(168703) 2000 GP 183
Asteroid (168703) 2000 GP 183 |
|
---|---|
Properties of the orbit ( animation ) | |
Orbit type |
CKBO ( "Cold" ) "Distant Object" |
Major semi-axis | 40.1 AU |
eccentricity | 0.082 |
Perihelion - aphelion | 36.799 AU - 43.402 AU |
Inclination of the orbit plane | 4.9 ° |
Length of the ascending node | 23.4 ° |
Argument of the periapsis | 221.1 ° |
Time of passage of the perihelion | March 21, 2023 |
Sidereal period | 253 a 11.3 M |
Mean orbital velocity | 4.665 km / s |
Physical Properties | |
Medium diameter | approx. 359 km |
Albedo | 0.04-0.09 |
Absolute brightness | 6.2 - 6.3 mag |
history | |
Explorer |
Chadwick A. Trujillo Jane X. Luu David C. Jewitt David J. Tholen Scott S. Sheppard |
Date of discovery | April 2, 2000 |
Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items. |
(168703) 2000 GP 183 is a large trans-Neptunian object in the Kuiper belt , which is classified as Cubewano (CKBO) in terms of railway dynamics . Due to its size, the asteroid may be one of the dwarf planet candidates .
discovery
2000 GP 183 was examined on April 2, 2000 by a team of astronomers consisting of Chad Trujillo , Jane Luu , Dave Jewitt , David Tholen and Scott Sheppard with the 3.6 m CFHT telescope at the Mauna Kea Observatory ( Hawaii ) discovered. The discovery was announced on July 22, 2000 together with Borasisi , the planetoid was later given the minor planet number 168703 by the IAU .
The observation arc of the planetoid begins with the official discovery observation on April 2, 2000. Since then, the planetoid has been observed through various earth-based telescopes. In April 2017, a total of 145 observations over a period of 16 years were available. The last observation so far was carried out in April 2017 at the Pan-STARRS telescope (PS1) ( Maui ). (As of March 15, 2019)
properties
Orbit
2000 GP 183 orbits the sun in 253.94 years on a slightly elliptical orbit between 36.80 AU and 43.40 AU from its center. The orbital eccentricity is 0.082, the orbit is inclined 4.91 ° to the ecliptic . Currently, the planetoid is 36.82 AU from the sun. He will next pass perihelion in 2023, so the last perihelion should have occurred in 1769.
Marc Buie ( DES ) classifies the asteroid as a Cubewano , whereby it belongs to the orbital dynamics "cold" classical KBO , while the Minor Planet Center does not have a specific classification; the latter classifies it as a non-SDO and generally as a “distant object” .
size
A diameter of 359 km is currently assumed, based on a reflectivity of 4% and an absolute brightness of 6.3 m . Based on this diameter, the total area is around 405,000 km². The apparent magnitude of 2000 GP 183 is 21.91 m .
Since it is conceivable that 2000 GP 183 is in hydrostatic equilibrium due to its size and could thus be largely round, it may meet the criteria for classification as a dwarf planet . Mike Brown expects that it is at 2000 GP 183 to perhaps is a dwarf planet.
2000 GP 183 seems to have a bluish (neutral) coloration, which is why the albedo is assumed to be comparatively low.
year | Dimensions km | source |
---|---|---|
2018 | 280.0 | Johnston |
2018 | 359.0 | Brown |
The most precise determination is marked in bold . |
See also
- List of trans-Neptunian objects
- List of dwarf planets of the solar system
- List of asteroids
- List of moons from asteroids
Web links
- How many dwarf planets are there in the outer solar system? Current list of the largest TNOs from Mike Brown
- Free the dwarf planets! Mike Brown's column on the IAU and the dwarf planets regarding their classifications (23 August 2011)
Individual evidence
- ^ A b Marc W. Buie : Orbit Fit and Astrometric record for 168703 . SwRI (Space Science Department). Retrieved March 15, 2019.
- ↑ a b c Wm. R. Johnston: List of Known Trans-Neptunian Objects . Johnston's Archives. October 7, 2018. Retrieved March 15, 2019.
- ↑ a b c (168703) 2000 GP183 at the IAU Minor Planet Center (English) Retrieved March 15, 2019.
- ↑ v ≈ π * a / period (1 + sqrt (1-e²))
- ↑ MPC : MPEC 2000-O12: 1999 RZ253, 2000 GP183 . IAU . July 22, 2000. Retrieved March 15, 2019.
- ↑ MPC : MPC / MPO / MPS Archive . IAU . Retrieved March 15, 2019.
- ↑ (168703) 2000 GP183 in the Small-Body Database of the Jet Propulsion Laboratory (English). Retrieved March 15, 2019.
- ↑ MPC : MPEC List Of Centaurs and Scattered-Disk Objects . IAU . Retrieved March 15, 2019.
- ↑ (168703) 2000 GP183 in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).
- ↑ a b c Mike Brown : How many dwarf planets are there in the outer solar system? . CalTech . November 12, 2018. Retrieved March 15, 2019.