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6312 Robheinlein

From Wikipedia, the free encyclopedia
Augusta or background asteroid from the inner regions of the asteroid belt

6312 Robheinlein
Orbital diagram ofRobheinlein
Discovery[1]
Discovered byH. E. Holt
Discovery sitePalomar Obs.
Discovery date14 September 1990
Designations
(6312) Robheinlein
Named after
Robert A. Heinlein[1]
(science fiction writer)
1990 RH4 · 1982 BW2
main-belt[1][2] · (inner)
background[3][4] · Augusta[5][6]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc36.26yr (13,244 d)
Aphelion2.3358AU
Perihelion2.0321 AU
2.1839 AU
Eccentricity0.0695
3.23 yr (1,179 d)
114.41°
0° 18m 19.44s / day
Inclination4.1155°
157.25°
283.14°
Physical characteristics
3.588±0.657 km[7]
0.314±0.109[7]
L(SDSS-MOC)[8]
14.1[1][2]

6312 Robheinlein (prov. designation:1990 RH4) is a brightAugusta orbackground asteroid from the inner regions of theasteroid belt, that measures approximately 3.5 kilometers (2.2 miles) in diameter. It was discovered on 14 September 1990, by American astronomerHenry Holt at thePalomar Observatory in California. The uncommonL-type asteroid was named for American science fiction writerRobert A. Heinlein.[1]

Orbit and classification

[edit]

When applying thehierarchical clustering method to the asteroid'sproper orbital elements,Robheinlein is considered to be a member of theAugusta family (as perZappalà)[6] as well as a non-family asteroid from the main belt'sbackground population (as perNesvorný).[3][4]

It orbits the Sun in theinner asteroid belt at a distance of 2.0–2.3 AU once every 3 years and 3 months (1,179 days;semi-major axis of 2.18 AU). Its orbit has aneccentricity of 0.07 and aninclination of 4° with respect to theecliptic.[2] The body'sobservation arc begins with its first observation as1982 BW2 at theKleť Observatory in January 1982, more than 8 years prior to its official discovery observation at Palomar.[1]

Naming

[edit]

Based on a suggestion by Belgian amateur astronomerJean Meeus, thisminor planet was named afterRobert Anson Heinlein (1907–1988), the Dean of Science Fiction, author of the mainstream literary classicStranger in a Strange Land, andscience fiction novelsStarship Troopers andThe Moon is a Harsh Mistress.[1] The official naming citation was published by theMinor Planet Center on 13 April 2006 (M.P.C. 56611).[9]

Heinlein helped narrateThe Moon Landing withWalter Cronkite on CBS in 1969, was involved in the planning of theStar Wars Defense program in the 1980s, contributed the wordsWaldo andGrok to the English language, and popularized the phrasesSpace Marine,TANSTAAFL, andPay it Forward.

Physical characteristics

[edit]

Robheinlein is anL-type asteroid in theSDSS-based taxonomy. It has anabsolute magnitude of 14.1.[1][2] As of 2018, no rotationallightcurve has been obtained fromphotometric observations. The body'srotation period,pole and shape remain unknown.[2]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Robheinlein measures 3.588 kilometers in diameter and its surface has a highalbedo of 0.314.[7]

References

[edit]
  1. ^abcdefgh"6312 Robheinlein (1990 RH4)".Minor Planet Center. Retrieved25 May 2018.
  2. ^abcdef"JPL Small-Body Database Browser: 6312 Robheinlein (1990 RH4)" (2018-04-26 last obs.).Jet Propulsion Laboratory. Retrieved25 May 2018.
  3. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Archived fromthe original on 2 August 2017. Retrieved6 December 2017.
  4. ^ab"Asteroid 6312 Robheinlein – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^"Asteroid 6312 Robheinlein".Small Bodies Data Ferret. Retrieved25 May 2018.
  6. ^abZappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997)."Asteroid Dynamical Families".NASA Planetary Data System: EAR-A-5-DDR-FAMILY-V4.1. Retrieved4 March 2020. (PDS main page)
  7. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.
  8. ^Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved25 May 2018.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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