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1848 Delvaux

From Wikipedia, the free encyclopedia
Stony Koronis asteroid

1848 Delvaux
Shape model ofDelvaux from itslightcurve
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date18 August 1933
Designations
(1848) Delvaux
Named after
(sister-in-law of)
Georges Roland[2]
1933 QD · 1936 DH
1948 SF · 1948 SK
1951 GV · 1952 ML
1953 TU1 · 1953 VE1
1956 GL · 1972 QN
1975 FV · A912 FA
main-belt · Koronis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc83.47 yr (30,486 days)
Aphelion3.0019AU
Perihelion2.7407 AU
2.8713 AU
Eccentricity0.0455
4.87yr (1,777 days)
138.35°
0° 12m 9.36s / day
Inclination1.4404°
331.66°
316.61°
Physical characteristics
Dimensions16.66±1.95 km[4]
17.030±0.114[5]
17.12 km(calculated)[3]
17.446±0.143 km[6]
17.51±0.63 km[7]
3.637h(adopted)[3]
3.638±0.001 h[8]
3.639±0.001 h[9]
3.639±0.001 h[10]
3.65±0.01 h[8]
0.2329±0.0432[6]
0.24(assumed)[3]
0.242±0.036[5]
0.255±0.020[7]
0.461±0.316[4]
SMASS =S[1] · S[3]
10.35[4] · 10.90[7] · 11.0[1][3][6] · 11.24±0.10[10] · 11.26±0.40[11]

1848 Delvaux (prov. designation:1933 QD) is a stonyKoronis asteroid from the outer region of theasteroid belt, approximately 17 kilometers in diameter. It was discovered on 18 August 1933, by Belgian astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle, Belgium.[12] It was later named after astronomerGeorges Roland's sister-in-law.[2]

Orbit and classification

[edit]

Delvaux is a stony asteroid and a member of theKoronis family, a collisional group consisting of a few hundred known bodies with nearlyecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.7–3.0 AU once every 4 years and 10 months (1,777 days). Its orbit has aneccentricity of 0.05 and aninclination of 1° with respect to the ecliptic.[1] First identified asA912 FA atSimeiz Observatory in 1912, the body's observation arc begins 3 day after its official discovery, as non of the previous observations were used.[12]

Physical characteristics

[edit]

In theSMASS taxonomyDelvaux is a commonS-type asteroid.[2]

Rotation period

[edit]

It has a well-determinedrotation period of 3.63 to 3.65 hours with a brightness variation of 0.57–0.69magnitude (U=3/3/3/3).[8][9][10] TheCollaborative Asteroid Lightcurve Link (CALL) adopts a period of 3.637 hours.[3]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Delvaux measures between 16.66 and 17.51 kilometers in diameter, and its surface has analbedo of 0.233 to 0.461.[4][5][6][7] CALL assumes a standard albedo for members of the Koronis family of 0.24, and calculates a diameter of 17.12 kilometers with anabsolute magnitude of 11.0.[3]

Name

[edit]

Thisminor planet was named after the sister-in-law of Georges Roland, astronomer at the observatory in Uccle and known as the co-discoverer of thecomet Arend–Roland.[2] The approved naming citation was published by theMinor Planet Center on 8 April 1982 (M.P.C. 6832).[13]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1848 Delvaux (1933 QD)" (2017-02-04 last obs.).Jet Propulsion Laboratory. Retrieved1 July 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1848) Delvaux".Dictionary of Minor Planet Names – (1848) Delvaux.Springer Berlin Heidelberg. p. 148.doi:10.1007/978-3-540-29925-7_1849.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1848) Delvaux". Asteroid Lightcurve Database (LCDB). Retrieved14 December 2016.
  4. ^abcdMasiero, 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. Retrieved14 December 2016.
  5. ^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 December 2016.
  6. ^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.
  7. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  8. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1848) Delvaux".Geneva Observatory. Retrieved14 December 2016.
  9. ^abArredondo, Anicia; Hartt, Anne-Marie; Yazdi, Sormeh K. (October 2014)."Rotation Periods and R Magnitudes of Three Koronis Family Members".The Minor Planet Bulletin.41 (4):252–254.Bibcode:2014MPBu...41..252A.ISSN 1052-8091. Retrieved14 December 2016.
  10. ^abcSlivan, Stephen M.; Binzel, Richard P.; Boroumand, Shaida C.; Pan, Margaret W.; Simpson, Christine M.; Tanabe, James T.; et al. (May 2008)."Rotation rates in the Koronis family, complete to H≈11.2".Icarus.195 (1):226–276.Bibcode:2008Icar..195..226S.doi:10.1016/j.icarus.2007.11.019. Retrieved14 December 2016.
  11. ^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. Retrieved14 December 2016.
  12. ^ab"1848 Delvaux (1933 QD)".Minor Planet Center. Retrieved14 December 2016.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved14 December 2016.

External links

[edit]
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