<p>Yes, you are correct. The luminosities can be added. Luminosity is the amount of electromagnetic energy emitted per unit of time (measured in <span class="math-container">$ \textrm{J} \cdot \textrm{s}^{-1} $</span> or <span class="math-container">$\textrm{W}$</span>). So if you have a multiple star system, the total amount of energy emitted (i.e. the total luminosity) is simply the sum of the energy emitted by each of its components.</p>
<p>This does not take into account any absorption of the radiation of one of the components by one of the others.</p>
<p>In the book by Jean Meeus [1], the formula for adding stellar magnitudes can be found in Chapter 56:</p>
<p><span class="math-container">$$ m = -2.5 \log_{10} \sum_{i=1}^{n} 10^{-0.4 m_i} $$</span></p>
<p>This formula is for the apparent magnitude, but would also apply for the absolute magnitude, which, after all, is only the apparent magnitude at <span class="math-container">$10\,\textrm{pc}$</span> distance.</p>
<p><span class="math-container">$$ M = -2.5 \log_{10} \sum_{i=1}^{n} 10^{-0.4 M_i} $$</span></p>
<p>[1] Jean Meeus, 1998, <em>Chapter 56: Stellar Magnitudes</em>, from Astronomical Algorithms, Willmann-Bell Inc. Second Edition.</p>

CC BY-SA 4.0
2020-11-02T22:30:35.187Z
So what is the formula for absolute magnitude?
WarpPrime
CC BY-SA 4.0
2020-11-03T08:02:15.600Z
The same, but with the visible magnitude m replaced by the absolute magnitude M. I've added it to the answer for completeness sake.
Dieudonné
CC BY-SA 4.0
2020-11-02T21:37:27.173Z
2020-11-03T08:03:45.703Z
2020-11-03T08:03:45.703Z
Dieudonné
<p>We know that the absolute magnitude of a single star can be calculated with the formulae:
<span class="math-container">$$M_{\rm bol} = 4.75 -2.5 \log_{10} \left(\frac{L_*}{L_{\odot}}\right)\ ,$$</span>
<span class="math-container">$$M = -2.5  \log_{10}(L_* / L_0),$$</span>
where <span class="math-container">$L_*$</span> is the luminosity of the given star, and <span class="math-container">$L_0$</span> being the luminosity of a magnitude 0 star at a distance of 10 pc (<span class="math-container">$79L_\odot)$</span>.</p>
<p>However, this only works for a single star, not multiple star systems. Is the formula for the absolute magnitude of a multiple star system defined as <span class="math-container">$L_*=L_1+L_2+...+L_n$</span> (the sum of all luminosities in the system), where <span class="math-container">$L_n$</span> is the luminosity of a star in the system, or is it something else?</p>

CC BY-SA 4.0
2020-11-03T08:09:22.670Z
I do not think you can talk of the luminosity of a star at 10pc. The luminosity is the electromagnetic energy emitted per second and is not dependent on the distance to the object.You would probably need the *Irradiance* instead, which is the amount of energy received per surface area. The Irradiance changes with distance to the object.
Dieudonné
<star><binary-star><mathematics><absolute-magnitude><multiple-star-systems>
Calculate the absolute magnitude for a multi-star system
WarpPrime
# Calculate the absolute magnitude for a multi-star system

(Asked by: username_0 on 2020-11-02)

We know that the absolute magnitude of a single star can be calculated with the formulae:
$$M\_{\rm bol} = 4.75 -2.5 \log\_{10} \left(\frac{L\_\*}{L\_{\odot}}\right)\ ,$$
$$M = -2.5 \log\_{10}(L\_\* / L\_0),$$
where $L\_\*$ is the luminosity of the given star, and $L\_0$ being the luminosity of a magnitude 0 star at a distance of 10 pc ($79L\_\odot)$.

However, this only works for a single star, not multiple star systems. Is the formula for the absolute magnitude of a multiple star system defined as $L\_\*=L\_1+L\_2+...+L\_n$ (the sum of all luminosities in the system), where $L\_n$ is the luminosity of a star in the system, or is it something else?

**Tags:** star, binary-star, mathematics, absolute-magnitude, multiple-star-systems

> **Comments:**
> **username_1**: I do not think you can talk of the luminosity of a star at 10pc. The luminosity is the electromagnetic energy emitted per second and is not dependent on the distance to the object.You would probably need the *Irradiance* instead, which is the amount of energy received per surface area. The Irradiance changes with distance to the object.  

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## 1 answers

### Answer by username_1 on 2020-11-02. Score: 4 | Accepted answer

Yes, you are correct. The luminosities can be added. Luminosity is the amount of electromagnetic energy emitted per unit of time (measured in $ \textrm{J} \cdot \textrm{s}^{-1} $ or $\textrm{W}$). So if you have a multiple star system, the total amount of energy emitted (i.e. the total luminosity) is simply the sum of the energy emitted by each of its components.

This does not take into account any absorption of the radiation of one of the components by one of the others.

In the book by Jean Meeus [1], the formula for adding stellar magnitudes can be found in Chapter 56:

$$ m = -2.5 \log\_{10} \sum\_{i=1}^{n} 10^{-0.4 m\_i} $$

This formula is for the apparent magnitude, but would also apply for the absolute magnitude, which, after all, is only the apparent magnitude at $10\,\textrm{pc}$ distance.

$$ M = -2.5 \log\_{10} \sum\_{i=1}^{n} 10^{-0.4 M\_i} $$

[1] Jean Meeus, 1998, *Chapter 56: Stellar Magnitudes*, from Astronomical Algorithms, Willmann-Bell Inc. Second Edition.

> **Comments:**
> **username_0**: So what is the formula for absolute magnitude?  
> **username_1**: The same, but with the visible magnitude m replaced by the absolute magnitude M. I've added it to the answer for completeness sake.  

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