Which is a type of star found on the lower end of the main sequence?
multipleQAs
Which is a type of star found on the lower end of the main sequence, based on its mass? Which is a type of star found on the lower end of the main sequence, based on its spectral class?
Stars below about 1.5 times the mass of the Sun
stars of spectral class F or cooler F or cooler
Main sequence
type of star found on the lower end of the main sequence
Main sequence Red dwarf Cepheid variable O-type star Stellar evolution White dwarf Subgiant Red giant Stellar core Star
When he plotted the spectral <b>types</b> of these <b>stars</b> against their absolute 
magnitude, he <b>found</b> that dwarf <b>stars</b> followed a distinct relationship. This allowed 
the real&nbsp;... A red dwarf is the smallest and coolest <b>kind of star</b> on the <b>main sequence</b>. Red 
dwarfs are by far ... The <b>lower</b> the mass of a red dwarf, the longer the lifespan. ... 
As giant <b>stars end</b> their short lives in supernova explosions, they spew out the ... 
indicate that long-orbital-period Neptune-mass planets are <b>found</b> around one in&nbsp;... Delta Scuti variables are A-<b>type stars</b> on or near the <b>main sequence</b> at the <b>lower</b> 
<b>end</b> of the instability strip and were originally referred to as dwarf Cepheids. O-<b>type stars</b> form only a tiny fraction of <b>main</b>-<b>sequence stars</b> and the vast majority 
of these are towards the <b>lower end</b> of the mass range. The most massive and&nbsp;... Stellar evolution is the process by which a <b>star</b> changes over the course of time. 
Depending on the mass of the <b>star</b>, its lifetime can <b>range</b> from a few million ... A 
mid-sized yellow dwarf <b>star</b>, like the Sun, will remain on the <b>main sequence</b> for ... 
<b>stars</b> cluster towards the cool <b>end</b> of the horizontal branch as K-<b>type</b> giants and 
are&nbsp;... A white dwarf, also called a degenerate dwarf, is a stellar core remnant 
composed mostly of ... White dwarfs were <b>found</b> to be extremely dense soon after 
their discovery. If a <b>star</b> is in ... If the mass of a <b>main</b>-<b>sequence star</b> is <b>lower</b> than 
approximately half a solar mass, it will never become hot enough to fuse helium 
in its core. A subgiant is a <b>star</b> that is brighter than a normal <b>main</b>-<b>sequence star</b> of the same 
spectral class ... <b>Stars</b> with a subgiant spectral <b>type</b> are not always on the 
evolutionary subgiant branch, and vice versa. ... This hook is generally defined as 
the <b>end of the main sequence</b> and the start of the subgiant branch in these <b>stars</b>. A red giant is a luminous giant <b>star</b> of low or intermediate mass (roughly 0.3–8 
solar masses ( M ☉)) in a late phase of stellar evolution. The outer atmosphere is 
inflated and tenuous, making the radius large and the surface temperature 
around 5,000 K (4,700 °C; 8,500 °F) or <b>lower</b>. ... Red giants are evolved from 
<b>main</b>-<b>sequence stars</b> with masses in the <b>range</b>&nbsp;... A stellar core is the extremely hot, dense region at the center of a <b>star</b>. For an 
ordinary <b>main sequence star</b>, the core region is the volume where the ... At <b>lower</b> 
stellar mass, the outer convection shell takes up an increasing ... These very low 
mass <b>stars</b> (VLMS) occupy the late <b>range</b> of the M-<b>type main</b>-<b>sequence stars</b>, or 
red&nbsp;... False color imagery of the Sun, a G-<b>type main</b>-<b>sequence star</b>, the closest to Earth. 
A <b>star</b> is an astronomical object consisting of a luminous spheroid of plasma held 
together by its ... Near the <b>end</b> of its life, a <b>star</b> can also contain degenerate matter
. ... <b>main sequence stars</b> can have surface temperatures of 50,000 K. <b>Smaller</b>&nbsp;...
Van Biesbroeck 's star
Main sequence