2008 ST291
Discovery[1] | |
---|---|
Discovered by |
M. E. Schwamb M. E. Brown D. L. Rabinowitz |
Discovery date | September 24, 2008 |
Designations | |
MPC designation | 2008 ST291 |
TNO (SDO)[2][3] | |
Orbital characteristics[4] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 5 | |
Observation arc | 745 days (2.04 yr) |
Aphelion | 154.47 AU (23.108 Tm) (Q) |
Perihelion | 42.400 AU (6.3429 Tm) (q) |
98.438 AU (14.7261 Tm) (a) | |
Eccentricity | 0.56927 (e) |
976.67 yr (356730 d) | |
22.781° (M) | |
Inclination | 20.8234° (i) |
331.1519° (Ω) | |
324.37° (ω) | |
Earth MOID | 41.4051 AU (6.19411 Tm) |
Jupiter MOID | 37.3733 AU (5.59097 Tm) |
Physical characteristics | |
Dimensions |
370–820 km[4][5] 612 km[6][7] |
22.2[1][8] | |
4.2[4] | |
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2008 ST291, also written as 2008 ST291, is a trans-Neptunian object with an absolute magnitude of 4.2,[4] making it possibly a dwarf planet.[9]
Size estimate
2008 ST291 is estimated to be about 612 kilometres (380 mi) in diameter, assuming a typical albedo of 0.09 for trans-Neptunian objects.[6] However, because its albedo is unknown and it has an absolute magnitude of 4.3,[4] it could be anywhere between 370 to 820 km in diameter.[5]
Distance
2008 ST291, currently 59.0 AU from the Sun,[8] came to perihelion around 1954[4] and will have moved beyond a distance of 60 AU by 2016. It takes over one thousand years to orbit the Sun. Of the known and suspected dwarf planets, only Sedna and 2005 QU182 are known to have longer orbits.
2008 ST291 has only been observed 26 times over three oppositions and has an orbit quality of 4 (0 being best; 9 being worst).[4]
Object name | Distance from the Sun (AU) | Magnitude (vmag) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Current | Perihelion | Aphelion | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
V774104 | 103 | N/A | N/A | 24 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Eris | 96.3 | 37.8 | 97.6 | 18.7 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2007 OR10 | 87.5 | 33.0 | 100.8 | 21.7 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Sedna | 85.7 | 76.0 | 939 | 21.0 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2014 FC69 | 84.2 | 40.3 | 106.9 | 24.1 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2006 QH181 | 83.4 | 37.8 | 96.7 | 23.6 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2012 VP113 | 83.3 | 80.5 | 438 | 23.4 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2013 FY27 | 80.3 | 36.1 | 81.8 | 22.1 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2010 GB174 | 70.8 | 48.7 | 693 | 25.1 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2000 CR105 | 60.5 | 44.3 | 412 | 23.9 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2008 ST291 | 59.9 | 42.4 | 154.5 | 22.2 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
2003 QX113 | 59.9 | 36.7 | 62.1 | 22.5 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Including all known objects currently located at least twice as far as Neptune.[10] See List of trans-Neptunian objects for more. |
See also
References
- 1 2 "MPEC 2009-V68 : 2008 ST291". IAU Minor Planet Center. 2009-11-14. Retrieved 2009-12-06.
- ↑ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2009-12-06.
- ↑ Marc W. Buie. "Orbit Fit and Astrometric record for 08ST291" (last observation: 2010-10-09 using 20 of 23 observations over 2.04 years). SwRI (Space Science Department). Retrieved 2009-12-06.
- 1 2 3 4 5 6 7 "JPL Small-Body Database Browser: (2008 ST291)" (last observation: 2010-10-09; arc: 2.04 years). Retrieved 28 March 2016.
- 1 2 "Absolute Magnitude (H)". NASA/JPL. Archived from the original on 26 November 2009. Retrieved 2009-12-06.
- 1 2 Dan Bruton. "Conversion of Absolute Magnitude to Diameter for Minor Planets". Department of Physics & Astronomy (Stephen F. Austin State University). Archived from the original on 10 December 2008. Retrieved 2008-12-09.
- ↑ Assuming an albedo of 0.09
- 1 2 "AstDyS 2008 ST291 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2014-03-28.
- ↑ "How many dwarf planets are there in the outer solar system?". Gps.caltech.edu. 2015-07-21. Retrieved 2015-07-22.
- 1 2 "AstDyS-2, Asteroids - Dynamic Site". 2016-02-26. Retrieved 2016-02-29.
Objects with distance from Sun over 59 AU
External links
- Orbital simulation from JPL (Java) / Horizons Ephemeris
- 2008 ST291 at the JPL Small-Body Database
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