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762 Pulcova

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Discovered by
  
G. N. Neujmin

Alternative names
  
1913 SQ

Observation arc
  
100.08 yr (36553 d)

Orbits
  
Sun

Discoverer
  
Grigory Neujmin

Moon
  
S/2000 (762) 1

Discovery date
  
3 September 1913

Minor planet category
  
Main belt

Discovered
  
3 September 1913

Spectral type
  
Discovery site
  
Simeiz Observatory

762 Pulcova httpsuploadwikimediaorgwikipediaeneea762

Aphelion
  
3.4801 AU (520.62 Gm) (Q)

Similar
  
45 Eugenia, 90 Antiope, 87 Sylvia, 107 Camilla, 121 Hermione

762 Pulcova is a main-belt asteroid. It was discovered by Grigoriy N. Neujmin in 1913, and is named after Pulkovo Observatory, near Saint Petersburg. Pulcova is 137 km in diameter, and is a C-type asteroid, which means that it is dark in colouring with a carbonate composition.

Contents

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.

Satellite

On February 22, 2000, astronomers at the Canada-France-Hawaii Telescope on Mauna Kea, Hawaii, discovered a small, 15-km moon (roughly a 10th the size of the primary) orbiting Pulcova at a distance of 800 km. Its orbital period is 4 days. The satellite is about 4 magnitudes fainter than the primary. It was one of the first asteroid moons to be identified.

Density

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. But estimates by Marchis in 2008 suggest a density of only 0.90 g/cm³, suggesting it may be a loosely packed rubble pile, not a monolithic object.

References

762 Pulcova Wikipedia


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