Samiksha Jaiswal (Editor)

444 Gyptis

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Discovered by
  
J. Coggia

Alternative names
  
1899 EL

Observation arc
  
116.54 yr (42568 d)

Orbits
  
Sun

Discoverer
  
Jérôme Eugène Coggia

Discovery site
  
Marseille Observatory

Discovery date
  
31 March 1899

Minor planet category
  
Main belt

Discovered
  
31 March 1899

Spectral type
  
C-type asteroid

Named after
  
Gyptis

Aphelion
  
3.25674 AU (487.201 Gm)

Similar
  
165 Loreley, 56 Melete, 51 Nemausa, 354 Eleonora, 423 Diotima

444 Gyptis is a main-belt asteroid that was discovered by J. Coggia on March 31, 1899, in Marseilles. It is classified as a C-type asteroid and is probably composed of carbonaceous material.

In 2004, Kochetova estimated Gyptis to have a mass of 1.25×1019 kg with a high density of 5.53 g/cm³. The adaptive optics instrument at the W. M. Keck Observatory showed an object with a diameter of 129 km, which is much smaller than the estimate of 160 km from the IRAS observatory measurements, indicating an irregular shape. The size ratio between the major and minor axes is estimated at 1.40. Observations of an occultation on October 14, 2007, produced six chords indicating a cross-section ellipsoid of 179×150 km.

References

444 Gyptis Wikipedia


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