http://www.jpl.nasa.gov/news/news.php?release=2014-244&utm_source=iContact&utm_medium=email&utm_campaign=NASAJPL&utm_content=comet20140725 from NASA mentions this possible future observation for the rovers:
"...Rover cameras may be used to observe the comet [Siding Spring] before the flyby, and to monitor the atmosphere for meteors while the comet's dust trail is closest to the planet..."
What are the chances that Deimos or Phobos could get in the shot along with the comet? That would be extraordinarily cool!
Here is at leased one Opportunity. This one is at 4:06:27 UTC Local Mars Time. on Oct 19. I'm sure there are probably many more opportunity's as well. I'm sure Starry Night isn't that accurate when rendering the approximate tail, coma size and brightness of the comet, but roughly
https://flic.kr/p/ot44eM
By the way, I'd advise these two posts and further discussions on the comet be moved to the astronomical observations thread.
Great work, James, and thanks for pointing this out. Hopefully any MER project people who pop in here will take note!
Per your suggestion, this thread will be for observations of this event regardless of the source.
Deimos and Siding Spring on Oct 18 at 00:28 UTC
from Gale
http://www.imagebam.com/image/c707d7341133252
Phobos Oct 18 13:30UTC
http://www.imagebam.com/image/3bef3f341133934
on the 19'th Phobos rises into the tail
http://www.imagebam.com/image/533796341134230
Nice, John!
I've been looking for magnitude estimates during closest approach with no luck. Understand that this is often a matter of guesswork for comets anyhow, but I calculated around mag -3 from Mars for the coma. Hopefully the tail will be at least that bright per a given unit of area; should be quite a show!
the comet tail above is 100% guessing
that and there is no real good way , right now, to use a real value in celestia
( the tails NEED some recoding in c++ and opengl )
and look at the last comet ( ison)
it was supposed to be GREAT!!!!, and HUGE!!!! ,and mind blowing !!!
then fizzled out on thanksgiving day
Well, yeah; think that an astronomer once said something like they're 'as unpredictable as cats'. I used what looked to be a middle-of-the-road activity index, and given the extremely close periapsis hoping that -3 is a conservative estimate. Still, we'll have to wait & find out.
Also great work John . I agree. It's all guess work with regard to the brightness and how big the comets tail will be. looks like at the time of closest approach, the comet will be below the horizon for Curiosity and Opportunity could be set up to image it. It will be daylight then as well for Oppy. The hours and nights before and after closest approach all look like great imaging opportunity's. At the time of that photo opportunity that I noted, SN gives an estimated -1.07 apparent mag. For Oppy it will be early morning after sunrise at closest approach, SN gives an estimated apparent mag of -8.00. I'd take this figure with a grain of salt and agree with you of a -3.00 or maybe less. I sure hope we are both wrong.
No topic like this is complete without a word of caution
During the morning before closest approach CA (for MER) and the evening after (MSL), the coma is comparable in size to the camera FOV. So the magnitude -5 comet is spread over a million pixels. That's a 15 magnitude downer, if the brightness were uniformly distributed--though it is not. JPL's horizons tool is currently saying around -5 for CA, and the comet has been running sightly brighter than that prediction (as seen from Earth). But the bigger and more impressive it looks in Starry Night, the harder it will be to see anything. Navcam is ~20x less sensitive than MCAM RGB (or Pancam L1 or MAHLI), so wide-field images are not simple. The comet is an AM object inbound, and a PM object outbound. I think people on this forum are familiar with the energy problems associated with the AM side, especially for Opportunity, which would need to skip deep sleep.
That said, various photo ops have been identified, but of course all plans are subject to the tactical operations context at the time--and the dust storm conditions (L_s=218, yikes). But figure the nucleus itself is within a factor of a couple of the size of Deimos, and the comet is maybe 20x further away. So there should be something to see, whether the comet is especially active or not.
Also, of course, cameras in orbit are free of many of the rover's constraints.
The Minor Planet Center
http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=c&o=CK13A010
and
Visual Comets in the Future
http://www.aerith.net/comet/future-n.html
predict about magnitude +8 1/2, as seen from Earth, about the time of closest approach to Mars. Not that our view has much to do with the ability to see the comet from Mars.
I only say this because it would be cool to have Mars and the comet together in the telescope eyepiece and be able to say 'they are actually near each other in space, not just in the sky!' at our monthly star party in October. That's often not the case as you can see with the pairing of planets, and our Moon and stars in August.
