Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1724 Vladimir

From Wikipedia, the free encyclopedia
Asteroid

1724 Vladimir
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date28 February 1932
Designations
(1724) Vladimir
Named after
Vladimir
(grandson of astronomer)
Milorad Protić[2]
1932 DC · 1932 ED1
1934 TB · 1952 UV1
1961 VK · 1965 SE
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc85.17 yr (31,110 days)
Aphelion2.8670AU
Perihelion2.5580 AU
2.7125 AU
Eccentricity0.0570
4.47yr (1,632 days)
119.75°
0° 13m 14.16s / day
Inclination12.232°
164.03°
298.51°
Physical characteristics
Dimensions28.40±12.05 km[4]
28.45±9.13 km[5]
32.85±0.42 km[6]
34.79 km(IRAS:15)[7]
35.84±0.48 km[8]
36.3±3.6 km[9]
38.476±0.236[10]
40±4 km[11]
42.505±0.219 km[12]
12.557±0.0123h[13]
12.57±0.01 h[a]
12.574±0.0043 h[13]
12.582±0.002 h[14]
0.0295±0.0129[12]
0.03±0.01[11]
0.037±0.005[10]
0.04±0.01[9]
0.042±0.006[8]
0.0441(IRAS:15)[7]
0.05±0.16[4]
0.051±0.002[6]
0.06±0.04[5]
FBCU::(Tholen)[1]
B(SMASS)[1] · X[15] · B[3]
B–V = 0.693[1]
U–B = 0.259[1]
11.250±0.003(R)[13] · 11.3[1][3][5][6][8][9][11][12] · 11.41[4] · 11.48±0.26[15]

1724 Vladimir, provisional designation1932 DC, is a rare-typeasteroid from the central region of theasteroid belt, approximately 35 kilometers in diameter. It was discovered on 28 February 1932, by Belgian astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle, Belgium.[16] The asteroid was later named by astronomerMilorad Protić after his grandson, Vladimir.[2]

Orbit and classification

[edit]

Vladimir orbits the Sun in thecentral main-belt at a distance of 2.6–2.9 AU once every 4 years and 6 months (1,632 days). Its orbit has aneccentricity of 0.06 and aninclination of 12° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Uccle in 1928.[16]

Physical characteristics

[edit]

The asteroid has a rareB- and FBCUspectral type in theSMASS andTholen taxonomy, respectively.[1]

Lightcurves

[edit]

Two rotational lightcurve ofVladimir were obtained by Serbian astronomer Vladimir Benishek at theBelgrade Observatory in April 2008, and August 2015. Analysis of the bimodal lightcurve gave arotation period of 12.57 and 12.582hours with a relatively low brightness variation of 0.14 and 0.24magnitude, respectively (U=2/2+).[14][a]

In December 2010, and January 2012, photometric observations in the R-band at thePalomar Transient Factory in California gave a period of 12.574 and 12.557 hours with an amplitude of 0.23 and 0.22, respectively (U=2/2).[13]

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,Vladimir measures between 28.40 and 42.505 kilometers in diameter, and its surface has a lowalbedo between 0.0295 and 0.037.[4][5][6][9][10][11]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by the Infrared Astronomical SatelliteIRAS, that is, an albedo of 0.0441 and a diameter of 34.79 kilometers with anabsolute magnitude of 11.30.[3][7]

Naming

[edit]

Thisminor planet was named by Serbian astronomerMilorad Protić, who rediscovered the body in 1952, and made its permanent numbering possible (also seeLost minor planet). Protić named it after his grandson,Vladimir.[2] The official naming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C. 5281).[17]

Notes

[edit]
  1. ^abBenishek (2011) web: rotation period12.57±0.01 hours with a brightness amplitude of0.14. Summary figures atAsteroid Lightcurve Database for (1724) Vladimir

References

[edit]
  1. ^abcdefghi"JPL Small-Body Database Browser: 1724 Vladimir (1932 DC)" (2017-05-02 last obs.).Jet Propulsion Laboratory. Retrieved7 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1724) Vladimir".Dictionary of Minor Planet Names – (1724) Vladimir.Springer Berlin Heidelberg. p. 137.doi:10.1007/978-3-540-29925-7_1725.ISBN 978-3-540-00238-3.
  3. ^abcd"LCDB Data for (1724) Vladimir". Asteroid Lightcurve Database (LCDB). Retrieved21 December 2016.
  4. ^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.
  5. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved7 June 2017.
  6. ^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)
  7. ^abcTedesco, 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. ^abcMasiero, 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.S2CID 46350317. Retrieved21 December 2016.
  9. ^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".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614.
  10. ^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. Retrieved21 December 2016.
  11. ^abcdAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680.S2CID 119214002. Retrieved21 December 2016.
  12. ^abcMainzer, 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.
  13. ^abcdWaszczak, 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.S2CID 8342929. Retrieved21 December 2016.
  14. ^abBenishek, Vladimir (April 2015)."Rotation Period Determinations for 1724 Vladimir, 3965 Konopleva, and 9222 Chubey".The Minor Planet Bulletin.42 (2):143–144.Bibcode:2015MPBu...42..143B.ISSN 1052-8091. Retrieved7 June 2017.
  15. ^abVeres, 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.S2CID 53493339. Retrieved21 December 2016.
  16. ^ab"1724 Vladimir (1932 DC)".Minor Planet Center. Retrieved21 December 2016.
  17. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved21 December 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=1724_Vladimir&oldid=1195822644"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp