QCM predicts that a body of mass [micro] orbiting a central massive object in a gravitationally
bound system obeys the angular momentum L per unit mass quantization condition
Just how big radially is this gravitationally
bound system involving the S-stars according to the QCM fit?
T]c, a characteristic distance for the gravitationally
An alternative planet-formation theory suggests that a piece of the disk becomes gravitationally
unstable and collapses on itself.
These geodynamic computer models show that the base of a magmatically over-thickened and magnesium-rich crust would have been gravitationally
unstable at mantle temperatures greater than 1,500 to 1,550 degrees Celsius and this would have caused it to sink in a process called 'delamination'.
Planets that share the same host star gravitationally
interact with each other.
The Fomalhaut team led by Kalas considers this circumstantial evidence there may be other planet-like bodies in the system that gravitationally
disturbed Fomalhaut b to place it in such a highly eccentric orbit.
Galaxies such as Segue 1, which have such a tiny amount of visible material to gravitationally
disturb the dark matter, are the best places to reveal the true distribution and nature of the unseen material.
We find excellent agreement with QCM for ten galactic clusters, demonstrating that dark matter is not needed to explain the rotation velocities and providing further support to the hypothesis that all gravitationally
bound systems have QCM quantization states.
Beletsky said that the two brown dwarfs are separated by about three times the distance between the Earth and the Sun, asserting that the binary brown dwarf systems are gravitationally
bound and orbit about each other.
When more than two stars share a small space, they gravitationally
pull on each other in a chaotic dance.
A hidden planet, for example, can distort the sequence of transits if it gravitationally
pulls on the transiting planet and delays some transits relative to others.