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335 Roberta

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]

335 Roberta
Orbital diagram
Discovery
Discovered byAnton Staus
Discovery date1 September 1892
Designations
(335) Roberta
Named after
Carl Robert Osten-Sacken
1892 C
Main belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.58 yr (45137 d)
Aphelion2.9014 AU (434.04 Gm)
Perihelion2.04926 AU (306.565 Gm)
2.47530 AU (370.300 Gm)
Eccentricity0.17212
3.89 yr (1422.5 d)
18.93 km/s
355.460°
0° 15m 11.095s / day
Inclination5.1005°
148.454°
140.006°
Earth MOID1.03587 AU (154.964 Gm)
Jupiter MOID2.2733 AU (340.08 Gm)
TJupiter3.456
Physical characteristics
Dimensions89.07±2.0 km[1]
12.054 h (0.5023 d)
0.0580±0.003[1]
0.058[2]
B–V = 0.624
U–B = 0.235
FP (Tholen)
B (SMASS)[1]
8.96[1]

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 edit

  1. ^ a b c d e "335 Roberta", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 11 May 2016
  2. ^ a b Yang, Bin; Jewitt, David (September 2010), "Identification of Magnetite in B-type Asteroids", The Astronomical Journal, 140 (3): 692–698, arXiv:1006.5110, Bibcode:2010AJ....140..692Y, doi:10.1088/0004-6256/140/3/692
  3. ^ "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
  4. ^ Kutter, A. (December 1957). "Nachruf auf Anton Staus (Obituary)". Mitteilungen der Astronomischen Gesellschaft (in German). 9: 5. Bibcode:1958MitAG...9....5K. Retrieved 6 July 2016.
  5. ^ Warner, Brian D.; et al. (December 2007), "Lightcurve Analysis of 335 Roberta", The Minor Planet Bulletin, vol. 34, no. 4, p. 99, Bibcode:2007MPBu...34...99W.
  6. ^ a b 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. ^ a b . Archived from the original on 22 June 2019. Retrieved 31 August 2015.

External links edit

  • Lightcurve plot of 335 Roberta, Palmer Divide Observatory, B. D. Warner (2007)
  • Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
  • 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
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 335 Roberta at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

roberta, roberta, minor, planet, designation, large, main, belt, asteroid, discovered, september, 1892, german, astronomer, anton, staus, heidelberg, observatory, roberta, 12th, asteroid, that, discovered, using, photography, only, asteroid, discovery, made, s. 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 4 335 RobertaOrbital diagramDiscoveryDiscovered byAnton StausDiscovery date1 September 1892DesignationsMPC designation 335 RobertaNamed afterCarl Robert Osten SackenAlternative designations1892 CMinor planet categoryMain beltOrbital characteristics 1 Epoch 31 July 2016 JD 2457600 5 Uncertainty parameter 0Observation arc123 58 yr 45137 d Aphelion2 9014 AU 434 04 Gm Perihelion2 04926 AU 306 565 Gm Semi major axis2 47530 AU 370 300 Gm Eccentricity0 17212Orbital period sidereal 3 89 yr 1422 5 d Average orbital speed18 93 km sMean anomaly355 460 Mean motion0 15m 11 095s dayInclination5 1005 Longitude of ascending node148 454 Argument of perihelion140 006 Earth MOID1 03587 AU 154 964 Gm Jupiter MOID2 2733 AU 340 08 Gm TJupiter3 456Physical characteristicsDimensions89 07 2 0 km 1 Synodic rotation period12 054 h 0 5023 d Geometric albedo0 0580 0 003 1 0 058 2 Spectral typeB V 0 624U B 0 235FP Tholen B SMASS 1 Absolute magnitude H 8 96 1 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 mm 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 edit a b c d e 335 Roberta JPL Small Body Database Browser NASA Jet Propulsion Laboratory retrieved 11 May 2016 a b Yang Bin Jewitt David September 2010 Identification of Magnetite in B type Asteroids The Astronomical Journal 140 3 692 698 arXiv 1006 5110 Bibcode 2010AJ 140 692Y doi 10 1088 0004 6256 140 3 692 Numbered Minor Planets 1 5000 Discovery Circumstances IAU Minor Planet center retrieved 7 April 2013 Kutter A December 1957 Nachruf auf Anton Staus Obituary Mitteilungen der Astronomischen Gesellschaft in German 9 5 Bibcode 1958MitAG 9 5K Retrieved 6 July 2016 Warner Brian D et al December 2007 Lightcurve Analysis of 335 Roberta The Minor Planet Bulletin vol 34 no 4 p 99 Bibcode 2007MPBu 34 99W a b 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 a b ASU Chondrites Archived from the original on 22 June 2019 Retrieved 31 August 2015 External links editLightcurve plot of 335 Roberta Palmer Divide Observatory B D Warner 2007 Asteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Observatoire de Geneve Raoul Behrend Discovery Circumstances Numbered Minor Planets 1 5000 Minor Planet Center 335 Roberta at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 335 Roberta at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 335 Roberta amp oldid 1191750759, wikipedia, wiki, book, books, library,

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