(523643) 2010 TY 53
Asteroid (523643) 2010 TY 53 |
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Properties of the orbit ( animation ) | |
Orbit type |
TNO - Centaur , "Distant Object" |
Major semi-axis | 38.826 AU |
eccentricity | 0.457 |
Perihelion - aphelion | 21,066 AU - 56,586 AU |
Inclination of the orbit plane | 22.5 ° |
Length of the ascending node | 111.2 ° |
Argument of the periapsis | 3.4 ° |
Time of passage of the perihelion | January 2, 2043 |
Sidereal period | 241 a 11.1 M |
Mean orbital velocity | 4.741 km / s |
Physical Properties | |
Medium diameter | approx. 329 km |
Albedo | 0.08-0.10 |
Absolute brightness | 5.34 ± 0.03 - 5.8 mag |
Spectral class | C. |
history | |
Explorer | Pan-STARRS |
Date of discovery | 4th August 2010 |
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. |
(523643) 2010 TY 53 is a large trans-Neptunian object , which is classified dynamically as a centaur crossing Neptune orbit . Due to its size, the asteroid may be one of the dwarf planet candidates .
discovery
2010 TY 53 was discovered on August 4, 2010 by a team of astronomers as part of the Pan-STARRS project at the Haleakalā Observatory ( Maui ). The discovery was made after the confirmation by the Haleakala-Faulkes Telescope North and the Astronomical Research Observatory ( Illinois announced) September 10, 2011, the asteroid was on 25 September 2018 the IAU , the Minor Planet -number 523643 .
After its discovery in 2010, TY 53 could be identified on photos taken as part of the Near Earth Asteroid Tracking Program (NEAT) at the Palomar Observatory ( California ) going back to October 7, 2004, thus changing its observation period extend six years to calculate its orbit more accurately. Since then, the planetoid has been observed through various earth-based telescopes. In October 2018 there were a total of 184 observations over a period of 14 years. The last observation so far was again carried out in January 2018 at the Pan-STARRS telescope. (As of March 24, 2019)
properties
Orbit
2010 TY 53 orbits the sun in 241.93 years in a strongly elliptical orbit between 21.06 AU and 56.59 AU from its center. The orbital eccentricity is 0.457, the orbit is inclined 22.46 ° with respect to the ecliptic . The planetoid is currently 29.28 AU from the Sun. He will next pass through perihelion in 2043, so the last perihelion should have occurred in 1801.
Both Marc Buie ( DES ) and the Minor Planet Center classify the planetoid as a centaur ; the latter also generally lists it as a "distant object" .
size
A diameter of 329 km is currently assumed, based on a reflectivity of 8% and an absolute brightness of 5.8 m . Based on this diameter, the total surface area is around 340,000 km 2 . The apparent magnitude of 2010 TY 53 is 20.60 m .
Since it is conceivable that 2010 TY 53 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 2010 TY 53 to perhaps is a dwarf planet.
year | Dimensions km | source |
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2013 | 304.46 | LightCurve DataBase |
2018 | 321.0 | Johnston |
2018 | 329.0 | 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 523643 . SwRI (Space Science Department). Retrieved March 24, 2019.
- ↑ a b MPC : MPEC List Of Centaurs and Scattered-Disk Objects . IAU . Retrieved March 24, 2019.
- ↑ a b c Wm. R. Johnston: List of Known Trans-Neptunian Objects . Johnston's Archives. October 7, 2018. Accessed March 24, 2019.
- ↑ a b c (523643) 2010 TY53 at the IAU Minor Planet Center (English) Accessed March 24, 2019.
- ↑ v ≈ π * a / period (1 + sqrt (1-e²))
- ↑ S. Benecchi, S. Sheppard : Light Curves of 32 Large Transneptunian Objects (PDF) . In: The Astronomical Journal . 145, No. 5, January 24, 2013, p. 124, 19. arxiv : 1301.5791 . bibcode : 2013AJ .... 145..124B . doi : 10.1088 / 0004-6256 / 145/5/124 .
- ↑ a b LCDB Data for (523643) . MinorPlanetInfo. 2013. Accessed March 24, 2019.
- ↑ MPC : MPEC 2011-R36: 2010 TY53 . IAU . September 10, 2011. Accessed March 24, 2019.
- ↑ MPC : MPC / MPO / MPS Archive . IAU . Retrieved March 24, 2019. Reference there: MPC 111778
- ↑ (523643) 2010 TY53 in the Small-Body Database of the Jet Propulsion Laboratory (English). Retrieved March 24, 2019.
- ↑ MPC : MPEC 2010-S44: Distant Minor Planets (2010 OCT.11.0 TT) . IAU . September 25, 2010. Accessed March 24, 2019.
- ↑ (523643) 2010 TY53 in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).
- ↑ a b Mike Brown : How many dwarf planets are there in the outer solar system? . CalTech . November 12, 2018. Retrieved March 24, 2019.