(55565) 2002 AW197
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Template:Mp (provisional designation Template:Mp) is a classical, non-resonant trans-Neptunian object from the Kuiper belt in the outermost region of the Solar System, also known as a cubewano. It was discovered on 10 January 2002 by astronomers at Palomar Observatory. With a diameter of about Template:Convert, Template:Mp is approximately tied with Template:Mpl (to within measurement uncertainties) as the largest unnamed object in the Solar System.
Template:Mp has a rotation period of 8.8 hours and has a moderately red color.[1] The object's brightness does not significantly vary as it rotates, which indicates it is likely spheroidal.
History
Discovery
Template:Mp was discovered on 10 January 2002, by astronomers at Palomar Observatory in San Diego County, California, United States.[2] Astronomers involved in the discovery were Michael Brown, Chad Trujillo, Eleanor Helin, Michael Hicks, Kenneth Lawrence and Steven Pravdo.[3] The object was discovered during Brown and Trujillo's Caltech Wide Area Sky Survey, which used Palomar Observatory's Template:Convert Samuel Oschin telescope to search for bright Kuiper belt objects.[4]Template:Rp This survey, which was operated jointly with the nightly Near Earth Asteroid Tracking (NEAT) program at Palomar,[4]Template:Rp would later discover several other large objects beyond Neptune, including the dwarf planets Template:Dp, Template:Dp, and Template:Dp.[5]Template:Rp
Template:Mp was found through manual vetting of potential moving objects identified by Brown and Trujillo's automatic image-searching software.[4]Template:Rp In terms of absolute magnitude, Template:Mp was the second-brightest Kuiper belt object known at the time.[6] It was detected at a red-filter apparent magnitude of 19.7.[3] Template:Mp was further observed by Trujillo and Brown using telescopes at Palomar and Mauna Kea Observatory during February to April 2002.[3] The discovery was announced by the Minor Planet Center on 20 July 2002 and the object was given the minor planet provisional designation of Template:Mp.[3]
Further observations
Within a month after Template:Mp's discovery, Trujillo and Brown collaborated with Jean-Luc Margot and Frank Bertoldi to measure the object's diameter and thermal emission using the IRAM 30m radio telescope at Sierra Nevada, Spain.[7][6] Astronomers also found additional observations of Template:Mp from the time before and during its discovery, which allowed for further refinement of orbit calculations.[8] The earliest pre-discovery observation of Template:Mp comes from an image taken on 29 December 1997 by the NEAT/GEODSS program at Haleakalā Observatory, Hawaii.[2][8] Template:As of, Template:Mp has been observed for over 27 years, or about 8% of its orbital period.[9][2]
Numbering and naming
Template:Mp received its permanent minor planet catalog number of 55565 from the Minor Planet Center on 16 February 2003.[10]Template:Rp As of yet, it remains unnamed and the discoverers' privilege for naming this object expired ten years after its numbering.[2][11]Template:Rp Per naming guidelines by the International Astronomical Union's Working Group for Small Bodies Nomenclature, Template:Mp is open for name suggestions that pertain to creation myths, as required for Kuiper belt objects in general.[11]Template:Rp
Orbit and classification
Template:Mp is a trans-Neptunian object (TNO) orbiting the Sun at a semi-major axis or average distance of 47.2 astronomical units (AU).[12]Template:Efn It follows an elliptical orbit with an eccentricity of 0.13.[12] During its 324-year orbital period, Template:Mp comes within 41.1 AU from the Sun at perihelion and up to 53.3 AU at aphelion.[12] It has an orbital inclination of 24.4° with respect to the ecliptic.[12] Template:Mp last passed perihelion in July 1753 and will make its next perihelion passage in May 2078.[13][14]
Template:Mp is located in the classical region of the Kuiper belt 39–48 AU from the Sun,[15]Template:Rp and is thus classified as a classical Kuiper belt object or cubewano.[15]Template:Rp Template:Mp's high orbital inclination qualifies it as a dynamically "hot" member of the classical Kuiper belt, which implies that it was gravitationally scattered out to its present location by Neptune's outward planetary migration in the Solar System's early history.[16]Template:Rp Hence, Template:Mp is sometimes classified as a "scattered" object.[17][18]Template:Rp
Physical characteristics
| Year of Publication |
Diameter (km) |
Method | Refs |
|---|---|---|---|
| 2002 | Template:Val | thermal (IRAM)Script error: No such module "Check for unknown parameters". |
[6][19]Template:Rp |
| 2005 | Template:Val | thermal (Spitzer)Script error: No such module "Check for unknown parameters". |
[20][21] |
| 2008 | Template:Val | thermal (Spitzer)Script error: No such module "Check for unknown parameters". |
[18]Template:Rp |
| 2009 | Template:Val | thermal (Spitzer, remodeled)Script error: No such module "Check for unknown parameters". |
[22]Template:Rp |
| 2014 | Template:Val | thermal (Herschel + Spitzer)Script error: No such module "Check for unknown parameters". |
[23] |
Size, shape, and rotation
Measurements of Template:Mp's infrared thermal emission by the Herschel and Spitzer space telescopes give a diameter of Template:Val (Template:Val).[23] This makes Template:Mp one of the largest unnamed Solar System objects with a measured diameter, tied with Template:Mpl to within uncertainties (diameter Template:Val).[24] Template:Mp is large enough that some astronomers consider it a dwarf planet candidate.[25][26]Template:Rp Template:Mp's brightness fluctuates very little as it rotates, which could indicate a spheroidal shape.[26]Template:Rp
Template:Mp has a likely rotation period of around 8.8 hours, according to telescopic observations of its brightness changes over time. Template:Mp's subtle brightness variations (by up to 0.08 magnitudes) can make it difficult to determine its light curve and true rotation period.[27]Template:Rp The first measurements of Template:Mp's rotation period made during 2002–2003 obtained a likely period of Template:Val hours.[28]Template:Rp[29]Template:Rp Although other alias periods of 13.94, 6.49, and 15.82 hours are possible, the 8.86 hour period stood out as the most likely.[29]Template:Rp Another set of observations from 2003–2004 obtained a period of 8.78 hours.[27]Template:Rp
Surface
Template:Mp has a dark and moderately red surface with a geometric albedo of about 11%.[23] The visible and near-infrared spectrum of Template:Mp lacks obvious absorption features, which suggests that tholins mostly cover its surface.[30] (in contrast to Quaoar, also red)
See also
- 174567 Varda – a similar TNO by orbit, size and color
- List of Solar System objects by size
Notes
References
External links
- Cruikshank, D., et al. High Albedo KBO (55565)2002 AW197, The Astronomical Journal Letters, 624,53 (May 2004). Abstract
- Physical and dynamical characteristics of icy "dwarf planets" (plutoids), G. Tancredi, IAU Symposium No. 263 (2009)
- Kuiper Belt Object Magnitudes and Surface Colors Template:Webarchive, Stephen C. Tegler, June 2018
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- Template:AstDys
- Template:JPL small body
Template:Trans-Neptunian objects
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