Viktor Safronov

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Viktor Sergeevich Safronov (Russian: Ви́ктор Серге́евич Сафро́нов) (born Velikie Luki; 11 October 1917 in Russia – 18 September 1999 in Moscow, Russia) was a Soviet astronomer who put forward the low-mass-nebula model of planet formation, a consistent picture of how the planets formed from a disk of gas and dust around the Sun.

Biography and legacy

Safronov graduated from

Moscow State University Department of Mechanics and Mathematics in 1941. He defended a dissertation for the Doctor of Physical and Mathematical Sciences in 1968. His scientific interests covered planetary cosmogony, astrophysics and geophysics
.

His planetesimal hypothesis of planet formation is still widely accepted among astronomers, although alternative theories exist (such as the gravitational fragmentation of the protoplanetary disk directly into planets).

A

3615 Safronov, discovered by US-American astronomer Edward L. G. Bowell in 1983, is named after him,[1]
as is
Safronov Regio
on Pluto.

The 1999 BBC documentary miniseries The Planets discusses Safronov's work at length.

Awards

  • USSR Academy of Sciences
    Prize
    (1974)
  • Leonard Prize Meteoritical Society (1989)
  • Kuiper Prize
    in Planetary Science
    (1990)

List of selected publications

  • Evolution of the Protoplanetary Cloud and Formation of the Earth and the Planets. Moscow: Nauka Press, 1969. Trans. NASA TTF 677, 1972.

See also

References

  1. ^ Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names (5th ed.). New York: Springer Verlag. p. 304. .

External links