762 Pulcova: Difference between revisions
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{{Short description|Main-belt asteroid}} |
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{{Infobox planet |
{{Infobox planet |
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| name = 762 Pulcova |
| name = 762 Pulcova |
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| image = 762Pulcova-SwRI.gif |
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| caption = 762 Pulcova and satellite as seen with [[adaptive optics]] in 2000<ref name=CFHT2000/> |
| caption = 762 Pulcova and satellite as seen with [[adaptive optics]] in 2000<ref name=CFHT2000/> |
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| discovery_ref = <ref name=jpldata/> |
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== Satellite == |
== Satellite == |
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[[File:762 Pulcova Hubble.jpg|thumb|left|Pulcova and its satellite imaged by the [[Hubble Space Telescope]] in January 2005]] |
[[File:762 Pulcova Hubble.jpg|thumb|left|Pulcova and its satellite imaged by the [[Hubble Space Telescope]] in January 2005]] |
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[[File:762 Pulkova orbit.png|thumb|left|Diagram of 762 Pulcova's orbit]] |
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On February 22, 2000,<ref name=CFHT2000>{{cite web |
On February 22, 2000,<ref name=CFHT2000>{{cite web |
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|date=2000-02-22 |
|date=2000-02-22 |
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|publisher=SwRI |
|publisher=SwRI |
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|url=http://www.boulder.swri.edu/merline/press/fig3.html |
|url=http://www.boulder.swri.edu/merline/press/fig3.html |
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|access-date=2009-10-20}} ([[Adaptive optics|AO]] image)</ref> astronomers at the [[Canada-France-Hawaii Telescope]] on [[Mauna Kea]], Hawaii, discovered a |
|access-date=2009-10-20}} ([[Adaptive optics|AO]] image)</ref> astronomers at the [[Canada-France-Hawaii Telescope]] on [[Mauna Kea]], Hawaii, discovered a 15-km moon (roughly a tenth the size of the primary)<ref name=swri2000>{{cite web |
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|date=2000-10-26 |
|date=2000-10-26 |
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|title=Astronomers Image Double Asteroid |
|title=Astronomers Image Double Asteroid |
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* {{JPL small body}} |
* {{JPL small body}} |
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{{Minor planets navigator |761 Brendelia |number=762 |763 Cupido}} |
{{Minor planets navigator |761 Brendelia |number=762 |763 Cupido}} |
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{{Small Solar System bodies}} |
{{Small Solar System bodies}} |
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{{Authority control}} |
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{{DEFAULTSORT:000762}} |
{{DEFAULTSORT:000762}} |
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[[Category:Background asteroids|000762]] |
[[Category:Background asteroids|000762]] |
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[[Category:Discoveries by Grigory Neujmin|Pulcova]] |
[[Category:Discoveries by Grigory Neujmin|Pulcova]] |
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[[Category:Minor planets named for places|Pulcova]] |
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[[Category:Named minor planets|Pulcova]] |
[[Category:Named minor planets|Pulcova]] |
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[[Category:Binary asteroids|000762]] |
[[Category:Binary asteroids|000762]] |
Latest revision as of 13:56, 15 June 2024
Discovery[2] | |
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Discovered by | G. N. Neujmin |
Discovery date | 3 September 1913 |
Designations | |
(762) Pulcova | |
Pronunciation | /ˈpʊlkəvə/ |
Named after | Pulkovo Heights |
1913 SQ | |
Main belt | |
Adjectives | Pulcovian /pʊlˈkoʊviən/[3] |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 100.08 yr (36553 d) |
Aphelion | 3.4801 AU (520.62 Gm) (Q) |
Perihelion | 2.8291 AU (423.23 Gm) (q) |
3.1546 AU (471.92 Gm) (a) | |
Eccentricity | 0.10319 (e) |
5.60 yr (2046.5 d) | |
348.62° (M) | |
0° 10m 33.276s / day (n) | |
Inclination | 13.089° (i) |
305.76° (Ω) | |
189.54° (ω) | |
Known satellites | S/2000 (762) 1[1] |
Earth MOID | 1.84297 AU (275.704 Gm) |
Jupiter MOID | 1.60162 AU (239.599 Gm) |
TJupiter | 3.158 |
Physical characteristics | |
68.54±1.6 km | |
Mass | 1.40×1018 kg[4] |
Mean density | 0.90 g/cm3[4] |
5.839 h (0.2433 d) | |
5.839 hr[2] | |
0.0458±0.002[2] | |
11.93 to 14.79[5] | |
8.28[2] | |
762 Pulcova is a main-belt asteroid. It was discovered by Grigoriy N. Neujmin in 1913,[2] and is named after Pulkovo Observatory, near Saint Petersburg. Pulcova is 137 km in diameter,[2] and is a C-type asteroid, which means that it is dark in colouring with a carbonate composition.
