Phil Stooke
Aug 1 2011, 04:04 PM
elakdawalla
Aug 1 2011, 04:07 PM
Cool rotation movie!! What a cool mini-planet!
http://www.nasa.gov/multimedia/videogaller...ia_id=104094441I am at JPL now so ironically I can't do my usual quick image processing magic. I will plan to decompose this movie into separate frames and also make an animates GIF later today -- but would be very happy if someone else beat me to it!
Phil Stooke
Aug 1 2011, 04:15 PM
The map is at the Photojournal now.
Phil
ugordan
Aug 1 2011, 04:25 PM
Whoa, groovy!
Explorer1
Aug 1 2011, 04:27 PM
False color... interesting splashes.
Juramike
Aug 1 2011, 04:57 PM
Well, now we know what the image release policy is going to be in the future...like MESSENGER with a selected processed image of the day.
(But no raw images like MER or Cassini). Ah well.
Explorer1
Aug 1 2011, 04:58 PM
There will still be PDS releases, right?
ugordan
Aug 1 2011, 04:58 PM
This image nicely showcases the equatorial grooves as well as curious dark spots in the dark hemisphere. I wonder what they're all about. Almost look like ejecta spray, but clumpy and more sporadic.
Juramike
Aug 1 2011, 04:58 PM
ugordan
Aug 1 2011, 04:59 PM
QUOTE (Explorer1 @ Aug 1 2011, 06:58 PM)
There will still be PDS releases, right?
Yes. I think that's pretty much mandatory for a U.S. mission. Not sure how it will play out with foreign instruments, but I wouldn't expect problems in this case.
MarkG
Aug 1 2011, 05:12 PM
Anyone know where/when the recording of the press conference will be available?
hendric
Aug 1 2011, 05:27 PM
Missed the press conference. Is this a close-up of a potential lava flow? (the darker area in the top right)
http://www.nasa.gov/mission_pages/dawn/mul...a/pia14324.html
volcanopele
Aug 1 2011, 05:30 PM
One major thought I had coming out of the presser was on the comments regarding the formation of the grooves. Now, Chris Russell stated that one idea is that the grooves formed shortly after the SP impact when Vesta was initially compressed in the N-S direction and then rebounded, forming grooves at the equator. But I think there is another possibility: Upspinning. It is possible that the impact sped up Vesta's rotation. Upspinning would cause the equatorial radius to expand and the polar radius to contract, resulting in extension at the equator and compression at the mid- to high-latitudes. Similar upspin/despin/re-orientation scenarios have been discussed for Iapetus (despinning to explain equatorial ridge) and Enceladus (upspinning and polar wander to explain south polar boundary, equatorial fractures, etc.)
john_s
Aug 1 2011, 05:36 PM
Complicating the picture is the possibility that the impact also changed the pole orientation, which may be quite likely as the missing mass associated with the impact crater is now aligned with the spin axis (shades of Enceladus again). A changed spin axis would produce stresses comparable to a spin-up or spin-down about the existing axis.
Excuse me if this was discussed at the press conference, which I missed...
John
siravan
Aug 1 2011, 06:03 PM
In the Enceladus case, change of the axis of rotation can be explained based on polhode phenomenon. But that needs an energy dissipation mechanism, which for Enceladus is based on the tidal lock (as also the possible 'ocean'). But for a free solid body like Vesta, what is the dissipation mechanism?
tasp
Aug 1 2011, 06:46 PM
My first thought about the cracks was we are seeing crustal sloughing into the crater hole. (it's big, for sure, but technically, the missing segment of Vesta is a hole) The tensile strength of the materials surrounding the crater would need to be checked for consistency this idea. Also, the segments between the cracks would be subject to compressive effects as the assemblage creeped (oozed? shifted?) downslope. Not sure I see anything that might be like that at this resolution in the images.
john_s
Aug 1 2011, 07:34 PM
QUOTE (siravan @ Aug 1 2011, 12:03 PM)
In the Enceladus case, change of the axis of rotation can be explained based on polhode phenomenon. But that needs an energy dissipation mechanism, which for Enceladus is based on the tidal lock (as also the possible 'ocean'). But for a free solid body like Vesta, what is the dissipation mechanism?
Large Vesta-sized bodies will settle fairly quickly into stable rotation about the minimum moment of inertia after their rotation is perturbed, due to internal frictional dissipation - tumbling will produce internal stresses that will cause motion along fractures, etc., that will dissipate energy and damp out the tumbling (Burns and Safronov 1973).
John
t_oner
Aug 1 2011, 07:54 PM
Here is a quick smoothing of the rotation clip. I had to compress a lot it due to 1 MB limit.
machi
Aug 1 2011, 08:30 PM
Excellent!
Beautiful rotation
Phil Stooke
Aug 1 2011, 08:36 PM
The color image is up on the photojournal now.
