Is the Sun a low-mass star or a medium-mass star?

In summary, the Sun is known as both a low-mass and medium-mass star in different sources. The range of what qualifies as a low-mass or medium-mass star varies, with some sources considering the Sun as low-mass and others as medium-mass. The difference in classification depends on the desired criteria and purpose. Additionally, the Hertsprung-Russel diagram shows the characteristics and behaviors of stars, with larger stars being brighter and having different zones of convection and radiation. Ultimately, the classification of the Sun as low-mass or medium-mass depends on the chosen definition and purpose.
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xoxo1001
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In many text, the Sun is referred to as a low-mass star, yet it is also referred to as a medium-mass (or intermediate-mass) star in some other text. Which one is "correct"? What is the range of low-mass vs medium-mass? Is it really just low-mass vs high-mass and that medium-mass is just the upper limit of the low-mass portion?

For example, here (https://www.le.ac.uk/se/centres/sci/selfstudy/eab4.htm) says low-mass stars are "stars with masses less than half the mass of the Sun". If this is true, then the Sun is technically medium-mass. However, here (https://sites.uAlberta.ca/~pogosyan/teaching/ASTRO_122/lect17/lecture17.html) says low-mass stars are between 0.4 MSun to 4 MSun, which means that the Sun is considered as low-mass.

Confusing.
 
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Low-mass and medium-mass are relative terms, it seems.
 
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The description of a high-mass star on the first web page seems wrong to me. I'm no expert in astronomy, but I'm fairly certain that a 3-solar mass star is not going to end its life as a supernova.

How a star evolves depends primarily on its mass. A low-mass star will evolve in one way while a high-mass star will evolve in a markedly different way. Depending on the criteria you choose to divide up stellar evolution, you can get different descriptions of what kinds of star qualify low mass, intermediate mass, and high mass.

When I teach ASTR 101, we divide up stars into two classes: low mass stars that will end their lives as a white dwarf and high-mass stars that will ultimately die as a Type II supernova. The Sun would fall into the first class.
 
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xoxo1001 said:
Which one is "correct"? What is the range of low-mass vs medium-mass?
With respect, who actually cares, except in a game of Top Trumps? The Sun is somewhere in between the very biggest and the very smallest stars. It is what it is and it does what it does and there is a load more of information about the Sun than about any others.
There are plenty of statistics around about millions / billions of stars that have been catalogued.
 
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  • #5
sophiecentaur said:
The Sun is somewhere in between the very biggest and the very smallest stars.
I could have been more helpful there. The Hertsprung Russel diagram gives a graph of characteristics of all (most) of the stars that we have observed. I chose this image because it shows dots where (some) stars have been measured.
hrdiagram_01.jpg

The Sun can be seen near the middle of that line of stars which follow 'normal' behaviour during their lifetimes. They spend most of the time somewhere on this Main Sequence line so ,when you observe a load of stars, most of them will sit somewhere on this line. There is a general rule which says Big Stars are brighter than small ones. So the big ones are top left and the small ones are bottom right for most of their lives.
 
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xoxo1001 said:
In many text, the Sun is referred to as a low-mass star, yet it is also referred to as a medium-mass (or intermediate-mass) star in some other text. Which one is "correct"?
Usually, when more than one definition is available, the choice of which definition makes the most sense depends upon why you want to know.
 
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ohwilleke said:
which definition makes the most sense depends upon why you want to know
Just like top Trumps :wink:. Even an Austin Seven can win.
 
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Red dwarfs are main sequence stars. They have convection all the way to the core.

Some stars have a radiative zone and convection in the upper layers.

Larger stars the radiative zone extends to the surface.

Some huge stars are fully convective.
 
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1. Is the Sun considered a low-mass star or a medium-mass star?

The Sun is considered a medium-mass star, with a mass that falls within the range of 0.8 to 1.4 times the mass of our Sun. This classification is based on the mass-luminosity relationship, which states that a star's mass is directly proportional to its luminosity.

2. What is the mass of the Sun compared to other stars?

The Sun's mass is considered average compared to other stars in our galaxy. It is larger than most low-mass stars, but smaller than high-mass stars. The majority of stars in our galaxy have masses similar to the Sun.

3. How does the Sun's mass affect its lifespan?

The Sun's mass plays a significant role in determining its lifespan. As a medium-mass star, the Sun is expected to have a lifespan of about 10 billion years. This is because medium-mass stars have a balance between the inward pull of gravity and the outward push of nuclear fusion, allowing them to maintain a stable energy output for a longer period of time.

4. What would happen if the Sun had a higher or lower mass?

If the Sun had a higher mass (greater than 1.4 times the mass of our Sun), it would be considered a high-mass star and would have a shorter lifespan. It would also have a much higher luminosity and would eventually end its life in a supernova explosion. If the Sun had a lower mass (less than 0.8 times the mass of our Sun), it would be considered a low-mass star and would have a longer lifespan but a lower luminosity. It would eventually end its life as a white dwarf.

5. How do scientists determine the mass of stars?

Scientists determine the mass of stars through various methods, including observing the star's motion in a binary system, studying its spectral lines, and using mathematical models to estimate its mass based on its luminosity and temperature. These methods allow scientists to accurately determine the mass of stars, including the Sun.

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