<p>The AAS Nova article cites <a href="https://ui.adsabs.harvard.edu/abs/2016ApJ...818..108R/abstract" rel="nofollow noreferrer">Rawls et al. 2016</a>,
who analyze light curves and spectra of the eclipsing binary <a href="https://simbad.u-strasbg.fr/simbad/sim-id?Ident=KIC+9246715" rel="nofollow noreferrer">KIC 9246715</a> to estimate its physical properties.
Besides the stellar masses and radii in the article, their Table 2 lists orbital semimajor axis <em>a</em> = 211 <em>R</em><sub>&#9737;</sub> = 147 million km = 0.98 au, and orbital eccentricity <em>e</em> = 0.356.
During the 171-day period, the distance between the two stars varies between 95 and 199 million km, or 0.63 and 1.33 au.</p>

CC BY-SA 4.0
2019-08-25T06:58:15.307Z
2019-08-25T06:58:15.307Z
Mike G
<p>I was going to ask if it's physically possible for one red giant to orbit another, but fortunately, I have just found such a thing--a red giant binary system known only as KIC 9246715.  In <a href="https://aasnova.org/2016/02/17/sizing-up-red-giant-twins/" rel="nofollow noreferrer">this article</a>, all I could find of the distance between the stars is that one orbits the other in an orbit of 171 days.</p>
<p>The only problem with that statement is that it doesn't tell how far one star orbits the other in miles.  In our solar system, a 171-day orbit would be midway between Mercury (orbital revolution:  88 days) and Venus (orbital revolution:  225 days).  Obviously, this couldn't be the case for two stars that are each bigger than our own sun.  But even binaries confer to Kepler's Third Law of Motion, that the farther one body is from its parent, the slower it'll complete one revolution.</p>
<p>So in this real system, <strong>have there been any estimations of how far one star orbits the others measured in miles or kilometers?</strong></p>

CC BY-SA 4.0
2019-08-25T16:34:54.253Z
Note that planetary orbital distances are normally given in Astronomical Units (AU) as kilometers is pretty hard to relate to in this context.
StephenG - Help Ukraine
<star><orbital-elements><red-giant><johannes-kepler>
In System KIC 9246715, How Far Does One Star Orbit the Other?
JohnWDailey
# In System KIC 9246715, How Far Does One Star Orbit the Other?

(Asked by: username_0 on 2019-08-25)

I was going to ask if it's physically possible for one red giant to orbit another, but fortunately, I have just found such a thing--a red giant binary system known only as KIC 9246715. In [this article](https://aasnova.org/2016/02/17/sizing-up-red-giant-twins/), all I could find of the distance between the stars is that one orbits the other in an orbit of 171 days.

The only problem with that statement is that it doesn't tell how far one star orbits the other in miles. In our solar system, a 171-day orbit would be midway between Mercury (orbital revolution: 88 days) and Venus (orbital revolution: 225 days). Obviously, this couldn't be the case for two stars that are each bigger than our own sun. But even binaries confer to Kepler's Third Law of Motion, that the farther one body is from its parent, the slower it'll complete one revolution.

So in this real system, **have there been any estimations of how far one star orbits the others measured in miles or kilometers?**

**Tags:** star, orbital-elements, red-giant, johannes-kepler
> **Comments:**
> **username_1**: Note that planetary orbital distances are normally given in Astronomical Units (AU) as kilometers is pretty hard to relate to in this context.  

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## 1 answers

### Answer by username_2 on 2019-08-25. Score: 4 | Accepted answer

The AAS Nova article cites [Rawls et al. 2016](https://ui.adsabs.harvard.edu/abs/2016ApJ...818..108R/abstract),
who analyze light curves and spectra of the eclipsing binary [KIC 9246715](https://simbad.u-strasbg.fr/simbad/sim-id?Ident=KIC+9246715) to estimate its physical properties.
Besides the stellar masses and radii in the article, their Table 2 lists orbital semimajor axis *a* = 211 *R*☉ = 147 million km = 0.98 au, and orbital eccentricity *e* = 0.356.
During the 171-day period, the distance between the two stars varies between 95 and 199 million km, or 0.63 and 1.33 au.


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