Phil
http://photojournal.jpl.nasa.gov/catalog/PIA14325PS before getting too carried away with explanations of grooves, let's consider the other grooved bodies - will the explanation work more generally?
jasedm
Aug 1 2011, 08:49 PM
Composed of completely different stuff I know, but it looks remarkably Miranda-esque to me
antipode
Aug 1 2011, 09:18 PM
The crater count looks low over the impact area - I guess that makes sense, what is it - a billion years old?
Seems to be several sites of mass wasting/downslope movement. And those dark areas are fascinating!
Very very rugged, very very cool. Might be a good place for a lightweight instrumented penetrator (if we ever visit again!)!
Although Ceres is the main course, this is a fantastic entree...
P
ugordan
Aug 1 2011, 09:22 PM
QUOTE (Tayfun Öner @ Aug 1 2011, 09:54 PM)
Here is a quick smoothing of the rotation clip.
Very nice!
nprev
Aug 1 2011, 11:23 PM
Fantastic, Tayfun!!!
Man...there's a LOT of interesting features on this little world!
elakdawalla
Aug 1 2011, 11:30 PM
QUOTE (Explorer1 @ Aug 1 2011, 09:58 AM)
There will still be PDS releases, right?
It may be a long wait. I asked about this after the press briefing, and Marc thought that the PDS timeline was 6 months....AFTER they leave Vesta.
In the meantime, I have now decomposed the high-resolution version of the animation into its component frames. Here you go, guys; have fun.
http://planetary.s3.amazonaws.com/misc/Vesta_rotating.zip
volcanopele
Aug 1 2011, 11:39 PM
Lol, I got to about frame28 before I noticed your message. Oh well. I will work up a few anaglyphs if and when I find my red-blue glasses. I know it is here somewhere.
nprev
Aug 2 2011, 12:40 AM
Mrs. nprev's comment on the movie:
"Huh. Looks like biscuit. Even has lines around the middle like biscuit!"
, but insightful. The grooves sure look like compressional features to me from the south polar impact.
MarkG
Aug 2 2011, 01:04 AM
What can make a series of long, straight grooves along the equator of an isolated self-gravitating body?
Debris collapse into extension cracks is one possibility. But what would cause straight cracks at the thickest part of the body?
In the South Pole impact, as the debris was blasting away, the center of mass of Vesta became shifted towards its North Pole, and the area around the crater rim became very high ground. The result static force on the equatorial region would have been compressive.
However, the dynamic situation would have been different. In solids, compression waves travel faster than shear waves, and the bulk (2/3) of the momentum transfer (apart from vaporization heating) from the impact would be transferred by the shear waves, especially an angular momentum change.
With Vesta getting its bell rung so hard, the equator could have been the mega null/shear zone between torsional resonance modes. With debris falling on/in/around the cracks and partially filling them, we could end up with the current distribution.
With limited information coming from Dawn, they'll just have to put up with theories from the bleachers (cheap seats for the Brits).
Phil Stooke
Aug 2 2011, 01:45 AM
Despite the Dawn team wanting this to be a very primitive body dating back to the Dawn of the solar system, there's no particular reason why it could not have been larger at a very early date and to have lost a lot of mass though large impacts to become what we see today. I only suggest this to say that the grooves may be explained by events whose records are no longer visible to us. It's like Phobos - everybody wanted the grooves to be the result of Stickney despite the fact they have no geometric relationship to it at all. At least we can lay the old story of Mars ejecta to rest at last!
Phil
Gladstoner
Aug 2 2011, 01:58 AM
Wow. It looks like baling wire is holding the asteroid together....
It never ceases to amaze me how new types of features keep showing up on these newly explored worlds.
Speaking of new features, this little image artifact
Click to view attachment looks a lot like Tsiolkovskiy on the moon:
Click to view attachment
Juramike
Aug 2 2011, 03:12 AM
Mashup of 3 images: full frame image coordinated to global mosaic, overlain by a warped false color view of IR data (?) PIA14325:
Click to view attachmentFull resolution on flickr:
http://www.flickr.com/photos/31678681@N07/6000679166/
Decepticon
Aug 2 2011, 03:17 AM
Gladstoner you read my mind.
I can't wait to see close ups of that crater.
elakdawalla
Aug 2 2011, 03:27 AM
I was excited when I first saw that too until I decomposed the animation and realized that it is in fact an artifact -- a bit of dust somewhere or something. Here's a teeny window on that little "Tsiolkovskiy" -- it doesn't move as Vesta rotates beneath it. There's a few other black specks that don't move from frame to frame.
Gladstoner
Aug 2 2011, 04:37 AM
Heh, I suppose the group of blemishes can be used to calibrate the cropped and blown-up images that are released to the media.
pablogm1024
Aug 2 2011, 06:11 AM
QUOTE (Gladstoner @ Aug 2 2011, 05:37 AM)
Heh, I suppose the group of blemishes can be used to calibrate the cropped and blown-up images that are released to the media.
Man, you are really crafty!!!
Lewis007
Aug 2 2011, 06:36 AM
Decepticon
Aug 2 2011, 06:44 AM
I shall call it the "Tsiolkovskiy Artifact"
Gladstoner
Aug 2 2011, 08:06 AM
And the next two largest specks can be "Grimaldi" and "Plato".
