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121P/Shoemaker-Holt

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121P/Shoemaker–Holt, also known as Shoemaker-Holt 2, is a periodic comet in the Solar System with an orbital period of about 8 years. The comet was discovered by Carolyn S. Shoemaker, Eugene M. Shoemaker, and Henry E. Holt on 9 March 1989. The comet then had an apparent magnitude of 13, was diffuse and had a tail about 2 arcminutes long. It was recovered by James V. Scotti on 29 August 1995 in images obtained as part of the Spacewatch survey.

Key facts

Comet.name
121P/Shoemaker-Holt
Comet.image
121P 2006-08-01 Spitzer image Level-2-PBCD-MIPS-24um.png
Comet.discoverer
Carolyn S. ShoemakerEugene Merle ShoemakerHenry E. Holt
Comet.discovery_date
March 9, 1989
Comet.designations
1989j; 1988 XI; 1995 Q3
Comet.epoch
March 6, 2006
Comet.semimajor
4.013 AU
Comet.perihelion
2.65 AU
Comet.aphelion
5.376 AU
Comet.eccentricity
0.3396
Comet.period
8.039 a
Comet.inclination
17.7218°
Comet.rotation
~10 hours
Comet.spectral_type
(V–R)
Comet.last_p
September 8, 2013September 1, 2004
Comet.next_p
2023-Jun-28

via Wikipedia infobox

Wikidata facts

Parent body
Sun
Diameter
3.24
Orbital period
2946.166484590266
Image
121P 2006-08-01 Spitzer image Level-2-PBCD-MIPS-24um.png
Show 14 more facts
discoverer or inventor
Eugene Merle Shoemaker
time of discovery or invention
1989-03-09
provisional designation
1988 XI
absolute magnitude
6.0
orbital eccentricity
0.3406038298142783
semi-major axis of an orbit
4.021973812676748
periapsis
2.652074128666313
apoapsis
5.391873496687183
orbital inclination
17.82702553259715
longitude of ascending node
99.09927639087128
argument of periapsis
7.391217241062686
mean anomaly
96.76248090532613
time of periapsis
2453253.615616086
Sources (2)

via Wikidata · CC0

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Encyclopedic overview

2 sections
Contents
  • References
  • External links

121P/Shoemaker–Holt, also known as Shoemaker-Holt 2, is a periodic comet in the Solar System with an orbital period of about 8 years. The comet was discovered by Carolyn S. Shoemaker, Eugene M. Shoemaker, and Henry E. Holt on 9 March 1989. The comet then had an apparent magnitude of 13, was diffuse and had a tail about 2 arcminutes long. It was recovered by James V. Scotti on 29 August 1995 in images obtained as part of the Spacewatch survey.

The nucleus of the comet is estimated to have a radius of 3.87 km based on infrared imaging by the Spitzer Space Telescope, when the comet displayed dust emission. Observations of the comet from the Isaac Newton Telescope indicate an effective radius of 3.61 kilometers. The rotational period was calculated to be 10 hours, but with high uncertainty.

Excerpted from Wikipedia’s “121P/Shoemaker-Holt” article, available under the CC BY-SA 4.0 licence.