(153591) 2001 SN263
Discovery [1] | |
---|---|
Discovered by | LINEAR |
Discovery site | Lincoln Lab's ETS |
Discovery date | 20 September 2001 |
Designations | |
MPC designation | (153591) 2001 SN263 |
2001 SN263 | |
NEO · Amor [1][2] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 25.18 yr (9,198 days) |
Aphelion | 2.9368 AU |
Perihelion | 1.0363 AU |
1.9865 AU | |
Eccentricity | 0.4783 |
2.80 yr (1,023 days) | |
148.57° | |
0° 21m 7.2s / day | |
Inclination | 6.6853° |
325.83° | |
172.86° | |
Known satellites | 2[3] |
Earth MOID | 0.0520 AU · 20.3 LD |
Physical characteristics | |
Mean diameter |
2 km[3] ±0.3 km 2.5[4] km 2.6[5] ±0.40 km 2.63[6] |
Mass | ±2.2)×1010 kg (917.5[7] |
Mean density | ±0.2 g/cm³ 1.1[4] |
±0.01 3.20h[8] ±0.001 h 3.423[lower-alpha 1] 10±0.00007 h 3.425[9] ±0.0002 h 3.4256[4] | |
±0.015 0.048[6] | |
C [8] · B [lower-alpha 2] | |
16.81[10] · 16.9[1] | |
|
(153591) 2001 SN263 is a carbonaceous trinary[3] asteroid, classified as near-Earth object and former potentially hazardous asteroid of the Amor group, approximately 2.6 kilometers in diameter.
It was discovered by the Lincoln Near-Earth Asteroid Research project at Lincoln Lab's Experimental Test Site in Socorro, New Mexico, on 20 September 2001.[2]
The two synchronous minor-planet moons measure approximately 770 and 430 meters and have an orbital period of 16.46 and 150 hours, respectively.[4][10]
Primary
2001 SN263, the primary object of this trinary system, is an unusual carbonaceous near-Earth asteroid of a C- or somewhat brighter B-type.[8][lower-alpha 2] It orbits the Sun at a distance of 1.0–2.9 AU once every 2 years and 10 months (1,023 days). Its orbit has an eccentricity of 0.48 and an inclination of 7° with respect to the ecliptic.[1] A first precovery was taken at Palomar Observatory during the Digitized Sky Survey in 1990, extending the body's observation arc by 11 years prior to its official discovery observation at Socorro.[2]
It has an Earth minimum orbital intersection distance (MOID) of 0.0520 AU (7,780,000 km), which translates into 20.3 lunar distances.[1] With an Earth MOID above 0.05 AU, 2001 SN263 is no longer a potentially hazardous asteroid, but it was classified as such by the MPC until early 2017.[2][11]
Radar observations show that it measures 2.5 kilometers in diameter.[4] Its surface has a low albedo of 0.048.[6] Rotational lightcurves obtained from photometric observations gave a rotation period of 3.423 hours (best result) with a brightness variation between 0.13 and 0.27 magnitude (U=2/3/3).[8][9][lower-alpha 1] Radar observations gave a concurring period of 3.4256 hours, and subsequent modeling of both radiometric and photometric observations gave a spin axis of (309.0°, −80.0°) in ecliptic coordinates (λ, β).[4]
Trinary system
In 2008, scientists using the planetary radar at Arecibo Observatory discovered that the object is orbited by two satellites, when the triple asteroid made a close approach to Earth of 0.066 AU (nearly 10 million kilometers). The largest body (preliminarily called Alpha) is spheroid in shape, with principal axes of ±0.1 2.8 km, ±0.1 2.7 km, and ±0.3 2.9 km, with an effective diameter of ±0.3 2.5 km and a density of ±0.2 g/cm3. The satellites, named Beta and Gamma, are several times smaller in size. Beta is 1.1±0.12 0.77 km in diameter and Gamma ±0.14 0.43 km.[4]
The only other unambiguously identified triple asteroids in the near-Earth population are (136617) 1994 CC, which was discovered to be a triple system in 2009, and 3122 Florence, which was found to be a triple system in September 2017.[12]
Orbital characteristics of satellites
The orbital properties of the satellites are listed in this table.[7] The orbital planes of both satellites are inclined relative to each other; the relative inclination is about 14 degrees. Such a large inclination is suggestive of past evolutionary events (e.g. close encounter with a terrestrial planet, mean-motion-resonance crossing) that may have excited their orbits from a coplanar configuration to an inclined state.