Stefan
Aug 2 2011, 09:32 AM
QUOTE (elakdawalla @ Aug 2 2011, 05:27 AM)
I was excited when I first saw that too until I decomposed the animation and realized that it is in fact an artifact -- a bit of dust somewhere or something. Here's a teeny window on that little "Tsiolkovskiy" -- it doesn't move as Vesta rotates beneath it. There's a few other black specks that don't move from frame to frame.
These are indeed artifacts present in the raw image. We can correct for most of them by using a flat field.
bk_2
Aug 2 2011, 09:44 AM
QUOTE (Phil Stooke @ Aug 1 2011, 09:36 PM)
PS before getting too carried away with explanations of grooves, let's consider the other grooved bodies - will the explanation work more generally?
It won't work on Phobos, since the grooves on that body tail off on the trailing hemisphere.
It will be interesting to see the extent of these grooves on Vesta.
PDP8E
Aug 2 2011, 01:26 PM
Here is a little article from the AP about Vesta
http://news.yahoo.com/scientists-stunned-s...-204550456.htmlthe last line has a 20th century kinda of feel to it:
....The team does not plan to post raw images online as other NASA missions have done. Instead, there will be just one picture released daily ....
elakdawalla
Aug 2 2011, 01:27 PM
QUOTE (pablogm1024 @ Aug 1 2011, 10:11 PM)
Man, you are really crafty!!!
Pablo, this community is nothing if not crafty.
QUOTE (PDP8E @ Aug 2 2011, 05:26 AM)
the last line has a 20th century kinda of feel to it:
....The team does not plan to post raw images online as other NASA missions have done. Instead, there will be just one picture released daily ....
I was very happy when Alicia (who has, several times, been nearly the only reporter besides me present onsite at Von Karman for a press briefing) asked that question, because I figured I'd worn out my welcome with such questions.
QUOTE (elakdawalla @ Aug 2 2011, 02:27 PM)
I was very happy when Alicia (who has, several times, been nearly the only reporter besides me present onsite at Von Karman for a press briefing) asked that question, because I figured I'd worn out my welcome with such questions.
Don't worry about it Emily, I think we're just going to have to accept that we're not going to make the mission's Powers That Be change their minds. It's a great shame, but it seems that, unlike the MER team for example, some of them just don't get how much they're going to miss out on having a hugely-enthusiastic community of space enthusiasts and image manipulators on their side, working with their raw images to create exciting new products that would benefit them. I think it's a huge, huge mistake, I really do, and jaw-droppingly short-sighted in this modern age of data sharing and "citizen science" when we're all encouraged to be part of the space missions we follow so devoutly. I don't "feel a part of" DAWN, I feel like I've been told I can watch what's going on but only if I go stand over there, out of the way, and don't make a nuisance of myself.
I'm hugely supportive of the mission, and very grateful for every image we have been shown, but oh, it could be so,
so much better than this. Oh well. Roll on MSL!
Explorer1
Aug 2 2011, 04:18 PM
Don't give up; they may very well change their minds for Ceres.
alan
Aug 2 2011, 04:25 PM
I was hoping for some numbers (dimensions, mass, density) at the press conference to compare with the previous estimates based on very distant observations. Guess we'll have to wait awhile longer for those.
dshaffer
Aug 2 2011, 04:27 PM
QUOTE (elakdawalla @ Aug 2 2011, 09:27 AM)
Pablo, this community is nothing if not crafty.
I was very happy when Alicia (who has, several times, been nearly the only reporter besides me present onsite at Von Karman for a press briefing) asked that question, because I figured I'd worn out my welcome with such questions.
IIRC, the question was whether all raw images will be made available as they were received (like MER), but was there a follow-up question as to why not?
hendric
Aug 2 2011, 05:03 PM
Any chance of showing Tayfun Oner's wonderful smoothing of the rotation movie to the Powers That Be? They could be getting stuff like this done *for free* by UMSF.
algorimancer
Aug 2 2011, 06:23 PM
QUOTE (dshaffer @ Aug 2 2011, 10:27 AM)
...why not?
If these were politicians getting out of line then we, as citizens, would have the option of not re-electing them next time around (this happened in my county a few years ago). In the case of mission PI's, I suppose an equivalent option would be to advocate appropriately to our elected representatives when the next round of mission funding occurs. Not all missions are going to get funded, so we can at least see about ensuring that the ones that
do have an immediate data-release policy in place. For that matter, this mission will presumably be seeking a post-Ceres extension....
stevesliva
Aug 2 2011, 06:40 PM
It's an orbital mission. Do the ones in orbit around the moon, mars, and mercury release everything immediately?
climber
Aug 2 2011, 06:42 PM
QUOTE (stevesliva @ Aug 2 2011, 08:40 PM)
It's an orbital mission. Do the ones in orbit around the moon, mars, and mercury release everything immediately?
Cassini?
This is a "lo-fi" version of our main content. To view the full version with more information, formatting and images, please
click here.