According to the BBC Dawn has sent back signals confirming it's in orbit:
Probe orbits asteroid Vesta
According to the BBC Dawn has sent back signals confirming it's in orbit:
Probe orbits asteroid Vesta
Dawn herself confirms
http://twitter.com/#!/NASA_Dawn
!
I've been following the progress of Dawn since launch. I get all the emails from the Dawn mission site, so I was very happy to hear that Dawn had entered orbit around Vesta successfully!
I'm looking forward to seeing the great images we can expect shortly as Dawn lowers its orbit.![]()
Nice image released today. Phil has a blog entry about it here.
Emily has been strangely silent about it (the approach and entry in to orbit), even though she's been back from vacation. I expect she'll have a rather nice write-up when she gets to it, though!
CJSF
Last edited by CJSF; 2011-Jul-18 at 09:10 PM.
"In the nightgown of the sullen moon, How the windows lean into the room, In the nightgown of the sullen moon."
-They Might Be Giants
Seems I was right. Here's Emily's Planetary Society blog entry.
CJSF
"In the nightgown of the sullen moon, How the windows lean into the room, In the nightgown of the sullen moon."
-They Might Be Giants
So, what's the data on surface composition?
They just achieved orbit 2 days ago. I suspect they haven't even started collecting that data yet, let alone transmit it to Earth, process it, and then do the human analysis. This is a year long mission (at least), they are not going to do everything in the first three days.
Order of Kilopi
Big article with new images from orbit:
http://www.nasa.gov/mission_pages/da...20110718.html#
How come all the images appear a bit blurry? They're not as crisp and detailed as I was hoping they'd be at this point.
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From the UT article:
“We will not have a steady stream of images until we are in one of our three science phases,”
... “When we are in transit from one place to another we thrust, stop, turn, image, turn, transmit, turn, thrust, and several days later repeat. All time spent not thrusting is time taken away from science later.”
[Prof. Chris Russll, Dawn’s Science Principal Investigator of UCLA]
STARGAZING: All I see are the lights of a billion places I'll never go. --Howard Tayler, Schlock Mercenary
Some more details from this R&D Magazine on-line article:
Although orbit capture is complete, the approach phase will continue for about three weeks. During approach, the Dawn team will continue a search for possible moons around the asteroid; obtain more images for navigation; observe Vesta's physical properties; and obtain calibration data.
In addition, navigators will measure the strength of Vesta's gravitational tug on the spacecraft to compute the asteroid's mass with much greater accuracy than has been previously available. That will allow them to refine the time of orbit insertion.
Dawn will spend one year orbiting Vesta, then travel to a second destination, the dwarf planet Ceres, arriving in February 2015. The mission to Vesta and Ceres is managed by JPL for the agency's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, which is managed by NASA's Marshall Space Flight Center in Huntsville, Ala.
New photo taken July 18th, released yesterday.
http://dawn.jpl.nasa.gov/feature_sto...back_photo.asp
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She has explained that is likely because the other satellite's have a high ice content, which deforms easier.
CJSF
"In the nightgown of the sullen moon, How the windows lean into the room, In the nightgown of the sullen moon."
-They Might Be Giants
That ice/rock thing puts the whole "dwarf planet" thing into question.
You mean the hydrostatic equilibrium part of the definition? It's true that a lumpy, misshapen rocky object can be much heavier than an icy one that's formed itself into a sphere, but it's not like there's any particular mass you can draw a line at. In this case, it seems likely that Vesta was big enough to pull itself into a sphere, its current condition being a result of impacts after it had completely solidified.
Fascinating pictures from the spacecraft so far, I eagerly await the rest of the photographs.
Would Vesta look different in color, or would it be more or less a colorless lump of rock like the Moon? I ask because this fuzzy picture of Ceres looks tantalizingly colorful.
The collision that created the big crater at the south pole did not heat up the planet sufficiently to restore hydrostatic equilibrium even temporarily. My intuition says that it should have, so obviously I need to recalibrate my intuition...
At any rate, is it possible with the instruments on Dawn to get an idea of what latitude the collision actually happened at? It's very unlikely to have happened exactly at the south pole, and if it happened elsewhere, forces would tend to tilt the planet until the crater was centered on the nearest pole, since that's the minimal energy state.
Assuming Vesta had a magnetic field in its early days, there should be magnetic grains in the rocks that would show the orientation of the field at the time the rocks cooled. But that would require measuring the rocks in situ, which Dawn is incapable of. So any ideas based on what instruments Dawn has?
In terms of scientific discoveries, I would assume that the observations of Dawn's orbit around Vesta will tell a lot about density, mass distribution and the like.
^
I'm guessing a magnetometer was very high on the team's wish list (it could also clinch the existence of a ionic mantle in Ceres), but was probably excluded partly for cost, and perhaps (though I'm no expert) possible interference from the ion drive with any readings.
The magnetometer was removed as a cost-cutting measure to prevent it from staying cancelled, IIRC.
New image from Dawn:
http://dawn.jpl.nasa.gov/multimedia/...age_072311.asp