<p>Higher mass stars will have shorter lives.  Even though they have more fuel for nucleosynthesis, they burn this fuel much quicker than lower mass stars.</p>
<p>Generally, you should think of &quot;red-giant&quot; as an evolutionary phase and not a particular type of star.</p>
<p>Looking at the Scheller et al. (Aston. Astrophys. Suppl., 96, 269, 1992) data given in one of the comments, you want to compare the times denoted by points 5 and 6: ascent of the (first) red giant branch.  For a one solar mass star, the elapsed time ascending the giant branch is 634 million years.  By comparison, the time for the same phase for a five solar mass star is 0.289 million years.</p>
<p>When looking at the Hertzsprung-Russell chart (surface luminosity vs effective temperature), the RGB tracks at lower masses are all bunched up.  Therefore, it is very difficult to discern stellar mass (and age) from just luminosity and temperature.  By looking at chemical composition through spectroscopy, it is possible to infer mass by the different types of nucleosynthesis.</p>

CC BY-SA 4.0
2021-03-13T21:32:32.857Z
2021-03-13T21:32:32.857Z
Emanuel V
<p>It turns out that red giant stars are not defined by uniform mass.  Some can be only one-third as massive as our sun, whereas others can be eight times as massive.  So I'm calling the both sides &quot;low-mass&quot; and &quot;high-mass&quot;, respectively.</p>
<p>I have been told that red giants last only as long as one billion years, but considering that lower masses equal longer lifespans, I have to ask--is it the high-mass red giants that have the one-G lifespan, or is it the low-mass?</p>

CC BY-SA 4.0
2021-03-10T14:10:58.740Z
I found Table 2 in the manuscript [Red giant masses and ages derived from carbon and nitrogen abundances](https://core.ac.uk/download/pdf/78472841.pdf) interesting.
B--rian
CC BY-SA 4.0
2021-03-10T14:12:44.320Z
Also maybe helpful: Figure 4 of https://courses.lumenlearning.com/astronomy/chapter/evolution-from-the-main-sequence-to-red-giants/
B--rian
CC BY-SA 4.0
2021-03-10T14:14:27.930Z
Related: https://astronomy.stackexchange.com/questions/34267/relation-between-initial-mass-and-evolutionary-phases-lifetimes
B--rian
<star><stellar-astrophysics><red-giant><stellar-dynamics>
Do low-mass red giants last longer than high-mass red giants?
JohnWDailey
# Do low-mass red giants last longer than high-mass red giants?

(Asked by: username_0 on 2021-03-09)

It turns out that red giant stars are not defined by uniform mass. Some can be only one-third as massive as our sun, whereas others can be eight times as massive. So I'm calling the both sides "low-mass" and "high-mass", respectively.

I have been told that red giants last only as long as one billion years, but considering that lower masses equal longer lifespans, I have to ask--is it the high-mass red giants that have the one-G lifespan, or is it the low-mass?

**Tags:** star, stellar-astrophysics, red-giant, stellar-dynamics

> **Comments:**
> **username_1**: I found Table 2 in the manuscript [Red giant masses and ages derived from carbon and nitrogen abundances](https://core.ac.uk/download/pdf/78472841.pdf) interesting.  
> **username_1**: Also maybe helpful: Figure 4 of https://courses.lumenlearning.com/astronomy/chapter/evolution-from-the-main-sequence-to-red-giants/  
> **username_1**: Related: https://astronomy.stackexchange.com/questions/34267/relation-between-initial-mass-and-evolutionary-phases-lifetimes  

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## 1 answers

### Answer by username_2 on 2021-03-13. Score: 3

Higher mass stars will have shorter lives. Even though they have more fuel for nucleosynthesis, they burn this fuel much quicker than lower mass stars.

Generally, you should think of "red-giant" as an evolutionary phase and not a particular type of star.

Looking at the Scheller et al. (Aston. Astrophys. Suppl., 96, 269, 1992) data given in one of the comments, you want to compare the times denoted by points 5 and 6: ascent of the (first) red giant branch. For a one solar mass star, the elapsed time ascending the giant branch is 634 million years. By comparison, the time for the same phase for a five solar mass star is 0.289 million years.

When looking at the Hertzsprung-Russell chart (surface luminosity vs effective temperature), the RGB tracks at lower masses are all bunched up. Therefore, it is very difficult to discern stellar mass (and age) from just luminosity and temperature. By looking at chemical composition through spectroscopy, it is possible to infer mass by the different types of nucleosynthesis.


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