<blockquote>
<p>How much mass would have to be added to the Sun to significantly alter
its characteristics</p>
</blockquote>
<p>Asking how much would be significant is inexact.  <a href="https://en.wikipedia.org/wiki/G-type_main-sequence_star" rel="nofollow noreferrer">The Sun is classified as a G2V main sequence star</a>.   Though the chart lists one solar mass as G4V, so there's some variation in there.   The classifications seem to relate to temperature.    To go 1 step up (and using the sun or any G star), the increase of one ranking (decrease in 1 number after G) alternates between a 2% and 5% increase in mass.   I'm going to round that to 3%-4%, so for our sun, that's about 30-40 Jupiters (31.4-41.9 if you care about significant digits), but I'm going with 30-40 Jupiter masses added for each step up the classification ladder, ignoring the effects of impact, which would be considerable.</p>
<p>That increase of one in classification level viewed from Earth would be quite significant.   3% more mass corresponds to about the 4th power of that or 12.5% more luminosity.   Earth would be very different if the Sun was 12.5% more luminous.  I would think that would be enough to turn Earth at least into a steam-bath, perhaps a full blown runaway greenhouse effect due to the abundance of water and feedback mechanisms.   Adding mass would also change Earth's orbit, drawing it in slightly and shortening the year, so the increase from Earth would be a bit more than 12.5%.</p>
<p>The stellar mass math goes something like this.</p>
<p>Lifespan decreases by about the 3rd power of an increase in mass.</p>
<p>Energy output or luminosity increases by about the 4th power of the mass, around 1 solar mass.  This increase slows down to about the 3.5th power with more massive main sequence stars.</p>
<p>Surface temperature increases slightly with mass, perhaps 10-20 K per 1% increase in mass, or about a 1% increase in temperature for every 3% increase in mass would be about ballpark.</p>
<p>Radius increases with added mass too, so the heavier sun would be both brighter and larger.   The radius increases enough that the surface gravity decreases.  A 3% increase in mass corresponds to around a 2% increase in radius, so the size wouldn't appear very different on these scales.</p>
<p>If the Sun became just 0.5% to 1% more luminous  (about 1.5-3 Jupiters in mass) that would be in the ballpark to man made climate change so far.  Enough to melt surface ice over time and cause oceans to rise, so, significant depends a lot on point of view.</p>
<p>These numbers should be taken with a grain of salt because other factors like metallicity and age matter too.   Stars like our Sun also change in size and luminosity during their lifetime, growing both larger and more luminous over time.  There are more massive main sequence stars than our Sun that are less luminous because they're younger and the reverse as well, though off hand, I can't name any.</p>
<p>Errors fixed.  Thankyou for pointing out.</p>
<p>I want to add, since you mention XKCD in the question, if Randall Munroe was answering this question, he would take it to the extreme, answering what happens if you add million Jupiters, or a billion.   Fun times.  Without his clever diagrams, it wouldn't be the same, so I'll stop here.</p>

CC BY-SA 4.0
2020-11-17T22:02:52.983Z
Would it be G3V instead of G5V, as G5 is cooler than G4?
WarpPrime
CC BY-SA 4.0
2020-11-17T22:09:40.100Z
Your absolutely right.  G3V is 1 step up/more massive.  I got that switched in my mind.
userLTK
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2020-11-18T05:03:04.673Z
I've made an edit to the question but I don't think it impacts your answer.
uhoh
CC BY-SA 4.0
2020-11-18T07:22:38.327Z
The Sun is a G2V star.
ProfRob
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2020-11-18T18:30:47.290Z
@RobJeffries  Sorry for the novice mistake.  I read the chart, saw one solar mass, didn't read far enough.
userLTK
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2020-11-17T21:15:15.303Z
2020-11-18T18:37:44.930Z
2020-11-18T18:37:44.930Z
userLTK
<p>While this might at first sound like an <a href="http://whatif.xkcd.com" rel="nofollow noreferrer">XKCD What If?</a> question, let's proceed with it because astronomical objects do occasionally merge.</p>
<p>How much mass would have to be added to the Sun to significantly alter its characteristics (lifetime, spectral type, size, etc.)?</p>
<hr />
<p>As an example, from Wikipedia's <a href="https://en.wikipedia.org/wiki/Rogue_planet" rel="nofollow noreferrer">Rogue planet</a>:</p>
<blockquote>
<p>A rogue planet (also termed an interstellar planet, nomad planet, free-floating planet, unbound planet, orphan planet, wandering planet, starless planet, or sunless planet) is a planetary-mass object that does not orbit a star directly. Such objects have been ejected from the planetary system in which they formed or have never been gravitationally bound to any star or brown dwarf. <strong>The Milky Way alone may have billions to trillions of rogue planets, a range which the upcoming Nancy Grace Roman Space Telescope will likely be able to narrow down.</strong></p>
</blockquote>
<p>...if one doesn't fall into the Sun first!</p>
<p>Just in the last few years alone we've seen both a comet and an asteroid with extra-solar velocities enter the inner solar system, compare that to the 4.6 billion year age of the Sun.</p>
<ul>
<li><a href="https://en.wikipedia.org/wiki/2I/Borisov" rel="nofollow noreferrer">2I/Borisov</a> 2.01 AU perihelion</li>
<li><a href="https://en.wikipedia.org/wiki/%CA%BBOumuamua" rel="nofollow noreferrer">ʻOumuamua</a> 0.255 AU perihelion</li>
</ul>

CC BY-SA 4.0
2020-11-17T20:51:47.850Z
Define "significantly"
James K
CC BY-SA 4.0
2020-11-18T05:11:31.950Z
I've made an edit to your question, feel free to roll back or edit further.
uhoh
CC BY-SA 4.0
2020-11-18T07:25:20.967Z
Comets fall into the Sun frequently. It is a negligible mass gain compared with mass lost in the solar wind.
ProfRob
<the-sun><mass><collision>
How much mass would have to be added to the Sun to significantly alter any of its characteristics?
WarpPrime
# How much mass would have to be added to the Sun to significantly alter any of its characteristics?

