![]() ![]() |
fp: The fraction of these stars having a
planetary system. The gas and dust clouds from which stars are formed
rotate. They have angular momentum - that is rotational
energy - which must be conserved. If, as generally seems the case, the stars themselves are not
rotating rapidly, then the angular momentum must reside elsewhere.
Around half of all stars are in binary or multiple star systems where
the motion of the stars around their common centre of gravity carries
the angular momentum. It is suspected that where the rotation of a
star is slow and it has no stellar companions, then the angular
momentum might reside in one or more unseen planets. It thus seems
that comparatively many stars would have planetary systems. We now have good observational evidence that this is indeed the
case. Not only have about 70 Jupiter-sized planets been detected
around Sun-like stars, but infra-red observations and direct imaging
by the ground- and space-based telescope have also shown that in the
Orion Nebula region, nearly half of all young stars are surrounded by
so called "protoplanetary
discs". These observations imply that about a half of all new stars will
be accompanied by planets.
|
![]()
Life in the Universe
SETI - The Search For Extraterrestrial Intelligence
The Drake Equation
The R* Term
The fp Term
The ne Term
The fl Term
The fi Term
The fc Term
The L Term
![]()
Last updated August 7, 2001