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1988 Delores

From Wikipedia, the free encyclopedia
Main-belt asteroid

1988 Delores
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date28 September 1952
Designations
(1988) Delores
Named after
Delores Owings
(Indiana University)[2]
1952 SV · 1951 GF1
1952 UU · 1971 UE
1973 GH
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc64.59 yr (23,591 days)
Aphelion2.3749AU
Perihelion1.9336 AU
2.1543 AU
Eccentricity0.1024
3.16yr (1,155 days)
226.97°
0° 18m 42.12s / day
Inclination4.2519°
106.38°
235.01°
Physical characteristics
Dimensions4.60 km(calculated)[3]
5.761±0.035 km[1][4]
5.818±0.097 km[5]
88.1521±0.3555h[6]
0.1895±0.0252[5]
0.193±0.024[1][4]
0.24(assumed)[3]
S[3]
13.401±0.002(R)[6] · 13.6[1][5] · 13.85[3]

1988 Delores, provisional designation1952 SV, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 5 kilometers in diameter.

It was discovered on 28 September 1952, byIU'sIndiana Asteroid Program at theGoethe Link Observatory near Brooklyn, Indiana, United States, and named after Delores Owings, a member of the program.[7]

Classification and orbit

[edit]

Delores is a stonyS-type asteroid and member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 1.9–2.4 AU once every 3 years and 2 months (1,155 days).

Its orbit has aneccentricity of 0.10 and aninclination of 4° with respect to theecliptic.[1] It was first observed as1951 GF1 at theMcDonald Observatory in April 1951, yet the astrometric data from this observation remained unused to extend the body'sobservation arc prior to its official discovery.[7]

Physical characteristics

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Rotation period

[edit]

A rotationallightcurve ofDelores was obtained at thePalomar Transient Factory in October 2012. It gave arotation period of 88 hours and a brightness variation of 0.74magnitude (U=2).[6]

While not being aslow rotator, a period of 88 hours is significantly above average, as most minor planets rotate once every 2–20 hours around their axis. It has also a high brightness amplitude, which typically indicates that the body has a non-spheroidal shape.

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Delores measures 5.8 kilometers in diameter and its surface has analbedo of 0.19,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 — derived from8 Flora, the family's largest member and namesake – and calculates a diameter of 4.6 kilometers with anabsolute magnitude of 13.85.[3]

Naming

[edit]

Thisminor planet was named after Delores Owings, member in the Indiana Asteroid Program of Indiana University, collaborator withTom Gehrels on the determination of absolute magnitudes of minor planets, who became the program's supervisor ofastrometric measurements onphotographic plates. The naming was suggested byPaul Herget, the then director of theMinor Planet Center (MPC).[2] The officialnaming citation was published by theMinor Planet Center on 30 June 1977 (M.P.C. 4190).[8]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1988 Delores (1952 SV)" (2017-05-01 last obs.).Jet Propulsion Laboratory. Retrieved10 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1988) Delores".Dictionary of Minor Planet Names – (1988) Delores.Springer Berlin Heidelberg. p. 161.doi:10.1007/978-3-540-29925-7_1989.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1988) Delores". Asteroid Lightcurve Database (LCDB). Retrieved26 October 2016.
  4. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved14 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.
  6. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved26 October 2016.
  7. ^ab"1988 Delores (1952 SV)".Minor Planet Center. Retrieved26 October 2016.
  8. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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Distant minor planet
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