Good luck to observers on Earth and on and near Mars!!! It's going be very exciting to see what we can see.
and on the inbound leg the optics WILL be pointed AWAY from the incoming DUST ( moving at 25,000 KPH )
now on the outbound leg , that is very different
They have shown they can deal with that for the Phoenix and MSL parachute descent images, so this should be well within their capabilities. Should be fascinating.
Phil
Will MEX's VMC be sensitive an wide angle enough to show both Mars and the comet?
They captured Earth two days ago with a 2-30 seconds exposures, so maybe they can expose separatedly to capture the coma and Mars; or if not, just do it when MEX is on Mars' night-side.
http://mars.jpl.nasa.gov/msl/news/whatsnew/index.cfm?FuseAction=ShowNews&NewsID=1723
Not a hard seartch to do....finding this took less time than typing it up.
http://lmgtfy.com/?q=mro+siding+spring
Third hit
http://cometcampaign.org/files/docs/session_4/Tamppari_CSS_CIOC_v3.pdf
Mars Reconnaissance Orbiter Observation Plan for Comet Siding Spring Encounter
Page 5 of which states....
Basically, we can expect something more like the radar pictures of 2012 DA14 last year than what we've gotten from close flybys. An identifiable shape, but not much else. Plenty of science can come from that alone.
T-minus 1 week....
I've been searching off & on for a couple of hours but no luck. Anybody know if there's a tau prediction for encounter time for each of the rovers yet? I hear that there are some pretty good localized sandstorms happening mostly in the southern hemisphere, dunno if any of those are expected to blow up into regional events that might affect surface observations on C-sol.
Earth-based observers have reported regional dust storms. This is seen at Opportunity's site as optical depths >1; the norm has been around 0.8 according to the MER weather page (http://www.lpl.arizona.edu/~lemmon/mars-tau-b.html). At the 8th Mars conference I saw that, as of that time, MSL and Opportunity optical depths had tracked each other fairly closely. This is pretty close to a time of year when larger (and sometimes much larger) dust storms can emerge.
Today's release is a ChemCam Siding-Spring imaging test : the scientists were to try Chemcam on Sirius (that can be observed in October before sunrise) and on Canopus (that can be observed for 4 hours before sunrise from August to September and which is low on the horizon)... But also at Archenar and at Spica... Do you know which stars they were pointing at ? Enjoy
http://mars.jpl.nasa.gov/msl/multimedia/raw/?s=777&camera=CHEMCAM_
http://astrogeology.usgs.gov/news/astrogeology/sol-775-777-update-on-curiosity-from-usgs-scientist-ken-herkenhoff-weekend-planning.
Trying to figure out a way to best show the viewing situation on sol 783, the sol of the closest approach, here's a cut at it:
With an albedo of 0.04, a distance of 139,500 km from Mars, a diameter of 0.7 km, and a distance of 1.5 a.u. from the Sun as model assumptions, I get an apparent visual magnitude estimate for the nucleus during closest approach of about 5.6 m:
VisualMagnitudeEstimate.pdf ( 41K )
: 596
For a distance of 1 million kilometers, the magnitude is 2.14 m fainter, hence about 7.8 m with the other assumptions kept the same.
Some Wikipedia links for the notions used:
http://en.wikipedia.org/wiki/Albedo, http://en.wikipedia.org/wiki/Solid_angle, http://en.wikipedia.org/wiki/Magnitude_(astronomy), http://en.wikipedia.org/wiki/Right_triangle, http://en.wikipedia.org/wiki/Moon.
OK, had to hack that together real quick, hope this is right for Oppy's view of the comet:
for any that want to run the sim and do not already know about this
http://forum.celestialmatters.org/viewtopic.php?f=18&t=578#p10789
i posted a celestia NAIF-spice add on for siding spring
using the HORIZONS database to make the position kernel
( i can not post images at this time - software error do to building VisionWorkbench and StereoPipline )
--- edited later -----
software fixed
Oct 19 at 18:27 UT
[attachment=33988:marsrise.jpg] [attachment=33989:marsrise1.jpg] [attachment=33990:ssm.jpg]
Mars Express with be using the super resolution channel of the high resolution stereo camera to catch any meteor activity from coma particles:
According to the http://astrogeology.usgs.gov/news/astrogeology/sol-781-update-on-curiosity-from-usgs-scientist-ken-herkenhoff-dumping-sample they'll be trying to image SS on sol 782 as well, the day before closest approach. Here's the viewing situation per http://naif.jpl.nasa.gov/pub/naif/generic_kernels/spk/comets/siding_spring_8-19-14.bsp
https://www.youtube.com/watch?v=9o348MOuu-c
View to Mars, spacecrafts (MRO, Mars Odyssey, Mars Express, MAVEN) rovers (MER-B Opportunity and Curiosity) from comet C/2013 A1
Comet will pass very close to Mars at 18:27:15 UTC (about 135 300 km to planet surface). I have stop for few seconds animation at that time.