Photometric observations of this asteroid from Leura, Australia during 2006 gave a light curve with a period of 5.8403 ± 0.0005 hours and a brightness variation of 0.20 ± 0.02 in magnitude. This result is in agreement with previous studies.[6]
Satellite
[edit]On February 22, 2000,[1] astronomers at the Canada-France-Hawaii Telescope on Mauna Kea, Hawaii, discovered a 15-km moon (roughly a tenth the size of the primary)[7] orbiting Pulcova at a distance of 800 km.[8] Its orbital period is 4 days.[9] The satellite is about 4 magnitudes fainter than the primary.[8] It was one of the first asteroid moons to be identified.
Density
[edit]In the year 2000, Merline estimated Pulcova to have a density of 1.8 g/cm3, which would make it more dense than the trinary asteroid 45 Eugenia, and binary 90 Antiope.[8] But estimates by Marchis in 2008 suggest a density of only 0.90 g/cm3,[4] suggesting it may be a loosely packed rubble pile, not a monolithic object.
References
[edit]- ^ a b c "762 Pulcova". SwRI. 22 February 2000. Retrieved 20 October 2009. (AO image)
- ^ a b c d e f g "JPL Small-Body Database Browser: 762 Pulcova (1913 SQ)" (2009-09-22 last obs). Retrieved 5 May 2016.
- ^ Catalogue of the Mathematical, Historical, Bibliographical and Miscellaneous Portion of the Celebrated Library of M. Guglielmo Libri, 1861, p. 216
- ^ a b c Jim Baer (2008). "Recent Asteroid Mass Determinations". Personal Website. Archived from the original on 2 July 2013. Retrieved 28 November 2008.
- ^ Magnitudes generated with JPL Horizons for the year 1950 through 2100
- ^ Oey, Julian (December 2006), "Lightcurves analysis of 10 asteroids from Leura Observatory", The Minor Planet Bulletin, 33 (4): 96–99, Bibcode:2006MPBu...33...96O.
- ^ Dr. William J. Merline & Maria Martinez (26 October 2000). "Astronomers Image Double Asteroid". SwRI Press Release. Retrieved 20 October 2009. (mentions both 90 Antiope and 762 Pulcova)
- ^ a b c W.J. Merline (SwRI); L.M. Close (ESO, U. Arizona); C. Dumas (JPL); J.C. Shelton (Mt. Wilson Obs.); F. Menard (CFHT); C.R. Chapman; et al. (21 June 2000). "Discovery of Companions to Asteroids 762 Pulcova and 90 Antiope by Direct Imaging" (PDF). SwRI. Retrieved 21 October 2009.
- ^ Johnston, Robert (1 September 2005). "(762) Pulcova". Johnston's Archive. Retrieved 1 November 2013.
External links
[edit]- Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
- 762 Pulcova at AstDyS-2, Asteroids—Dynamic Site
- 762 Pulcova at the JPL Small-Body Database