<p>Looking at <a href="http://sci.esa.int/rosetta/14615-comet-67p/" rel="nofollow">this site</a>, there is a table, which has some information.</p>

<blockquote>
  <p>Rotation period: 12.4043 ± 0.0007 * hours    </p>
</blockquote>

<p>It also rotates around a fixed axis</p>

<blockquote>
  <p>recent observations suggest that the axis is tilted about 40 degrees</p>
</blockquote>

<p>There are actually only two objects known to rotate chaotically in the solar system - one is Saturn's moon Hyperion, and the other is a small asteroid called 4179 Toutatis (source: <a href="http://www.guinnessworldrecords.com/records-12000/largest-object-chaotically-rotating/" rel="nofollow">this link from Guinness World Records</a>)</p>

CC BY-SA 3.0
2014-11-20T23:40:06.720Z
40 degrees - that suggests a pretty big "polar night" area. Now if we could get direction of the tilt relative to orbital semi-major axis (at what distance from the Sun equinox happens?)...
SF.
CC BY-SA 3.0
2014-11-20T21:00:45.187Z
2014-11-20T21:00:45.187Z
Superdavo
<p>Some useful sources:</p>

<p>Instructions:
<a href="http://naif.jpl.nasa.gov/pub/naif/self_training/individual_docs/25_shape_model_preview.pdf" rel="nofollow">http://naif.jpl.nasa.gov/pub/naif/self_training/individual_docs/25_shape_model_preview.pdf</a></p>

<p>3d model: <a href="http://naif.jpl.nasa.gov/pub/naif/ROSETTA/kernels/dsk/former_versions/" rel="nofollow">http://naif.jpl.nasa.gov/pub/naif/ROSETTA/kernels/dsk/former_versions/</a></p>

<p><strong>"Ancient", preliminary data from ros_67pcg_v00.tpc:</strong></p>

<ul>
<li>BODY1000012_POLE_RA = ( 270.0 0.0 0.0 )  </li>
<li>BODY1000012_POLE_DEC = (  66.560709 0.0 0.0 )  </li>
<li>BODY1000012_PM = ( 0.0 720.0 0.0 )</li>
<li>BODY1000012_RADII = ( 2.5 1.5 1.5 )  (ellipsoid, kilometers)</li>
</ul>

<p><strong>2012 data from ROS_CGS_RSOC_V03.TPC:</strong></p>

<ul>
<li>BODY1000012_POLE_RA       = (  220.0            0.0            0.0 )</li>
<li>BODY1000012_POLE_DEC      = (  -70.0            0.0            0.0 )</li>
<li>BODY1000012_PM            = (  -86.369364827  679.245283019    0.0 )</li>
<li>BODY1000012_RADII         = (    2.398          1.887          1.532   )</li>
</ul>

<p>"679.245283019" should define rotation period in terms of degrees: 24*360/679.245283019  gives 12.72 (hours?)
Don't know about the "-86.369364827", anyway "PM" should stay for "Prime Meridian".
Anyway the xxx_PM row corresponds to this definition (from pck00010.tpc ):</p>

<ul>
<li>W  =  -86.369364827  + 679.245283019 d</li>
</ul>

<p>No nutation/precession data available.</p>

<p>For xxx_RADII:
"The first number is the largest equatorial radius (the length of the semi-axis containing the prime meridian), the second number is the smaller equatorial radius, and the third is the polar radius."</p>

CC BY-SA 3.0
2014-11-25T14:45:03.673Z
Retrieving orbital data: http://ssd.jpl.nasa.gov/horizons.cgi#top
jumpjack
CC BY-SA 3.0
2014-11-25T14:46:15.350Z
More recent 3d model: ftp://ssols01.esac.esa.int/pub/data/SPICE/ROSETTA/LSSP  (CSHP files)
jumpjack
CC BY-SA 3.0
2014-11-25T14:54:46.183Z
Welcome to Astronomy.SE! It may be helpful for you to provide context for your links, as described in the [help center](http://astronomy.stackexchange.com/help/how-to-answer). Links can be useful, but your answer should still answer the question even if the links aren't available. Additionally, note that you can edit your answer to provide additional information.
Mitch Goshorn
CC BY-SA 3.0
2014-11-25T15:51:50.453Z
I provided links which should be useful to retrieve orientation data for the comet, but I am not actually able to get advantage of these data. Links lead to quite long files (hundreds of lines) which of course would not fit here...
jumpjack
CC BY-SA 3.0
2014-11-25T14:44:29.797Z
2014-11-25T16:51:00.047Z
2014-11-25T16:51:00.047Z
jumpjack
<p>What can be said about 67P/Churyumov-Gerasimenko axial tilt?</p>

<p>Is it fixed (if so, at what value), only changing with precession (at what rate?) or does 67P "tumble" with axial tilt changing over time? (and if so, at what rate?)</p>

<p>I'm interested in estimating the 'polar night' area of the comet, and how it changes over time - but without knowing the rotation properties this is quite hard to do.</p>

<comets><67p><obliquity>
How does 67P rotate?
SF.
# How does 67P rotate?