Name | Mass | Semi-major axis | Orbital period | Eccentricity |
---|---|---|---|---|
Gamma (inner) | ~10×1010 kg | 3.8 km | 0.686 days | 0.016 |
Beta (outer) | ~24×1010 kg | 16.6 km | 6.225 days | 0.015 |
Numbering and naming
This minor planet was numbered by the Minor Planet Center on 2 April 2007.[13] As of 2018, the primary and its moons have not been named.[2] In the scientific literature, the components of the trinary system are generically referred to as Alpha, Beta and Gamma, but these labels are not recognized by the IAU.[5][4]
Notes
- 1 2 Warner (2011) web: lightcurve plot of (153591) 2001 SN263, Palmer Divide Observatory, Brian D. Warner (2008). Photometric observations from 20 February 2008: rotation period ±0.001 hours with a brightness amplitude of 3.423±0.02 magnitude. Quality code: 3. Summary figures for all obtained lightcurves at 0.14Collaborative Asteroid Lightcurve Link (CALL) for (153591)
- 1 2 Perna (2014): photometric observation from 24 June 2011: with a brightness amplitude of mag. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (153591)
References
- 1 2 3 4 5 6 "JPL Small-Body Database Browser: 153591 (2001 SN263)" (2015-12-01 last obs.). Jet Propulsion Laboratory. Retrieved 1 June 2017.
- 1 2 3 4 5 "153591 (2001 SN263)". Minor Planet Center. Retrieved 3 September 2017.
- 1 2 3 Nolan, M. C.; Howell, E. S.; Benner, L. A. M.; Ostro, S. J.; Giorgini, J. D.; Busch, M. W.; et al. (February 2008). "(153591) 2001 SN_263". Central Bureau Electronic Telegrams (1254). Bibcode:2008CBET.1254....1N. Retrieved 22 March 2017.
- 1 2 3 4 5 6 7 8 Becker, Tracy M.; Howell, Ellen S.; Nolan, Michael C.; Magri, Christopher; Pravec, Petr; Taylor, Patrick A.; et al. (March 2015). "Physical modeling of triple near-Earth Asteroid (153591) 2001 SN263 from radar and optical light curve observations". Icarus. 248: 499–515. Bibcode:2015Icar..248..499B. doi:10.1016/j.icarus.2014.10.048. Retrieved 22 March 2017.
- 1 2 Becker, Tracy; Howell, E. S.; Nolan, M. C.; Magri, C. (September 2008). "Physical Modeling of Triple Near-Earth Asteroid 153591 (2001 SN263)". American Astronomical Society. 40: 437. Bibcode:2008DPS....40.2806B. Retrieved 22 March 2017.
- 1 2 3 Delbo, Marco; Walsh, Kevin; Mueller, Michael; Harris, Alan W.; Howell, Ellen S. (March 2011). "The cool surfaces of binary near-Earth asteroids". Icarus. 212 (1): 138–148. Bibcode:2011Icar..212..138D. doi:10.1016/j.icarus.2010.12.011. Retrieved 22 March 2017.
- 1 2 Fang, Julia; Margot, Jean-Luc; Brozovic, Marina; Nolan, Michael C.; Benner, Lance A. M.; Taylor, Patrick A. (May 2011). "Orbits of Near-Earth Asteroid Triples 2001 SN263 and 1994 CC: Properties, Origin, and Evolution". The Astronomical Journal. 141 (5): 15. arXiv:1012.2154. Bibcode:2011AJ....141..154F. doi:10.1088/0004-6256/141/5/154. Retrieved 1 June 2017.
- 1 2 3 4 Betzler, Alberto Silva; Novaes, Alberto Brum; Celedon, Julian Hermogenes Quesada (October 2008). "A Study of the Trinary NEA 2001 SN263". The Minor Planet Bulletin. 35 (4): 182–184. Bibcode:2008MPBu...35..182B. ISSN 1052-8091. Retrieved 22 March 2017.
- 1 2 Oey, Julian (January 2009). "Lightcurve Analysis of Asteroids from Leura and Kingsgrove Observatories in the First Half of 2008". The Minor Planet Bulletin. 36 (1): 4–6. Bibcode:2009MPBu...36....4O. ISSN 1052-8091. Retrieved 22 March 2017.
- 1 2 "LCDB Data for (153591)". Asteroid Lightcurve Database (LCDB). Retrieved 3 September 2017.
- ↑ "153591 (2001 SN263)". Minor Planet Center. web.archive.org. 22 March 2017. Archived from the original on 22 March 2017. Retrieved 3 September 2017.
- ↑ "Radar Reveals Two Moons Orbiting Asteroid Florence". Jet Propulsion Laboratory. September 1, 2017.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 February 2018.
External links
- CBET No. 1254 – (153591) 2001 SN263, Central Bureau for Astronomical Telegrams
- Robert Roy Britt, Triple Asteroid Found Near Earth, Space.com, 13 Feb 2008
- Emily Lakdawalla, Triple Near-Earth Asteroid Discovered The Planetary Society, 13 Feb 2008
- Images of the asteroid and its moons
- A Lander to Investigate a C-type Triple Near-Earth Asteroid System: 2001 SN263
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- (153591) 2001 SN263 at the JPL Small-Body Database