Stars on the main sequence produce energy by fusing hydrogen into?
singleAnswer
helium
Main sequence
Stars on the main sequence produce energy by fusing hydrogen into?
Main sequence Nuclear fusion 13 Trianguli Alpha Mensae HD 28185 Stellar nucleosynthesis Red giant Groombridge 1618 Stellar evolution Sun
All <b>main</b>-<b>sequence stars</b> have a core region where <b>energy</b> is generated ... fuses 
<b>hydrogen</b> together <b>in</b> a series of stages <b>to produce</b> helium. ... as intermediaries <b>in</b> 
the process of <b>fusing hydrogen into</b> helium. For its use <b>in producing energy</b>, see Fusion power. The Sun is a <b>main</b>-<b>sequence</b> 
<b>star</b>, and thus generates its <b>energy</b> by nuclear fusion of <b>hydrogen</b> nuclei <b>into</b>&nbsp;... 13 Trianguli is the Flamsteed designation for a <b>star in</b> the northern constellation 
of Triangulum. ... A stellar classification of G0 V indicates this is a <b>main sequence</b> 
<b>star</b> that is <b>generating energy by fusing hydrogen into</b> helium at its core. α Mensae is the brightest <b>star in</b> the constellation Mensa. At a magnitude of 5.09, 
it is the ... This <b>star</b> has a stellar classification of G7 V, indicating that it is a G-type 
<b>main sequence star</b> that is <b>generating energy by fusing hydrogen into</b> helium at&nbsp;... HD 28185 is similar <b>to</b> our Sun <b>in</b> terms of mass, radius, and luminosity. The <b>star</b> 
is on the <b>main sequence</b> and is <b>generating energy by fusing hydrogen in</b> its&nbsp;... Stellar nucleosynthesis is the creation (nucleosynthesis) of chemical elements by 
nuclear ... <b>In</b> 1939, <b>in</b> a paper entitled &quot;<b>Energy Production in Stars</b>&quot;, Hans Bethe ... 
percent of all <b>stars</b>, with the exception of white dwarfs, are <b>fusing hydrogen</b> by ... 
<b>Main sequence stars</b> accumulate helium <b>in</b> their cores as a result of <b>hydrogen</b>&nbsp;... A red giant is a luminous giant <b>star</b> of low or intermediate mass (roughly 0.3–8 
solar masses ( M ... Red giants differ <b>in</b> a way by which they <b>generate energy</b>: ... 
on the red-giant branch (RGB) that are still <b>fusing hydrogen into</b> helium <b>in</b> a shell 
... Over its <b>main sequence</b> life, the <b>star</b> slowly converts the <b>hydrogen in</b> the core 
<b>into</b>&nbsp;... Groombridge 1618 is a <b>star in</b> the northern constellation Ursa Major. With an 
apparent visual magnitude of +6.6, it lies at or below the threshold of <b>stars</b> visible 
<b>to</b> the naked eye for an average observer. It is relatively close <b>to</b> Earth, at 15.88 
light years. This is a <b>main sequence star</b> of spectral type K7.5 Ve, having just 67
% of the ... <b>main sequence star</b> that is <b>generating energy by fusing hydrogen</b> at its 
core. Stellar evolution is the process by which a <b>star</b> changes over the course of time. 
Depending on ... <b>Stars</b> with at least half the mass of the Sun can also begin <b>to</b> 
<b>generate energy</b> through the ... When a <b>star</b> exhausts the <b>hydrogen in</b> its core, it 
leaves the <b>main sequence</b> and begins <b>to</b> fuse <b>hydrogen in</b> a shell outside the 
core. Since the Sun formed, the <b>main</b> fusion process has involved <b>fusing hydrogen into</b> 
helium. Over the past 4.6 billion years, the amount of helium and its location&nbsp;...
helium
Main sequence