(225088) 2007 OR10
Artist's impression of (225088) 2007 OR10
|Discovered by||M. E. Schwamb
M. E. Brown
D. L. Rabinowitz
Palomar Observatory (675)
|MPC designation||(225088) 2007 OR10|
|Minor planet category||3:10 resonance (DES)|
|Epoch February 8, 2011|
|Aphelion||100.79 AU (15.1 Tm)|
|Perihelion||33.62 AU (5.03 Tm)|
|Semi-major axis||67.21 AU (10.054 Tm)|
|Orbital period||550.98 yr|
|Mean anomaly||101.0° (M)|
|Longitude of ascending node||336.86°|
|Argument of perihelion||207.18°|
−200 km (fit to volatile-retention model)
|Absolute magnitude (H)||1.9|
(225088) 2007 OR10 is a very large trans-Neptunian object located in the scattered disc. It is the largest known body in the Solar System without a name, approximately the size of Haumea, and appears to be a dwarf planet.
2007 OR10 was discovered by California Institute of Technology astronomers as part of the PhD thesis of Meg Schwamb, who was at the time a graduate student of Michael E. Brown. Brown nicknamed the object "Snow White" for its presumed white color, as it would have to be very large or very bright to be detected by their survey. It was also the "seventh dwarf" discovered by Brown's team, after Quaoar in 2002, Sedna in 2003, Haumea and Orcus in 2004, and Makemake and Eris in 2005. However, "Snow White" turned out to be one of the reddest objects in the Kuiper belt, comparable only to Quaoar, making the nickname inappropriate.
2007 OR10 is currently the largest known object in the Solar System without an official name. In 2011 Brown decided he finally had enough information to justify giving it one, because the discovery of water ice and the possibility of methane makes it noteworthy enough to warrant further study.
2007 OR10 came to perihelion around 1857. It is currently 87.0 AU from the Sun. This makes it the second-farthest known large body in the Solar System, after Eris (97 AU), and farther out than Sedna (86.3 AU). It has been farther from the Sun than Sedna since 2013. 2007 OR10 will be farther than both Sedna and Eris by 2045, and it will reach aphelion in 2130.
The size of an object can be calculated from its absolute magnitude (H) and the albedo (the amount of light it reflects). 2007 OR10 has an absolute magnitude (H) of 1.92, which makes it the fifth-brightest TNO known, a little less bright than Sedna (H=1.6; D=1,000 km) and brighter than Orcus (H=2.3; D≈800 km).
Surface composition and atmosphere
The spectrum of 2007 OR10 shows signatures for both water ice and methane, which makes it similar in composition to Quaoar. The presence of red methane frost on the surfaces of both 2007 OR10 and Quaoar implies the existence of a tenuous methane atmosphere on both objects, slowly evaporating into space. Although 2007 OR10 comes closer to the Sun than Quaoar, and is thus warm enough that a methane atmosphere should evaporate, its larger mass makes retention of an atmosphere just possible. The presence of water ice on the surface of 2007 OR10 implies a brief period of cryovolcanism in its distant past.
Semi-major axis and orbital period
The Deep Ecliptic Survey (DES) shows the orbit to be in a 3:10 resonance with Neptune. The MPC lists it as a scattered-disc object. 2007 OR10 was discovered when searching for objects in the region of Sedna.
It was formally announced on January 7, 2009.
The orbit of 2007 OR10 compared to the orbit of Eris and Pluto.
The motion of 2007 OR10 librating in a 3:10 resonance with Neptune.
Brown states that 2007 OR10 "must be a dwarf planet even if predominantly rocky", and Scott Sheppard et al. believe it is "likely" to be one, based on its minimum possible diameter (552 km) and what is understood of the conditions for hydrostatic equilibrium in cold icy and rocky bodies. However, the IAU has not classified it as a dwarf planet. It has not been proven that a TNO of 552 km will necessarily be in equilibrium. It is too distant to resolve its diameter directly; Brown's estimate of 1,000–1,500 km is based on calculating the albedo that is the best fit in his model, though this agrees with the 1,070–1,490 km determined from observations by the Herschel space observatory. 2007 OR10 has no known satellite, and without a satellite with a well-determined orbit its mass cannot be calculated directly (see three-body problem); mass is also a factor in hydrostatic equilibrium.
