Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

59P/Kearns–Kwee

From Wikipedia, the free encyclopedia
Periodic comet

59P/Kearns–Kwee
Comet Kearns–Kwee photographed from theZwicky Transient Facility on 31 January 2019
Discovery[1]
Discovered byCharles E. Kearns
Kiem King Kwee
Discovery sitePalomar Observatory
Discovery date17 August 1963
Designations
P/1963 Q1, P/1971 O1
  • 1963 VIII, 1972 XI
  • 1981 XX, 1990 XXV
  • 1963d, 1971c, 1981h
  • 1989u
Orbital characteristics[3][4]
Epoch25 February 2023 (JD 2460000.5)
Observation arc55.62 years
Number of
observations
1,849
Aphelion6.618 AU
Perihelion2.348 AU
Semi-major axis4.483 AU
Eccentricity0.47617
Orbital period9.492 years
Inclination9.344°
312.79°
Argument of
periapsis
127.52°
Mean anomaly168.35°
Last perihelion16 September 2018
Next perihelion15 March 2028[2]
TJupiter2.771
EarthMOID1.381 AU
JupiterMOID0.006 AU
Physical characteristics[5]
Mean radius
0.79±0.03 km
0.04 (assumed)
Comet total
magnitude
(M1)
10.4
Comet nuclear
magnitude (M2)
14.7

59P/Kearns–Kwee is aperiodic comet in theSolar System with a current orbital period of 9.49 years.[3][6]

Observational history

[edit]

It was discovered by Charles E. Kearns and Kiem King Kwee on a photographic plate taken on 17 August 1963 during a search for the then-lost comet55P/Tempel–Tuttle, and was later confirmed byElizabeth Roemer at theUS Naval Observatory Flagstaff Station in Arizona. She estimated its brightness at a faint magnitude of 16. The perihelion was initially calculated as 28 October 1963 and the periodicity as 8.48 years, but calculations based on further observations revised the data to 7 December and 8.95 years.

The 1972 apparition was observed by Elizabeth Roemer and L. M. Vaughn of theUniversity of Arizona, using the 229-cm reflector at Kitt Peak as early as 26 July 1971. It was relocated in 1981 byTsutomu Seki of Japan and again on 10 September 1989 by J. Gibson atPalomar Observatory. It was also successfully re-observed in 1999 and 2009.

Physical characteristics

[edit]

The nucleus of the comet has an effective radius of0.79±0.03 km, assuming ageometric albedo of 0.04.[5]

See also

[edit]

References

[edit]
  1. ^C. E. Kearns; K. K. Kwee; M. Schmidt; E. Roemer (30 August 1963). K. A. Thernöe (ed.)."Comet Kearns–Kwee (1963d)".IAU Circular (1).
  2. ^"Horizons Batch for 59P/Kearns-Kwee (90000649) on 2028-Mar-15" (Perihelion occurs when rdot flips from negative to positive).JPL Horizons.Archived from the original on 29 September 2025. Retrieved29 September 2025. (JPL#K182/6 Soln.date: 2023-Jan-17)
  3. ^ab"59P/Kearns–Kwee Orbit".Minor Planet Center. Retrieved24 February 2019.
  4. ^"59P/Kearns–Kwee – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved10 June 2025.
  5. ^abP. L. Lamy; I. Toth; H. A. Weaver; M. F. A'Hearn; L. Jorda (2009)."Properties of the nuclei and comae of 13 ecliptic comets from Hubble Space Telescope snapshot observations".Astronomy & Astrophysics.508 (2):1045–1056.Bibcode:2009A&A...508.1045L.doi:10.1051/0004-6361/200811462.S2CID 125249770.
  6. ^G. W. Kronk."59P/Kearns-Kwee".Cometography.com. Retrieved21 February 2015.

External links

[edit]


Numbered comets
Previous
58P/Jackson–Neujmin
59P/Kearns–KweeNext
60P/Tsuchinshan
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=59P/Kearns–Kwee&oldid=1314045305"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp