Astronomy:335 Roberta
Orbital diagram | |
Discovery | |
---|---|
Discovered by | Anton Staus |
Discovery date | 1 September 1892 |
Designations | |
(335) Roberta | |
Named after | Carl Robert Osten-Sacken |
1892 C | |
Minor planet category | Main belt |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 123.58 yr (45137 d) |
|{{{apsis}}}|helion}} | 2.9014 astronomical unit|AU (434.04 Gm) |
|{{{apsis}}}|helion}} | 2.04926 AU (306.565 Gm) |
2.47530 AU (370.300 Gm) | |
Eccentricity | 0.17212 |
Orbital period | 3.89 yr (1422.5 d) |
Average Orbital speed | 18.93 km/s |
Mean anomaly | 355.460° |
Mean motion | 0° 15m 11.095s / day |
Inclination | 5.1005° |
Longitude of ascending node | 148.454° |
140.006° | |
Earth MOID | 1.03587 AU (154.964 Gm) |
Jupiter MOID | 2.2733 AU (340.08 Gm) |
TJupiter | 3.456 |
Physical characteristics | |
Dimensions | 89.07±2.0 km[1] |
Rotation period | 12.054 h (0.5023 d) |
Geometric albedo | 0.0580±0.003[1] 0.058[2] |
B–V = 0.624 U–B = 0.235 FP (Tholen) B (SMASS)[1] | |
Absolute magnitude (H) | 8.96[1] |
Roberta (minor planet designation: 335 Roberta) is a large main belt asteroid. It was discovered on 1 September 1892, by German astronomer Anton Staus at Heidelberg Observatory.[3] Roberta was the 12th asteroid that was discovered using photography, and the only asteroid discovery made by Staus.[4]
Photometric observations of this asteroid from multiple sites during 2007 gave a light curve with a period of 12.054 ± 0.003 hours and a brightness variation of 0.13 ± 0.02 in magnitude. This agrees with a result reported in 1992, but differs from period estimates of 8.03 hours and 4.349 reported in 1987 and 2001, respectively.[5]
Under the SMASS classification taxonomy, this asteroid is listed as a B-type; a group that combines both the Tholen B and F types. The spectrum of this object suggests the presence of magnetite (Fe3O4), which gives it the spectrally-blue coloration that is a characteristic of this SMASS class. The spectrum of this asteroid also displays a band feature near 2.9 μm that indicate the presence of a hydrated mineral. This suggests that the asteroid has undergone significant water-based alteration.[2]
335 Roberta was identified as one of three asteroids that were likely to be a parent body for chondrites along with 449 Hamburga and 304 Olga.[6] All three asteroids were known to have low-albedo (not reflect as much light) and be close to "meteorite producing resonances".[6] Chrondrites are the most common type of meteor found on Earth, accounting for over 80% of all meteors.[7] They are named for the tiny spherical silicate particles that are found inside them (those particles are called chondrules).[7]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 "335 Roberta", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=335, retrieved 11 May 2016
- ↑ 2.0 2.1 Yang, Bin; Jewitt, David (September 2010), "Identification of Magnetite in B-type Asteroids", The Astronomical Journal 140 (3): 692–698, doi:10.1088/0004-6256/140/3/692, Bibcode: 2010AJ....140..692Y
- ↑ "Numbered Minor Planets 1–5000", Discovery Circumstances (IAU Minor Planet center), https://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html, retrieved 7 April 2013.
- ↑ Kutter, A. (December 1957). "Nachruf auf Anton Staus (Obituary)" (in de). Mitteilungen der Astronomischen Gesellschaft 9: 5. Bibcode: 1958MitAG...9....5K. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1958MitAG...9....5K. Retrieved 6 July 2016.
- ↑ Warner, Brian D. et al. (December 2007), "Lightcurve Analysis of 335 Roberta", The Minor Planet Bulletin 34 (4): p. 99, Bibcode: 2007MPBu...34...99W.
- ↑ 6.0 6.1 Lunar and planetary science: abstracts of papers submitted to the ... Lunar and Planetary Science Conference, Volume 27, Part 1 - Lunar and Planetary Institute, Jan 1, 1996
- ↑ 7.0 7.1 "ASU - Chondrites". https://meteorites.asu.edu/meteorites/meteorite-types/stony-meteorites/chondrites.
External links
- Lightcurve plot of 335 Roberta, Palmer Divide Observatory, B. D. Warner (2007)
- 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
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 335 Roberta at AstDyS-2, Asteroids—Dynamic Site
- 335 Roberta at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/335 Roberta.
Read more |