If certain debris disks are able to hold onto appreciable amounts of gas, it might push back astronomers» expected deadline for
giant planet formation around young stars, the astronomers speculate.
This finding could offer new insights into the timeline for
giant planet formation around young stars.
Not exact matches
The resonance may date back to the
planets» births and thus may yield insights into the
formation of
giant planets around other stars, including our sun.
We present and exploit new near - infrared images and integral - field spectra of the four gas
giants surrounding HR8799 obtained with SPHERE, the new
planet f... ▽ More The planetary system discovered
around the young A-type HR8799 provides a unique laboratory to: a) test
planet formation theories, b) probe the diversity of system architectures at these separations, and c) perform comparative (exo) planetology.
The detection of close - in
giant planets around other stars was the first clue that this pattern is not universal, and that
planets» orbits can change substantially after their
formation.
This artist's impression shows the
formation of a gas
giant planet around a young star.
On December 1, 2009, two astronomers submitted a pre-print suggesting that the
planet's extreme axial tilt (an obliquity of 97 degrees) may have resulted from the presence of a large moon that has since been ejected from orbit
around the ice
giant by the pull of another
planet during the orbital migration of the
giant planets early in the
formation of the Solar System.
According to the prevalent theory for the moon's
formation — the «
giant - impact hypothesis» — the Earth's axis (the invisible line that runs through the
planet and connects its two magnetic poles,
around which the
planet spins each day) used to run perpendicular to its orbit.