702 Alauda
 | |
| Discovery[2] | |
|---|---|
| Discovered by | Joseph Helffrich |
| Discovery date | July 16, 1910 |
| Designations | |
| Pronunciation | /əˈlɔːdə/ ə-LAW-də |
| Alternative names | 1910 KQ |
| Minor planet category | Main belt |
| Orbital characteristics[2] | |
| Epoch June 18, 2009 (2455000.5) | |
| Aphelion | 3.2614 AU (Q) |
| Perihelion | 3.1238 AU (q) |
| Semi-major axis | 3.1926 AU (a) |
| Eccentricity | 0.02155 |
| Orbital period | 5.70 yr |
| Mean anomaly | 149.62° (M) |
| Inclination | 20.612° |
| Longitude of ascending node | 289.96° |
| Argument of perihelion | 353.32° |
| Known satellites | S/2007 (702) 1[3] |
| Physical characteristics | |
| Dimensions | 194.73 km[2] |
| Mass | (6.057 ± 0.36)×1018 kg³[4] |
| Mean density | (1.57 ± 0.5) g/cm³[4] |
| Albedo | 0.0587[2] |
| Spectral type | C-type |
| Apparent magnitude | 11.42 to 13.57[5] |
| Absolute magnitude (H) | 7.25[2] |
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702 Alauda is a large minor planet, measuring 194.73 km in diameter.[2] It was discovered in 1910 by Joseph Helffrich from the observatory at Heidelberg University. It is named after the lark (alauda). In 2007, a small moon, named Pichi üñëm, was discovered.
Satellite
Alauda's satellite was discovered from observations using adaptive-optics imaging with the European Southern Observatory (ESO) 8-m Very Large Telescope (VLT) on Cerro Paranal, Chile.[3] It is 5.5 km in diameter and has a projected separation from Alauda of 900 km.[6][7] It was named Pichi üñëm, meaning "little bird" in the Mapuche language of Chile, the country from which the moon was discovered.[8]
Orbital characteristics
Alauda has been identified as the largest member of a dynamical family.[3] Other members of this family include: 581 Tauntonia, 1101 Clematis, 1838 Ursa, 3139 Shantou, 3325 TARDIS, 4368 Pillmore, 5360 Rozhdestvenskij, 5815 Shinsengumi, and many others.[9] Alauda's moon may be a result of the collision that created the asteroid family.[3]
Physical characteristics
The discovery of Alauda's moon enabled Alauda's mass to be determined. Rojo and Margot (2010) have estimated its mass to be 6.06×1018 kg with a density of 1.57 g/cm³.[4]
Occultations
Alauda has been observed to occult stars on several occasions, providing important information on its size and shape. It produced occultations on 2001-07-12 and 2004-04-21.[10] It may have occulted an apparent magnitude 9.5 star in the constellation of Gemini on 2009-10-17 at 08:18 UT.[1] This event should have been visible from Uruguay, Argentina, and Chile.[1]
References
- ↑ 1.0 1.1 1.2 Steve Preston. "(702) Alauda / TYC 1920-00620-1 event on 2009 Oct 17, 08:18 UT". Asteroid Occultation Updates. Retrieved 2009-10-05.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 "JPL Small-Body Database Browser: 702 Alauda (1910 KQ)". 2009-02-15 last obs. Retrieved 2009-10-06.
- ↑ 3.0 3.1 3.2 3.3 Margot, Jean-Luc; Rojo, P. (2007). "Discovery of a Satellite to Asteroid Family Member (702) Alauda". American Astronomical Society 39: 440. Bibcode:2007DPS....39.1608M.
- ↑ 4.0 4.1 4.2 Rojo, P.; Margot, J. L. (2010). "Mass and Density of the B-type Asteroid (702) Alauda". The Astrophysical Journal 727 (2): 69. arXiv:1011.6577. Bibcode:2011ApJ...727...69R. doi:10.1088/0004-637X/727/2/69.
- ↑ Magnitudes generated with JPL Horizons for the year 1950 through 2100
- ↑ Daniel W. E. Green (2007-08-02). "Electronic Telegram No. 1016". IAU Central Bureau for Astronomical Telegrams. Retrieved 2011-07-05.
- ↑ "Asteroid and Dwarf Planet News". Retrieved 2009-10-06.
- ↑ New Names of Minor Planets PDF (2.19 MB)
- ↑ "Opposition dates and magnitudes for 702 family members (2004–2008)". Italian organization of minor planet observers. Retrieved 2009-10-05.
- ↑ David Dunham. "Observed asteroidal occultation list". Retrieved 2011-01-27.
External links
- Orbital simulation from JPL (Java) / Ephemeris
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