- "MPEC 2009-A42 : 2007 OR10". Minor Planet Center. 2009-01-07. Retrieved 2009-01-20.
- "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2009-01-20.
- Marc W. Buie (2008-08-23). "Orbit Fit and Astrometric record for 225088". SwRI (Space Science Department). Retrieved 2009-03-11.
- "JPL Small-Body Database Browser: 225088 (2007 OR10)". 2009-11-06 last obs. Retrieved 2011-01-02.
- Santos-Sanz, P., Lellouch, E., Fornasier, S., Kiss, C., Pal, A., Müller, T. G., Vilenius, E., Stansberry, J., Mommert, M., Delsanti, A., Mueller, M., Peixinho, N., Henry, F., Ortiz, J. L., Thirouin, A., Protopapa, S., Duffard, R., Szalai, N., Lim, T., Ejeta, C., Hartogh, P., Harris, A. W., & Rengel, M. (2012). “TNOs are Cool”: A Survey of the Transneptunian Region IV - Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS
- Michael E. Brown; Burgasser, A.J.; Fraser W.C. (2011). "The Surface Composition of Large Kuiper Belt Object 2007 OR10". Mike Brown's Website. arXiv:1108.1418. Retrieved 2011-08-08.
- "AstDys 2007OR10 Ephemerides". Department of Mathematics, University of Pisa, Italy. Archived from the original on 2009-05-17. Retrieved 2009-03-16.
- Michael E. Brown (2009-03-10). "Snow White needs a bailout". Mike Brown's Planets (blog). Archived from the original on 2009-05-17. Retrieved 2010-02-17.
- "Astronomers Find Ice and Possibly Methane On Snow White, a Distant Dwarf Planet". Science Daily. August 22, 2011. Retrieved 2011-08-22.
- "Horizon Online Ephemeris System". California Institute of Technology, Jet Propulsion Laboratory. Retrieved 2012-01-31.
- JPL Horizons On-Line Ephemeris System (2011-02-17). "Horizons Output for Sedna 2076/2114". Retrieved 2011-02-17.
- Mike Brown (2011). "The Redemption of Snow White (Part 2 of 3)". Mike Brown's Planets. Retrieved 2012-02-08.
- "JPL Small-Body Database Browser: 90377 Sedna (2003 VB12)". 2008-10-23 last obs. Retrieved 2009-01-21.
- "JPL Small-Body Database Browser: 90482 Orcus (2004 DW)". 2008-12-04 last obs. Retrieved 2009-02-05.
- Mike Brown (2011). "The Redemption of Snow White (Part 3 of 3)". Mike Brown's Planets. Retrieved 2011-08-23.
- Schwamb, Megan E.; Michael E. Brown, David L. Rabinowitz (2009). "A Search for Distant Solar System Bodies in the Region of Sedna". Astrophysical Journal Letters. arXiv:0901.4173. Bibcode:2009ApJ...694L..45S. doi:10.1088/0004-637X/694/1/L45.
- Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Retrieved 2011-09-23.
- Sheppard, Scott S.; Trujillo, C.; Udalski, A,; et al. (2011). "A Southern Sky and Galactic Plane Survey for Bright Kuiper Belt Objects". Astronomical Journal 142 (4). arXiv:1107.5309. Bibcode:2011AJ....142...98S. doi:10.1088/0004-6256/142/4/98.
|Wikimedia Commons has media related to (225088) 2007 OR10.|
- Orbital simulation from JPL (Java) / Horizons Ephemeris
- 2007 OR10 Precovery Images
- 2007 OR10 Minor planet designation number
- The redemption of Snow White (Part 1) (Mike Brown blog 9 Aug 2011)