At 18:48 UTC Mars will enter path of the comet dust trail
At 20:05 UTC Mars will be at center of the dust trail. Mars Express will try observe meteors on Mars atmosphere
The animation show view from above the comet.
Simple law - comet see the spacecraft = spacecraft see the comet !
About rovers:
Opportunity will see the comet at night to the set comet at morning (18:35 UTC - 10 min after CA)
In the Curiosity sky comet will rise at the daytime and transit at 20:39 UTC (after dusk sky)
This two rovers will have good conditions to see the comet.
Animation are made in Celestia and orbital data are from SPICE/BSP (NAIF/NASA site http://naif.jpl.nasa.gov/pub/naif )
Precision are compared with HORIZONS/JPL ephemerides and ORB files in spk folders.
Nice animation--good to see all the players at once, except the Indian orbiter, which doesn't use SPICE, unfortunately.
I was going by this from a http://naif.pds.nasa.gov/naif/SPICE_News_August_2013.pdf from last year:
I think the new 781 mastcam observations are the first of the SS field. All I could see is a faint trail on one of the frames, in the lower-left quadrant:
It's probably http://en.wikipedia.org/wiki/Pi_Eridani, sorry meant http://en.wikipedia.org/wiki/Pi_Ceti, just outside Eridanus. There may be some more stars hidden in the noise. The pointing is good, but I couldn't identify the comet thus far. I'll try to identify the star(s), and edit this post later with more stars identified, if possible.
Here an excessively processed and tentatively annotated version of the Sol 781 Pi Ceti image:
i think the issue is that there are no naif ck and spk folders for "mom "
like there is for, say Cassini.
ftp://naif.jpl.nasa.gov/pub/naif/CASSINI/kernels/ck/
ftp://naif.jpl.nasa.gov/pub/naif/CASSINI/kernels/spk/
but the data in horizons is current just in a different form
I know that. But it's still SPICE that's driving HORIZONS. The same SPICE driving 'Eyes..' and telling the DSN where to point.
Opportunity also imaged Pi Ceti during a test run a few sols ago. In addition to increased extinction, the distant dust storms make for an annoyingly bright twilight. http://mars.nasa.gov/mer/gallery/all/1/p/3812/1P466564406EFFCHYOP2664L1M1.JPG
Haven't seen this posted yet. Emily has a nice summary of real-time telescopic webcasts & other resources in her most recent http://www.planetary.org/blogs/emily-lakdawalla/2014/10171350-watching-siding-springs.html.
There are rather impressive Sol 782 night shots. Here a brightness-stretched and denoised ML image:
I think the sol 782 images taken around 4:08am, elevation 70 degrees, azimuth 100 degrees are the ones with SS in frame, if visible, e.g.,
http://mars.jpl.nasa.gov/msl-raw-images/msss/00782/mcam/0782MR0033730040404149C00_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00782/mcam/0782MR0033730030404148C00_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00782/mcam/0782ML0033730050400344C00_DXXX.jpg
Based on the ML shots, seems there was quite a bit of sky brightness in the east around 4:10am, a little over an hour before sunrise:
http://curiosityrover.com/synth/?camera=ML&station=246
A preliminary stitch of three of the Sol 782 ML images:
http://imgur.com/bUzmuCeThe shape of the comet begins to become more apparent. (Wishful thinking, see next post.)
Sorry if I sounds like an orbital mechanics rookie, but what are the closest approach distances of the 5 Mars orbiters to the comet?
As Joe said, the comet was up at 70 deg when the twilight images happened. The sky was brighter than any comet has ever been at 1.5 AU from the Sun.
The latest predictions (i.e., what I see in Starry Night - 2 magnitudes, per http://cometcampaign.org/current-status) suggest the comet may total 100X as bright as M31, outside of twilight, at a time when its coma has >5X the angular extent: so the light is diluted to <20X M31. If you've seen previous attempts to image M31 (http://www.unmannedspaceflight.com/index.php?s=&showtopic=7238&view=findpost&p=185599 and http://www.unmannedspaceflight.com/index.php?s=&showtopic=7730&view=findpost&p=203306) in less dusty conditions, then you have an appropriate sense of how bright the comet may appear.
Opportunity's night is done, but it is a long wait for a relay pass. Curiosity should get to work soon, but again it will be a long wait.
