Take the most common type of star in the Milky Way - so -
called red dwarf stars that are cooler, smaller and longer - lived than stars like the sun.
However, most stars in the galaxy, around 75 %, are lower mass stars
called red dwarfs, or M stars (See Figure 1).
Not exact matches
Consider, for instance, the
red dwarf star
called TRAPPIST - 1, just under 40 light - years away.
Boss has recently proposed a similar effect to explain the discovery of two gas giants and two so -
called super-Earths, or big rocky planets, each orbiting a small
red dwarf star.
In May, Drake Deming of NASA was collecting data he hoped might reveal a super-Earth in the habitable zone of a
red dwarf (a small and relatively cool star)
called Gliese 436; NASA had allowed him to use a spacecraft
called Epoxi, which is on its way to a rendezvous with a comet, to observe several stars that are already known to have planets.
The star is a
red dwarf just 4.3 light years away from us with a planet
called Proxima Centauri b orbiting in the habitable zone.
The planet circles a dim
red dwarf called Gliese 876, just 15 light - years from Earth.
The star,
called Gliese 1132, is an M
dwarf (commonly known as a
red dwarf).
As stars like our sun age, they puff up into
red giants and then gradually lose about half or more of their mass, shrinking into skeletons of stars,
called white
dwarfs.
The two planets orbit a star
called K2 - 18, which is a
red dwarf star (dimmer and smaller than our sun) lying about 111 light - years from Earth.
It orbits a
red dwarf star about 200 light years away, which is
called K2 - 155.
When this happens, smaller stars expand into what astronomers
call red giants, then shrink into faint white
dwarfs, according to NASA.