(Asked by: username_0 on 2014-11-20)

What can be said about 67P/Churyumov-Gerasimenko axial tilt?

Is it fixed (if so, at what value), only changing with precession (at what rate?) or does 67P "tumble" with axial tilt changing over time? (and if so, at what rate?)

I'm interested in estimating the 'polar night' area of the comet, and how it changes over time - but without knowing the rotation properties this is quite hard to do.

**Tags:** comets, 67p, obliquity


---

## 2 answers

### Answer by username_1 on 2014-11-20. Score: 2 | Accepted answer

Looking at [this site](http://sci.esa.int/rosetta/14615-comet-67p/), there is a table, which has some information.

> Rotation period: 12.4043 ± 0.0007 \* hours

It also rotates around a fixed axis

> recent observations suggest that the axis is tilted about 40 degrees

There are actually only two objects known to rotate chaotically in the solar system - one is Saturn's moon Hyperion, and the other is a small asteroid called 4179 Toutatis (source: [this link from Guinness World Records](http://www.guinnessworldrecords.com/records-12000/largest-object-chaotically-rotating/))

> **Comments:**
> **username_0**: 40 degrees - that suggests a pretty big "polar night" area. Now if we could get direction of the tilt relative to orbital semi-major axis (at what distance from the Sun equinox happens?)...  

---

### Answer by username_2 on 2014-11-25. Score: 2

Some useful sources:

Instructions:
<http://naif.jpl.nasa.gov/pub/naif/self_training/individual_docs/25_shape_model_preview.pdf>

3d model: <http://naif.jpl.nasa.gov/pub/naif/ROSETTA/kernels/dsk/former_versions/>

**"Ancient", preliminary data from ros\_67pcg\_v00.tpc:**

* BODY1000012\_POLE\_RA = ( 270.0 0.0 0.0 )
* BODY1000012\_POLE\_DEC = ( 66.560709 0.0 0.0 )
* BODY1000012\_PM = ( 0.0 720.0 0.0 )
* BODY1000012\_RADII = ( 2.5 1.5 1.5 ) (ellipsoid, kilometers)

**2012 data from ROS\_CGS\_RSOC\_V03.TPC:**

* BODY1000012\_POLE\_RA = ( 220.0 0.0 0.0 )
* BODY1000012\_POLE\_DEC = ( -70.0 0.0 0.0 )
* BODY1000012\_PM = ( -86.369364827 679.245283019 0.0 )
* BODY1000012\_RADII = ( 2.398 1.887 1.532 )

"679.245283019" should define rotation period in terms of degrees: 24\*360/679.245283019 gives 12.72 (hours?)
Don't know about the "-86.369364827", anyway "PM" should stay for "Prime Meridian".
Anyway the xxx\_PM row corresponds to this definition (from pck00010.tpc ):

* W = -86.369364827 + 679.245283019 d

No nutation/precession data available.

For xxx\_RADII:
"The first number is the largest equatorial radius (the length of the semi-axis containing the prime meridian), the second number is the smaller equatorial radius, and the third is the polar radius."

> **Comments:**
> **username_2**: Retrieving orbital data: http://ssd.jpl.nasa.gov/horizons.cgi#top  
> **username_2**: More recent 3d model: ftp://ssols01.esac.esa.int/pub/data/SPICE/ROSETTA/LSSP  (CSHP files)  
> **username_3**: Welcome to Astronomy.SE! It may be helpful for you to provide context for your links, as described in the [help center](http://astronomy.stackexchange.com/help/how-to-answer). Links can be useful, but your answer should still answer the question even if the links aren't available. Additionally, note that you can edit your answer to provide additional information.  
> **username_2**: I provided links which should be useful to retrieve orientation data for the comet, but I am not actually able to get advantage of these data. Links lead to quite long files (hundreds of lines) which of course would not fit here...  

---