(Asked by: username_0 on 2020-11-17)

While this might at first sound like an [XKCD What If?](http://whatif.xkcd.com) question, let's proceed with it because astronomical objects do occasionally merge.

How much mass would have to be added to the Sun to significantly alter its characteristics (lifetime, spectral type, size, etc.)?

---

As an example, from Wikipedia's [Rogue planet](https://en.wikipedia.org/wiki/Rogue_planet):

> A rogue planet (also termed an interstellar planet, nomad planet, free-floating planet, unbound planet, orphan planet, wandering planet, starless planet, or sunless planet) is a planetary-mass object that does not orbit a star directly. Such objects have been ejected from the planetary system in which they formed or have never been gravitationally bound to any star or brown dwarf. **The Milky Way alone may have billions to trillions of rogue planets, a range which the upcoming Nancy Grace Roman Space Telescope will likely be able to narrow down.**

...if one doesn't fall into the Sun first!

Just in the last few years alone we've seen both a comet and an asteroid with extra-solar velocities enter the inner solar system, compare that to the 4.6 billion year age of the Sun.

* [2I/Borisov](https://en.wikipedia.org/wiki/2I/Borisov) 2.01 AU perihelion
* [ʻOumuamua](https://en.wikipedia.org/wiki/%CA%BBOumuamua) 0.255 AU perihelion

**Tags:** the-sun, mass, collision

> **Comments:**
> **username_1**: Define "significantly"  
> **username_2**: I've made an edit to your question, feel free to roll back or edit further.  
> **username_3**: Comets fall into the Sun frequently. It is a negligible mass gain compared with mass lost in the solar wind.  

---

## 1 answers

### Answer by username_4 on 2020-11-17. Score: 4 | Accepted answer

> How much mass would have to be added to the Sun to significantly alter
> its characteristics

Asking how much would be significant is inexact. [The Sun is classified as a G2V main sequence star](https://en.wikipedia.org/wiki/G-type_main-sequence_star). Though the chart lists one solar mass as G4V, so there's some variation in there. The classifications seem to relate to temperature. To go 1 step up (and using the sun or any G star), the increase of one ranking (decrease in 1 number after G) alternates between a 2% and 5% increase in mass. I'm going to round that to 3%-4%, so for our sun, that's about 30-40 Jupiters (31.4-41.9 if you care about significant digits), but I'm going with 30-40 Jupiter masses added for each step up the classification ladder, ignoring the effects of impact, which would be considerable.

That increase of one in classification level viewed from Earth would be quite significant. 3% more mass corresponds to about the 4th power of that or 12.5% more luminosity. Earth would be very different if the Sun was 12.5% more luminous. I would think that would be enough to turn Earth at least into a steam-bath, perhaps a full blown runaway greenhouse effect due to the abundance of water and feedback mechanisms. Adding mass would also change Earth's orbit, drawing it in slightly and shortening the year, so the increase from Earth would be a bit more than 12.5%.

The stellar mass math goes something like this.

Lifespan decreases by about the 3rd power of an increase in mass.

Energy output or luminosity increases by about the 4th power of the mass, around 1 solar mass. This increase slows down to about the 3.5th power with more massive main sequence stars.

Surface temperature increases slightly with mass, perhaps 10-20 K per 1% increase in mass, or about a 1% increase in temperature for every 3% increase in mass would be about ballpark.

Radius increases with added mass too, so the heavier sun would be both brighter and larger. The radius increases enough that the surface gravity decreases. A 3% increase in mass corresponds to around a 2% increase in radius, so the size wouldn't appear very different on these scales.

If the Sun became just 0.5% to 1% more luminous (about 1.5-3 Jupiters in mass) that would be in the ballpark to man made climate change so far. Enough to melt surface ice over time and cause oceans to rise, so, significant depends a lot on point of view.

These numbers should be taken with a grain of salt because other factors like metallicity and age matter too. Stars like our Sun also change in size and luminosity during their lifetime, growing both larger and more luminous over time. There are more massive main sequence stars than our Sun that are less luminous because they're younger and the reverse as well, though off hand, I can't name any.

Errors fixed. Thankyou for pointing out.

I want to add, since you mention XKCD in the question, if Randall Munroe was answering this question, he would take it to the extreme, answering what happens if you add million Jupiters, or a billion. Fun times. Without his clever diagrams, it wouldn't be the same, so I'll stop here.

> **Comments:**
> **username_0**: Would it be G3V instead of G5V, as G5 is cooler than G4?  
> **username_4**: Your absolutely right.  G3V is 1 step up/more massive.  I got that switched in my mind.  
> **username_2**: I've made an edit to the question but I don't think it impacts your answer.  
> **username_3**: The Sun is a G2V star.  
> **username_4**: @RobJeffries  Sorry for the novice mistake.  I read the chart, saw one solar mass, didn't read far enough.  

---

