stable orbit with the smaller body P/2003 T12 (SOHO), both avoiding close encounters with Jupiter. It is possible that both comets likely fragmented from a parent body a bit over 2,000 years ago.[5][6] A further fragmentation even about 4,500 to 5,000 years ago could have produced the meteors of the alpha Capricornids meteor shower. The total estimated mass of the meteors is similar to that of the surviving comet.[7]

References

[edit]
  1. ^ab"169P/NEAT – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved22 June 2022.
  2. ^ab"169P/NEAT Orbit".Minor Planet Center. Retrieved2 June 2014.
  3. ^abcB. E. A. Mueller; N. H. Samarasinha (2018)."Further Investigation of Changes in Cometary Rotation".The Astronomical Journal.156 (3):107–114.arXiv:1806.11158.Bibcode:2018AJ....156..107M.doi:10.3847/1538-3881/aad0a1.
  4. ^169P NEAT and P/2003 T12 - 300 years ago
  5. ^abcS. R. Alvarez; A. S. Oyarzabal (2024). "Comet P/2003 T12 (SOHO): A possible fragment of comet 169P/NEAT?".Planetary and Space Science.246 105902.doi:10.1016/j.pss.2024.105902.
  6. ^abA. Sosa; J. A. Fernández; A. Fitzsimmons (2015). "Comets 169P/NEAT and P/2003 T12 (SOHO): Two possible fragments of a common ancestor?".American Astronomical Society.29.Bibcode:2015IAUGA..2255583S.
  7. ^P. Jenniskens; J. Vaubaillon (2010). "Minor Planet2002 EX12(169P/NEAT) and the Alpha Capricornid Shower".The Astronomical Journal.139 (5):1822–1830.doi:10.1088/0004-6256/139/5/1822.

External links

[edit]


Numbered comets
Previous
168P/Hergenrother
169P/NEATNext
170P/Christensen
Features
Comet C/1996 B2 (Hyakutake)
Types
Related
Exploration
Latest
Culture and
speculation
Periodic
comets
Until 1985
(all)
After 1985
(notable)
Comet-like
asteroids
Lost
Recovered
Destroyed
Not found
Visited by
spacecraft
Near-Parabolic
comets
(notable)
Until 1990
After 1990
After 1910
(by name)
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=169P/NEAT&oldid=1314030240"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp