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461 Saskia

From Wikipedia, the free encyclopedia
Main-belt asteroid

461 Saskia
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date22 October 1900
Designations
(461) Saskia
PronunciationGerman:[ˈzaski.aː][2]
Named after
Saskia van Uylenburgh[3]
(wife of Rembrandt)
1900 FP · 1935 CT
A917 XE · A924 DB
main-belt[1][4] · (outer)
Themis[5][6]
Orbital characteristics[4]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc117.58yr (42,946 d)
Aphelion3.5621AU
Perihelion2.6834 AU
3.1227 AU
Eccentricity0.1407
5.52 yr (2,016 d)
71.934°
0° 10m 42.96s / day
Inclination1.4634°
157.03°
305.17°
Physical characteristics
39.81±13.20 km[7]
43.10±1.05 km[8]
43.603±0.256 km[9][10]
44.1±4.4 km[11]
7.348 h[12][13]
0.06[7][11]
0.069[8]
0.112[9]
Tholen =FCX[4][14]
X(S3OS2)[5][15]
B–V =0.610±028[4]
U–B =0.310±014[4]
10.48[1][4][8][9][11][16]
10.63[7]

461 Saskia, provisional designation1900 FP, is aThemistian asteroid from the outer regions of theasteroid belt, approximately 44 kilometers (27 miles) in diameter. It was discovered on 22 October 1900, by German astronomerMax Wolf at theHeidelberg Observatory in southwest Germany.[1] TheX-type asteroid has arotation period of 7.3 hours.[14] It was named after Rembrandt's wife,Saskia van Uylenburgh.[3]

Orbit and classification

[edit]

Saskia is a core member of the carbonaceousThemis family (602),[5][6] one of the largestasteroid families named after24 Themis.[17] It orbits the Sun in theouter asteroid belt at a distance of 2.7–3.6 AU once every 5 years and 6 months (2,016 days;semi-major axis of 3.12 AU). Its orbit has aneccentricity of 0.14 and aninclination of 1° with respect to theecliptic.[4] The body'sobservation arc begins at Heidelberg the night after its official discovery observation.[1]

Naming

[edit]

Thisminor planet was named afterSaskia van Uylenburgh (1612–1642), wife of renowned Dutch painterRembrandt(4511 Rembrandt). The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 50).[3]

Physical characteristics

[edit]

In theTholen classification, this asteroid'sspectral type is ambiguous, closest to a darkF-type asteroid, and somewhat similar to that of aC- andX-type (FCX),[4] while in both the Tholen- and SMASS-like taxonomy of theSmall Solar System Objects Spectroscopic Survey (S3OS2),Saskia is anX-type asteroid.[5][15] It has also been characterized as a primitiveP-type asteroid by theWide-field Infrared Survey Explorer (WISE).[14][16]

Rotation period

[edit]

In April 2007, a rotationallightcurve ofSaskia was obtained fromphotometric observations by French amateur astronomerPierre Antonini. Lightcurve analysis gave a well-definedrotation period of7.348±0.001 hours with a brightness variation of 0.36magnitude (U=3).[12][14] In December 2016, an identical period with an amplitude of 0.28 magnitude was determined by Daniel Klinglesmith at Etscorn Campus Observatory (719), New Mexico (U=3-).[13] This result supersedes two previous observations that gave a period of 7.34 and 7.349 hours, respectively (U=2/3-).[18][19]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA's WISE telescope,Saskia measures between 39.8 and 44.1 kilometers in diameter and its surface has analbedo between 0.06 and 0.112,[7][9][10][11] while the JapaneseAkari satellite determined a diameter of 43.10 kilometers with an albedo of 0.069.[8] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.10 and derives a smaller diameter of 33.69 kilometers based on anabsolute magnitude of 10.48.[14]

References

[edit]
  1. ^abcde"461 Saskia (1900 FP)".Minor Planet Center. Retrieved17 July 2018.
  2. ^(German Names)
  3. ^abcSchmadel, Lutz D. (2007). "(461) Saskia".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 52.doi:10.1007/978-3-540-29925-7_462.ISBN 978-3-540-00238-3.
  4. ^abcdefgh"JPL Small-Body Database Browser: 461 Saskia (1900 FP)" (2018-05-22 last obs.).Jet Propulsion Laboratory. Retrieved17 July 2018.
  5. ^abcd"Asteroid 461 Saskia".Small Bodies Data Ferret. Retrieved17 July 2018.
  6. ^ab"Asteroid (461) Saskia". AstDyS-2, Asteroids – Dynamic Site. Retrieved25 May 2018.
  7. ^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.
  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. Retrieved17 July 2018. (online,AcuA catalog p. 153)
  9. ^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. Retrieved17 July 2018.
  10. ^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.S2CID 119293330.
  11. ^abcdAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids"(PDF).Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.
  12. ^abBehrend, Raoul."Asteroids and comets rotation curves – (461) Saskia". Geneva Observatory. Retrieved17 July 2018.
  13. ^abKlinglesmith, Daniel A., III (April 2017). "Spin-Shape Model Lightcurves".The Minor Planet Bulletin.44 (2):127–129.Bibcode:2017MPBu...44..127K.ISSN 1052-8091.{{cite journal}}: CS1 maint: numeric names: authors list (link)
  14. ^abcde"LCDB Data for (461) Saskia". Asteroid Lightcurve Database (LCDB). Retrieved17 July 2018.
  15. ^abLazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004)."S3OS2: the visible spectroscopic survey of 820 asteroids"(PDF).Icarus.172 (1):179–220.Bibcode:2004Icar..172..179L.doi:10.1016/j.icarus.2004.06.006. Retrieved17 July 2018.
  16. ^abMainzer, 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. (catalog)
  17. ^Nesvorný, 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 978-0-8165-3213-1.S2CID 119280014.
  18. ^Buchheim, Robert K. (September 2006). "Lightcurves of asteroids 125 Liberatrix, 461 Saskia, and 2781 Kleczek".The Minor Planet Bulletin.33 (3): 63.Bibcode:2006MPBu...33...63B.ISSN 1052-8091.
  19. ^Klinglesmith, Daniel A. III; Hanowell, Jesse; Risley, Ethan; Turk, Janek; Vargas, Angelica; Warren, Curtis Alan (October 2013). "Inversion Model Candidates".The Minor Planet Bulletin.40 (4):190–193.Bibcode:2013MPBu...40..190K.ISSN 1052-8091.

External links

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