Frigga (minor planet designation: 77 Frigga) is a large, M-type, possibly metallic main-belt asteroid. It was discovered by the German-American astronomer C. H. F. Peters on November 12, 1862. The object is named after Frigg, the Norse goddess. The asteroid is orbiting the Sun with a period of 4.36years and completes a rotation on its axis every nine hours.
Frigga has been studied by radar.[5] The spectra of this asteroid displays a feature at a wavelength of 3μm, indicating the presence of hydrated minerals on the surface.[6] The near infrared spectrum is reddish and shows no spectral absorption features. Potential analogs of this spectrum include enstatite chondrites and nickel-iron meteorites.[7]
A three-chord occultation plot of the asteroid 77 Frigga, observed 2018 April 11th from eastern Australia.
Since 1999 there have been four stellar occultations by the asteroid. The first three were single chord observations, and the fourth was a 3-chord observation, and a miss. The best fit ellipse measures 60.0x74.0 kilometres at PA -14degrees.[8]
References
Upton, Clive; Kretzschmar, William A., Jr. (2017). The Routledge Dictionary of Pronunciation for Current English (2nded.). Routledge. p.519. ISBN978-1-138-12566-7.
Takir, D.; etal. (March 2008), "The Near-Infrared Spectroscopy of Two M-Class Main Belt Asteroids, 77 Frigga and 325 Heidelberga", 39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas. LPI Contribution No. 1391., p.1084, Bibcode:2008LPI....39.1084T
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