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2368 Beltrovata

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2368 Beltrovata
Discovery [1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date4 September 1977
Designations
(2368) Beltrovata
Named after
Betty Tendering
(friend ofGottfried Keller)[2]
1977 RA
NEO · Amor[1][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc38.65 yr (14,117 days)
Aphelion2.9751AU
Perihelion1.2356 AU
2.1054 AU
Eccentricity0.4131
3.05yr (1,116 days)
39.633°
0° 19m 21.36s / day
Inclination5.2222°
287.34°
43.081°
Earth MOID0.2334 AU · 90.9LD
Physical characteristics
Dimensions2.3 km[1]
2.70 km(calculated)[4]
3.003±0.493 km[5]
5.9 h[6][7]
0.161±0.081[5]
0.20(assumed)[4]
0.27[1]
Tholen = SQ [1] · S[4]
B–V = 0.830[1]
U–B = 0.520[1]
15.21[1][4][5] · 15.33±0.40[8]

2368 Beltrovata, provisional designation1977 RA, is an eccentric stonyasteroid andnear-Earth object of theAmor group, approximately 2.7 kilometers in diameter. It was discovered on 4 September 1977, by Swiss astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland.[3] The asteroid was named for Betty Tendering, a friend of authorGottfried Keller.[2]

Orbit and classification

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Beltrovata orbits the Sun in theinner main-belt at a distance of 1.2–3.0 AU once every 3 years and 1 month (1,116 days). Its orbit has aneccentricity of 0.41 and aninclination of 5° with respect to theecliptic.[1]

As anAmor asteroid, it approaches the orbit of Earth from the outside but does not cross it. It has an Earthminimum orbit intersection distance of 0.2334 AU (34,900,000 km), which corresponds to 90.9lunar distances.[1] The asteroid'sobservation arc begins with its official discovering observation at Zimmerwald.[3]

Physical characteristics

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In theTholen classificationBeltrovata is a SQ-type asteroid, an intermediate between the commonS-type andQ-type asteroids.[1]

Rotation period

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A first rotationallightcurve ofBeltrovata was obtained from photoelectric observations made by U.S. astronomersEdward Bowell andSchelte Bus in the 1970s (IAUC 3111), and gave arotation period of5.9 hours with a brightness variation of 0.84magnitude (U=n.a.).[7] In 2000, theNear-Earth Objects Follow-up Program published an identical period but with a higher amplitude of 1.05 magnitude.(U=2).[6]

Diameter and albedo

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According to the space-based survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures 3.0 kilometers in diameter and its surface has analbedo of 0.16,[5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 2.7 kilometers with anabsolute magnitude of 15.21.[4]

Naming

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Thisminor planet is named "Beltrovata", which is the name by whom the Swiss authorGottfried Keller from Zürich called his friend Betty Tendering. She served as role model for the character of "Dortchen Schönfund" in Keller's novelGreen Henry.[2] The official naming citation was published by theMinor Planet Center on 1 August 1981 (M.P.C. 6209).[9]

References

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  1. ^abcdefghijkl"JPL Small-Body Database Browser: 2368 Beltrovata (1977 RA)" (2016-04-29 last obs.).Jet Propulsion Laboratory. Retrieved13 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2368) Beltrovata".Dictionary of Minor Planet Names – (2368) Beltrovata.Springer Berlin Heidelberg. p. 193.doi:10.1007/978-3-540-29925-7_2369.ISBN 978-3-540-00238-3.
  3. ^abc"2368 Beltrovata (1977 RA)".Minor Planet Center. Retrieved1 September 2016.
  4. ^abcde"LCDB Data for (2368) Beltrovata". Asteroid Lightcurve Database (LCDB). Retrieved1 September 2016.
  5. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.S2CID 35447010.
  6. ^abErikson, A.; Mottola, S.; Lagerros, J. S. V.; Lindgren, M.; Piironen, J.; Oja, T.; et al. (October 2000)."The Near-Earth Objects Follow-up Program. III. 32 Lightcurves for 12 Objects from 1992 and 1995".Icarus.147 (2):487–497.Bibcode:2000Icar..147..487E.doi:10.1006/icar.2000.6457. Retrieved1 September 2016.
  7. ^abBus, S. J.; Lauer, T.; Gibson, J.; Giclas, H. L.; Kantz, M. L.; Bowell, E.; et al. (September 1977)."1977 RA".IAU Circ.3111 (3111): 2.Bibcode:1977IAUC.3111....2B. Retrieved1 September 2016.
  8. ^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.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved1 September 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 September 2016.

External links

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