Astronomy:2006 QH181
Hubble Space Telescope image of 2006 QH181 taken in 2010 | |
Discovery | |
---|---|
Discovered by | CTIO |
Discovery date | 21 August 2006 |
Designations | |
2006 QH181 | |
Minor planet category | |
Orbital characteristics[4] | |
Epoch 13 January 2016 (JD 2457400.5)[4] | |
Uncertainty parameter 6 | |
Observation arc | 2634 days (7.21 yr) |
|{{{apsis}}}|helion}} | 96.680 astronomical unit|AU (14.4631 Tm) (Q) |
|{{{apsis}}}|helion}} | 37.789 AU (5.6532 Tm) (q) |
67.235 AU (10.0582 Tm) (a) | |
Eccentricity | 0.43795 (e) |
Orbital period | 551.31 yr (201366 d) |
Mean anomaly | 102.28° (M) |
Mean motion | 0° 0m 6.436s / day (n) |
Inclination | 19.144° (i) |
Longitude of ascending node | 73.840° (Ω) |
211.02° (ω) | |
Earth MOID | 36.7863 AU (5.50315 Tm) |
Jupiter MOID | 32.6588 AU (4.88569 Tm) |
Physical characteristics | |
Dimensions | |
Apparent magnitude | 23.6[7] |
Absolute magnitude (H) | 4.3[4] |
2006 QH181, also written as 2006 QH181, is a trans-Neptunian object (TNO) in the scattered disc.[2][3] Its orbit is currently too poorly determined (U=6)[4] to know whether it is in a resonance with Neptune.
Distance
It came to perihelion around 1858.[4] It is currently 83.8 AU from the Sun[7] and moving away from the Sun at 1.04 kilometers per second (2,300 miles per hour).[8] The only large objects currently farther from the Sun are Eris (96.1 AU),[9] 2014 UZ224 (90.9 AU), 2015 TH367 (~89 AU), Gonggong (88.0 AU),[10] Sedna (85.1 AU),[11] 2013 FS28 (84.8 AU), and 2014 FC69 (84.7 AU). Because it is so far from the Sun, it only has an apparent magnitude of 23.6.[7]
Orbit
It has been observed 15 times over only three oppositions and thus currently has a somewhat poorly known orbit. JPL ranks orbital quality from 0 to 9 (0 being best), and 2006 QH181 is currently listed with an orbit quality of 6.[4][12]
See also
- List of Solar System objects most distant from the Sun
References
- ↑ "MPEC 2008-O05 : Distant Minor Planets". Minor Planet Center & Tamkin Foundation Computer Network. 2008-07-17. http://cfa-www.harvard.edu/iau/mpec/K08/K08O05.html.
- ↑ 2.0 2.1 "List Of Centaurs and Scattered-Disk Objects". MPC. http://www.minorplanetcenter.org/iau/lists/Centaurs.html.
- ↑ 3.0 3.1 Marc W. Buie (2008-03-05). "Orbit Fit and Astrometric record for 06QH181". SwRI (Space Science Department). http://www.boulder.swri.edu/~buie/kbo/astrom/06QH181.html.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 "JPL Small-Body Database Browser: (2006 QH181)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2006QH181.
- ↑ "Absolute Magnitude (H)". NASA/JPL. http://neo.jpl.nasa.gov/glossary/h.html.
- ↑ Wm. Robert Johnston. "List of Known Trans-Neptunian Objects". Johnston's Archive. http://www.johnstonsarchive.net/astro/tnoslist.html.
- ↑ 7.0 7.1 7.2 "AstDyS 2006QH181 Ephemerides". Department of Mathematics, University of Pisa, Italy. https://newton.spacedys.com/astdys/index.php?pc=1.1.3.0&n=2006QH181.
- ↑ "Horizon Online Ephemeris System". California Institute of Technology, Jet Propulsion Laboratory. http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2006QH181.
- ↑ "AstDyS (136199) Eris Ephemerides". Department of Mathematics, University of Pisa, Italy. https://newton.spacedys.com/astdys/index.php?pc=1.1.3.0&n=Eris.
- ↑ "AstDyS 2007OR10 Ephemerides". Department of Mathematics, University of Pisa, Italy. https://newton.spacedys.com/astdys/index.php?pc=1.1.3.0&n=2007OR10.
- ↑ "AstDyS (90377) Sedna Ephemerides". Department of Mathematics, University of Pisa, Italy. https://newton.spacedys.com/astdys/index.php?pc=1.1.3.0&n=Sedna.
- ↑ "2006 QH181". Minor Planet Center, IAU. http://www.minorplanetcenter.net/db_search/show_object?object_id=2006+QH181.
External links
- 2006 QH181 at AstDyS-2, Asteroids—Dynamic Site
- 2006 QH181 at the JPL Small-Body Database