Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989em%26p...44..175f&link_type=abstract
Earth, Moon, and Planets (ISSN 0167-9295), vol. 44, Feb. 1989, p. 175-179. Research supported by CNR and MPI.
Astronomy and Astrophysics
Astrophysics
1
Nereid, Solar System, Astronomical Photometry, Gravitational Effects, Luminosity, Orbit Perturbation, Tides
Scientific paper
If real, Nereid's recently observed large photometric variations can be explained by modeling this Neptunian satellite as a quasi-contact binary system made of two similar, ellipsoidal components distorted by their mutual tides. Both the amplitude and the likely periodicity of the observed luminosity changes are consistent with the binary model, provided Nereid's density is close to 1 g/cu cm. The assumed binary would be probably stable against Neptune's gravitational perturbations, and its origin could be due to rotational fission following a catastrophic impact.
Cellino Alberto
Farinella Paolo
Paolicchi Paolo
Zappala Vincent
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