Minimum mass
In astronomy, minimum mass is the lower-bound calculated mass of objects like planets, stars, nebulae,[1] and black holes.
Minimum mass is used a lot for extrasolar planets discovered by the radial velocity method. It is found using the binary mass function.
Minimum Mass Media
Unit circle: the radius has length 1. The variable t measures the angle referred to as θ in the text.
Animation showing how the sine function (in red) y = \sin(\theta) is graphed from the y-coordinate (red dot) of a point on the unit circle (in green) at an angle of θ.
References
- ↑ Arbutina, B. (2007-06-01). "The minimum mass ratio of W UMa-type binary systems". Monthly Notices of the Royal Astronomical Society. 377 (4): 1635–1637. doi:10.1111/j.1365-2966.2007.11723.x. ISSN 0035-8711.