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1707 Chantal

From Wikipedia, the free encyclopedia
Stony background asteroid from the Florian region in the inner asteroid belt

1707 Chantal
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date8 September 1932
Designations
(1707) Chantal
Named after
Niece of astronomer Georges Roland[1]
1932 RL · 1942 TC
1950 BF1 · 1955 QA1
A906 YJ
main-belt[1][2] · (inner)
background[3][4]
Orbital characteristics[2]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc111.83yr (40,847 d)
Aphelion2.5989AU
Perihelion1.8390 AU
2.2189 AU
Eccentricity0.1712
3.31 yr (1,207 d)
37.923°
0° 17m 53.52s / day
Inclination4.0315°
6.1128°
42.974°
Physical characteristics
7.459±0.114 km[5][6]
7.578±0.291 km[7]
7.62±1.37 km[8]
10 h(at least)[9]
0.28[8]
0.2969[7]
0.306[6][5]
Tholen =S[2][10]
B–V = 0.870[2]
U–B = 0.530[2]
12.54[1][2][5][7][10]
12.79[8]

1707 Chantal, provisional designation1932 RL, is a stony backgroundasteroid from the Florian region in the innerasteroid belt, approximately 7.5 kilometers (4.7 miles) in diameter. It was discovered on 8 September 1932, by astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle.[1] TheS-type asteroid has arotation period of at least 10 hours.[10] It was named for Chantal, the niece of Belgian astronomer Georges Roland.[1]

Orbit and classification

[edit]

According to modernHCM-analyses byNesvorný, as well as byMilani andKnežević,Chantal is a non-family asteroid from the main belt'sbackground population.[3][4] In an older HCM-analysis (Zappalà (1990–97), it is a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[3] It orbits the Sun in theinner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,207 days;semi-major axis of 2.22 AU). Its orbit has aneccentricity of 0.17 and aninclination of 4° with respect to theecliptic.[2] The asteroid was first observed asA906 YJ at theHeidelberg Observatory in December 1906. The body'sobservation arc begins atUccle Observatory in October 1932, or seven weeks after its official discovery observation.[1]

Naming

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Thisminor planet was named by the discovererEugène Delporte after Chantal, a niece of Belgian astronomerGeorges Roland (1922–1991) of Uccle and co-discoverer of theComet Arend–Roland.[1] The official naming citation was published by theMinor Planet Center on 8 April 1982 (M.P.C. 6832).[11] Asteroid1711 Sandrine was also named by the discoverer after a (grand)-niece of Roland.

Physical characteristics

[edit]

In theTholen classification,Chantal is a common, stonyS-type asteroid.[2][3]

Rotation period

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In October 1975, a rotationallightcurve ofChantal was obtained fromphotometric observations by Swedish astronomerClaes-Ingvar Lagerkvist at theUppsala Astronomical Observatory. Analysis of the fragmentary lightcurve gave arotation period of at least10 hours with a brightness amplitude of more than 0.2magnitude (U=1).[9]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Chantal measures between 7.46 and 7.62 kilometers in diameter and its surface has analbedo between 0.28 and 0.31.[5][6][7][8] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 9.23 kilometers based on anabsolute magnitude of 12.54.[10]

References

[edit]
  1. ^abcdefgh"1707 Chantal (1932 RL)".Minor Planet Center. Retrieved10 December 2018.
  2. ^abcdefgh"JPL Small-Body Database Browser: 1707 Chantal (1932 RL)" (2018-10-22 last obs.).Jet Propulsion Laboratory. Retrieved10 December 2018.
  3. ^abcd"Asteroid 1707 Chantal".Small Bodies Data Ferret. Retrieved10 December 2018.
  4. ^ab"Asteroid (1707) Chantal – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved10 December 2018.
  5. ^abcdMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0".NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0.Bibcode:2016PDSS..247.....M. Retrieved10 December 2018.
  6. ^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.S2CID 119293330.
  7. ^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 118700974. (catalog)
  8. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.S2CID 119289027.
  9. ^abLagerkvist, C.-I. (March 1978). "Photographic photometry of 110 main-belt asteroids".Astronomy and Astrophysics Supplement Series.31:361–381.Bibcode:1978A&AS...31..361L.
  10. ^abcd"LCDB Data for (1707) Chantal". Asteroid Lightcurve Database (LCDB). Retrieved10 December 2018.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved10 December 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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