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627 Charis

From Wikipedia, the free encyclopedia
Main-belt asteroid

627 Charis
Discovery[1]
Discovered byA. Kopff
Discovery siteHeidelberg Obs.
Discovery date4 March 1907
Designations
(627) Charis
Pronunciation/ˈkrɪs/
Named after
Charis(Greek mythology)[2]
1907 XS · 1929 RJ1
1929 RN1 · 1932 CZ
1947 GK · 1966 DR
A917 DE
main-belt · (outer)[3]
Charis[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc110.65 yr (40,415 days)
Aphelion3.0675AU
Perihelion2.7320 AU
2.8998 AU
Eccentricity0.0578
4.94yr (1,804 days)
318.92°
0° 11m 58.56s / day
Inclination6.4732°
142.48°
176.72°
Physical characteristics
Dimensions38.018±0.146 km[5]
44.745±0.140 km[6]
48.51±2.6 km[3][7]
49.47±0.51 km[8]
62.68±0.41 km[9]
>24h(dated)[10]
27.888±0.002 h[11]
0.047±0.007[9]
0.0786±0.009[3][7]
0.080±0.002[8]
0.0925±0.0225[6]
Tholen =XB:[1]
SMASS =X[1][3] · P[6]
B–V = 0.680[1]
U–B = 0.261[1]
9.44±0.85[12] · 9.95[1][3][6][7][8][9]

627 Charis/ˈkrɪs/ is anasteroid and the parent body of theCharis family, located in the outer regions of theasteroid belt, approximately 49 kilometers in diameter. It was discovered on 4 March 1907, by German astronomerAugust Kopff at theHeidelberg-Königstuhl State Observatory in southwest Germany.[13] The asteroid was named after the Greek goddessCharis,[2] a name which may have been inspired by the asteroid's provisional designation1907 XS. ('Charis' is in Greek is spelled 'Χάρις'.)

Orbit and classification

[edit]

Charis is theparent body of theCharis family (616),[4] anasteroid family of more than 800 known members.[14]: 23  It orbits the Sun in theouter main-belt at a distance of 2.7–3.1 AU once every 4 years and 11 months (1,804 days;semi-major axis of 2.90 AU). Its orbit has aneccentricity of 0.06 and aninclination of 6° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Heidelberg in March 1907.[13]

Physical characteristics

[edit]

The overallspectral type for members of the Charis family is that of aC- andX-type.[14]: 23  In theSMASS classificationCharis is an X-type asteroid,[1][3] while in theTholen classification, its type is ambiguous, closest to an X- and somewhat similar to a carbonaceousB-type asteroid including a reported noisy spectrum (XB:).[1] Conversely, theWide-field Infrared Survey Explorer (WISE) characterized it as a primitiveP-type asteroid.[6]

Rotation period

[edit]

Photometric observations of this asteroid by American astronomerFrederick Pilcher at the Organ Mesa Observatory (G50) in Las Cruces, New Mexico, during May 2012 gave a well-definedlightcurve with arotation period of 27.888 hours and a brightness variation of 0.35 inmagnitude (U=3).[11] The result supersedes a tentative period of at least 24 hours obtained by French amateur astronomerPierre Antonini in March 2011 (U=2-).[10]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Charis measures between 38.018 and 62.68 kilometers in diameter and its surface has analbedo between 0.047 and 0.0925.[5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0786 and a diameter of 48.51 kilometers based on anabsolute magnitude of 9.95.[3][7]

Naming

[edit]

Thisminor planet was named fromGreek mythology, after the goddessCharis, the wife ofHephaestus after whom the minor planet2212 Hephaistos was also named. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 65).[2]

References

[edit]
  1. ^abcdefghij"JPL Small-Body Database Browser: 627 Charis (1907 XS)" (2017-10-27 last obs.).Jet Propulsion Laboratory. Retrieved20 December 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(627) Charis".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 63.doi:10.1007/978-3-540-29925-7_628.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (627) Charis". Asteroid Lightcurve Database (LCDB). Retrieved20 December 2017.
  4. ^ab"Asteroid 627 Charis – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved24 October 2019.
  5. ^abMasiero, 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.
  6. ^abcdefMainzer, 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. ^abcdeTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  8. ^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.
  9. ^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. Retrieved20 December 2017.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (627) Charis". Geneva Observatory. Retrieved20 December 2017.
  11. ^abPilcher, Frederick (October 2012)."Rotation Period Determinations for 47 Aglaja, 252 Clementina 611 Valeria, 627 Charis, and 756 Lilliana".The Minor Planet Bulletin.39 (4):220–222.Bibcode:2012MPBu...39..220P.ISSN 1052-8091. Retrieved20 December 2017.
  12. ^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. Retrieved20 December 2017.
  13. ^ab"627 Charis (1907 XS)".Minor Planet Center. Retrieved20 December 2017.
  14. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.

External links

[edit]
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