Rosetta navigation camera (NAVCAM) image taken on 22 August 2014 at a distance of about 64 km from comet 67P/C-G.
CometWatch – 22 August
- access_time 23/08/2014
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Written by
Claudia
Claudia is an astronomer and science writer working for ESA.
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23 August 2014
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26 comments
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Ambition the film
Click image to watch Ambition
Read Rosetta: the ambition to turn science fiction into science fact
Mission milestones
Event | Date |
Launch | 2 Mar 2004 |
Earth swingby | 4 Mar 2005 |
Mars swingby | 25 Feb 2007 |
... more |
Discussion: 26 comments
Encore une autre image magnifique, j’adore cette mission 🙂
My theory is that originally eons ago the Comet was spherical, due to its orbit as it came into our Solar system and became warmed up it sublimated water and gases which would be jetted from the part receiving the most heating from Solar rays. That is the most solid part, as this occurred then the dust etc. was ejected into space and slowly the valley almost cutting the Comet in half was formed.
I think now that another pass around Our Sun may cause enough sublimation to actually severe the 2 parts and make 2 Comets!
This is just a theory, but may explain the odd shape of the Comet at this time.
I welcome comment on this.
Clive
Or, it was two clumps, slowly orbiting and weakly attracted to each other, that gradually got close enough to ‘touch’, but, continue to ‘tumble’ around their common center of mass. The stuff in the ‘isthmus’ is just dust & small debris collected by their mutual weak gravity. Would be nice to have a density print of the two (?) snowball’s interiors and the ‘isthmus. Seems like a simpler explanation, and after continued passes in toward the sun, should retain it’s basic configuration. Nice we’ll see after the current pass, which, being outside earth’s orbit, is not, really, very close to the sun …
Because of the many meteor impacts which are visble around the comet, I don’t think that the constriction is the result of erosion by the sunwind. Otherwise the sunwind erosion should have flatten the rest of the comet as well. And most of all the sunwind erosion should have mage a smooth constreiction in the” neck” wich is not the case…
I think that we are looking at the genisis of the comet; Two heated masses in a semi-liquid state.clashes and due their own kinetic energy and different directions they want to split up again but the gravity and adhesion forces are a bit stronger and holds the two parts together in a sort of potato shape. Thesame sort of shape when waterdrops collide.
Philip
This is amazing, it seems from this and the other photos that this centre ‘neck’ potion (valley, gorge) was either gouged out with a glancing blow, leaving the cliff faces intact or collapsed into itself leaving just soft material at the bottom and boulders. The striations on the ‘head’ seems to indicate a rejoining.
But hey! I’m only an armchair comet watcher 🙂
How about a rotating binary of two snowballs, gradually getting closer until they touch?
Sorry Claudia,
That should read ‘portion’ not ‘potion’
Ps. Thanks for the posts.
David
Are we gonna see any more pic’s from the OSIRIS cam?
And are there boulders on the move?
Thank you for your precious time
Hmmm…
On the other hand… check out asteroid Toutatis: https://www.youtube.com/watch?v=fo38qU00HlQ
and Itokawa:
https://www.youtube.com/watch?v=0cnIGdrrM6I
Since asteroids so often look potato-shaped and double-lobed, maybe we should be drawing conclusions from studying asteroids. No ice or sublimation needed?
…Just playing devil’s advocate (yes, I drove my professors crazy).
Indeed. Here some higher resolution images of 4179 Toutatis from the Chinese Chang’e 2 spacecraft.
https://phys.org/news/2013-12-chinese-flyby-asteroid-space-rubble.html
Like 67P/ C-G there are boulders and double lobed. Unlike 67 C-G, no layering and striations, also no outgassing.
Very different types of objects for sure.
Nice that we can see more surface detail now that we are closer.
Striations on head now clear it’s not layering, leaving us to work out how it was eroded.
Liked the idea that the neck was gouged out but how did the glancing blow go right round the neck? MAybe it was Potato peeler?
William I agree with you comets and astoroids are beginning to look very similar to the point you have to ask do they have similar birth.
Gently accumulating ice and dust in a very cold part of the solar system seems to be less and less likely.
Can’t wait for even closer photos
How come that large hole/crater in ‘front’ of the ‘head’ is never shown in recent images?
The crater on the head was shown is quite some detail in the following, particularly the last one.
https://blogs.esa.int/rosetta/2014/08/15/cometwatch-14-august/
https://blogs.esa.int/rosetta/2014/08/18/cometwatch-17-august/
https://blogs.esa.int/rosetta/2014/08/21/cometwatch-20-august/
You are right.
My bad.
Thanks!
Just announced today that the aforementioned crater is one of the potential landing sites for Philae. Not surprised as that being a possibility.
https://www.esa.int/spaceinimages/Images/2014/08/Candidate_landing_site_B
Are you testing the gravitational force at different points of the comet? The comet has such a peanut shape that it will be interesting if there is less gravity at say the thin middle area compared to the long ends. Adversely if the gravitational force is the same in any circumference then this will also be remarkable.
Thank you very much for taking time out of your weekend to provide this update for us Claudia.
The layering on the larger lobe is interesting as are the striations on the ‘chin’ of the head.
Boulders are found near enough everywhere despite terrain types.
Will be interesting to see the five finalists for the Philae landing site tomorrow.
Maybe the black surface is polymerised hydrocarbons. With heat from the sun and the sublimation of sulfur, the polymer would then be vulcanized. How ironic would it be if the rubber ducky had a skin of vulcanized rubber?
I’m getting excited. My kid brother, Dale Miller of DMC ground the elliptical antenna on the space station that will receive the data from the lander on the comet. Unfortunately, Dale didn’t live to see it happen. We were following the events of the space craft from launching and I still follow it. Jet Propulsion Laboratory said that Gale’s antenna was the 1st item in the istory of JPL that was perfect right out of the box and needed no revisions. I’m very proud of Dale’s accomplishments attained on only a High school education. DMC is the leading Jig Grinding company in the world and can gring to 1 millionths tolerance.
Why are we looking at still images in stead of videos?
There is no video camera on board Rosetta, but you can put images together to make nice sequences, for example: https://www.esa.int/spaceinimages/Images/2014/08/NavCam_animation_6_August
These CometWatch NavCam images are great, especially now when distance to comets nucleus is getting smaller.
But you haven’t posted any new image since August 22.
Will there be more daily images???
Hi Paja, the way in which the daily images are taken has changed – please see this post for more information: https://blogs.esa.int/rosetta/2014/08/27/cometwatch-update/
¿ Si tan poca gravedad tiene porque hay un argayo en el pescuezo del corío ?.
Un saludo desde ASTURIES
This mission is so cool. I have not been this excited since the Viking landers on Mars. I read that the gravity on the surface was something like 1/10,000 that of earth. Escape velocity is less than .5m/s , so if you were on the surface and you jumped, would you go into orbit? It looks like from the “highlands” looking down into the valley isthmus would be around a mile or more. I hope this all goes well, this is all very super cool sci/fi for real. I can’t wait to see the out gassing as it happens. Well done to all the team working on this.
This is simply the bigggest Champagne Cork in the galaxy.