Astronomy:2201 Oljato
| Discovery [1] | |
|---|---|
| Discovered by | H. L. Giclas |
| Discovery site | Lowell Obs. |
| Discovery date | 12 December 1947 |
| Designations | |
| (2201) Oljato | |
| Named after | Oljato–Monument Valley (Navajo Reservation)[2] |
| 1947 XC · 1979 VU2 1979 XA | |
| Minor planet category | NEO · PHA · Amor [1][3] |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 84.90 yr (31,008 days) |
| Earliest precovery date | 3 December 1931 |
| |{{{apsis}}}|helion}} | 3.7257 AU |
| |{{{apsis}}}|helion}} | 0.6243 AU |
| 2.1750 AU | |
| Eccentricity | 0.7130 |
| Orbital period | 3.21 yr (1,172 days) |
| Mean anomaly | 255.69° |
| Inclination | 2.5224° |
| Longitude of ascending node | 74.991° |
| 98.264° | |
| Earth MOID | 0.0031 AU · 1.2 LD |
| Physical characteristics | |
| Dimensions | 1.80±0.1 km (IRAS:11)[4] 2.15 km[5] |
| Rotation period | 24 h[6] 26 h[lower-alpha 1] |
| Geometric albedo | 0.24[5] 0.4328±0.030 (IRAS:11)[4] |
| SMASS = Sq [1] · C [7] · S [8][9] | |
| Absolute magnitude (H) | 15.00[9] · 15.25[1][4] · 15.50[5][8] · 15.50±0.42[7] · 15.55[6] |
2201 Oljato, provisional designation 1947 XC, is a stony and extremely eccentric active[10] asteroid and sizable near-Earth object of the Apollo group, approximately 2 kilometers in diameter. It has an Earth minimum orbit intersection distance of 0.0031 astronomical unit|AU (460 thousand km) and is associated with the Beta Taurids daytime meteor shower.
Discovery
Oljato was discovered by American astronomer Henry L. Giclas at the U.S Lowell Observatory in Flagstaff, Arizona, on 12 December 1947.[3] After its discovery, this near-Earth Apollo asteroid became a lost asteroid for 32 years and was recovered under the provisional designation 1979 XA, by the American astronomers Passey and Bus at the Californian Palomar Observatory in 1979.[2]
Orbit and classification
Oljato is a member of the Apollo asteroids, a subgroup of near-Earth asteroids which cross the orbit of Earth. It is also a potentially hazardous object due to its size and its Earth minimum orbit intersection distance (MOID) of 0.0031 astronomical unit|AU (460,000 km), which is only about 1.2 lunar distances . It orbits the Sun at a distance of 0.6–3.7 AU once every 3 years and 3 months (1,172 days). Its orbit has an eccentricity of 0.71 and an inclination of 3° with respect to the ecliptic.[1]
It was a target of Hubble search for transition comets, a spectroscopic study involving amateur astronomers and the use of the Hubble Space Telescope. The asteroid belongs to the Taurid Complex (also see Taurids), a group of near-Earth asteroids thought to be extinct cometary nuclei, that are associated with four meteor showers on Earth, due to their disintegration. The Taurid Complex includes several other Apollo asteroids such as 4183 Cuno, 4341 Poseidon, 5143 Heracles, and 5731 Zeus.[11]
Close approaches
The next notable close approach to Earth will be on 28 November 2024, passing at a nominal distance of 0.47 AU (70,000,000 km; 44,000,000 mi).[1] Due to the eccentricity of its orbit, Earth is not the only planet it passes. In 2044 it will pass close to Venus (on 24 Apr at 0.08 AU) as well as Earth (on 30 May at 0.129 AU), and in 2046 it will pass Jupiter (on 15 Jan at 1.4 AU). However, although it crosses the orbit of Mars, it will pass Earth, Venus and Jupiter several times before the next notable close approach to Mars, which will not be until 30 July 2127, passing at a nominal distance of 0.0306 AU (4,580,000 km; 2,840,000 mi)[1]
Physical characteristics
Oljato has a rotation period of 26 hours.[lower-alpha 1] The stony asteroid is classified as a Sq-subtype in the SMASS taxonomic scheme, with a geometric albedo of 0.24.[5] An alternative and exceptionally high albedo of 0.43 was determined by 11 observations from the Infrared Astronomical Satellite, IRAS.[4]
Naming
This minor planet was named after the Oljato–Monument Valley in Utah, on the Navajo Indian Reservation.[2] The official naming citation was published by the Minor Planet Center on 28 March 1983 (M.P.C. 7782).[12]
Notes
- ↑ 1.0 1.1 Pravec (1995) web: rotation period 26 hours with a brightness amplitude of 0.1 mag. Summary figures for (2201) Oljato at Collaborative Asteroid Lightcurve Link (CALL)
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 "JPL Small-Body Database Browser: 2201 Oljato (1947 XC)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002201;cad=1. Retrieved 11 June 2017.
- ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(2201) Oljato". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 179. doi:10.1007/978-3-540-29925-7_2202. ISBN 978-3540002383.
- ↑ 3.0 3.1 "2201 Oljato (1947 XC)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=2201. Retrieved 7 December 2016.
- ↑ 4.0 4.1 4.2 4.3 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 22 October 2019.
- ↑ 5.0 5.1 5.2 5.3 Harris, Alan W. (February 1998). "A Thermal Model for Near-Earth Asteroids". Icarus 131 (2): 291–301. doi:10.1006/icar.1997.5865. Bibcode: 1998Icar..131..291H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1998Icar..131..291H. Retrieved 15 December 2015.
- ↑ 6.0 6.1 Harris, A. W.; Young, J. W. (April 1983). "Asteroid rotation. IV". Icarus 54 (1): 59–109. doi:10.1016/0019-1035(83)90072-6. ISSN 0019-1035. Bibcode: 1983Icar...54...59H. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1983Icar...54...59H. Retrieved 15 December 2015.
- ↑ 7.0 7.1 Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 – Preliminary results". Icarus 261: 34–47. doi:10.1016/j.icarus.2015.08.007. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 7 December 2016.
- ↑ 8.0 8.1 "LCDB Data for (2201) Oljato". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2201%7COljato. Retrieved 7 December 2016.
- ↑ 9.0 9.1 Carry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry". Icarus 268: 340–354. doi:10.1016/j.icarus.2015.12.047. Bibcode: 2016Icar..268..340C. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016Icar..268..340C. Retrieved 7 December 2016.
- ↑ Jewitt, David; Hsieh, Henry; Agarwal, Jessica (2015). "The Active Asteroids". in Michel, P.; others. Asteroids IV. University of Arizona. pp. 221–241. doi:10.2458/azu_uapress_9780816532131-ch012. ISBN 978-0816532131. Bibcode: 2015aste.book..221J. http://www2.ess.ucla.edu/~jewitt/papers/2015/JHA15.pdf. Retrieved 2020-01-30.
- ↑ Babadzhanov, P. B. (2001). "Search for meteor showers associated with Near-Earth Asteroids". Astronomy and Astrophysics 373 (1): 329–335. doi:10.1051/0004-6361:20010583. Bibcode: 2001A&A...373..329B.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. Retrieved 7 December 2016.
External links
- Search for meteor showers associated with Near-Earth Asteroids – P. B. Babadzhanov, 2001
- Asteroid Lightcurve Database (LCDB), query form (info )
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- 2201 Oljato at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
- 2201 Oljato at ESA–space situational awareness
- 2201 Oljato at the JPL Small-Body Database
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