Thanks very much for the update, Deimos.
I've seen unconfirmed reports that the coma is greater in extent than anticipated (though no means for determining that was specified; presuming it was via Earth-based telescopes, but I'd think that the glare from Mars would complicate that). Does anyone have any reliable information regarding this, or anything else of interest for that matter?
EDIT: Found a http://mars.nasa.gov/comets/sidingspring/ for US orbiter status post-passage. Not particularly informative at the moment; all statuses are 'pending'.
Just to shuffle these numbers a bit, current magnitude would be about 11.5 from Earth, translating to -4.7 from Mars at closest approach. If M31 is 3.5 magnitude, then SS is about 2000 times as bright. If SS has 5 times the angular diameter as M31, then the areal extent is 25x. Thus the surface brightness would be 80x that of M31.
Seen from Earth, an image 8hrs before closest approach from comets-ml is here where it looks pretty well condensed in an area smaller than 1 arcminute, with the overall coma being around 1 arcminute: http://www.dpreview.com/galleries/4594584079/photos/3051425/comet-c-2013-a1-approaching-mars?inalbum=comets
Via Twitter today is this pretty neat color image: http://cf.tzecmaun.org/2014/10/mars-and-comet-c2013-a1-siding-spring/
An Oct 17th visual description is here: https://groups.yahoo.com/neo/groups/CometObs/conversations/topics/5852
According to DSN Now everything went well Maven, MRO, Mars Express, and Odyssey. Communications going on just fine...
As expected. It'll be interesting to see if there have been any effects at all on any of the spacecraft.
http://mars.nasa.gov/news/whatsnew/index.cfm?FuseAction=ShowNews&NewsID=1734 MRO's fine & successfully maneuvered for all planned observations.
some sim images
Comet rise then set for Curiosity
rise at about 14:20 UT , then set will be at about 22:30
http://imgbox.com/DwYXFwLt http://imgbox.com/MfP5h27r
https://plus.google.com/u/0/photos/102695901291398562941/albums/6072078138374025457/6072078141990992834?pid=6072078141990992834&oid=102695901291398562941
https://plus.google.com/u/0/photos/102695901291398562941/albums/6072078138374025457/6072078145988026242?pid=6072078145988026242&oid=102695901291398562941
for Opportunity
Comet rise as of a few min. ago 20:25 and it will set at about 7:00 UT Oct.20
http://imgbox.com/p6jk4S5D http://imgbox.com/2t0vMaH5
https://plus.google.com/u/0/photos/102695901291398562941/albums/6072078138374025457/6072078145374466034?pid=6072078145374466034&oid=102695901291398562941
https://plus.google.com/u/0/photos/102695901291398562941/albums/6072078138374025457/6072078153065408226?pid=6072078153065408226&oid=102695901291398562941
image folder
https://plus.google.com/u/0/photos/102695901291398562941/albums/6072078138374025457
Using the new HiRise-based solution 101 at Horizons, I got ~1/3 of the way from Pi Cet toward Tau1 Eri as a presumed location.
Yeah, that agrees with Joe's coordinates. I've circled the location with a large circle here:
Just before sunrise, taken around 4:20 AM on Sol782 in an attempt to capture Comet Siding Spring.
EDIT (10/22/2014): I updated the mosaic to further remove the noise in the scene.
https://flic.kr/p/pGxmaQ
Here is comet Siding-Spring spotted by the Opportunity rover in the Martian sky ! (pictures are just de-noised) :
http://qt.exploratorium.edu/mars/opportunity/pancam/2014-10-20/1P467007331EFFCH0HP2665L1M1.JPG
Capture time based on et in the filename is 2014OCT19 16:14:24 UT.
The local time was about 3am. The comet was at maximum elevation (60 degrees), range about 400,000 km. Closest approach (~140,000 km) was a couple hours later, after the comet had set. So this perhaps was the best chance and they nailed it.
An attempt to enhance the Siding Springs comet in the Oppy image:
The structure you're seeing in that extreme zoom is almost entirely jpeg and other noise...
Here's my best shot at the longer exposure. Bandpass up to 4 pix and down to 100 pix, with horizontal stripe suppression, followed by a linear stretch trying not to loose information:
My take at the MC34 mosaic taken at dawn. Noise was removed manually with GIMP for the surface (it was quite a long work) and with a filter for the sky.
https://flic.kr/p/pK46Dn
Here's a similar treatment (bandpass, stretch) on one of the MSL navcam frames. The pointing is not correct yet (the three navcam frames show the same pointing), so I don't know if this was meant to image SS or not (actually I think SS would have been higher than this frame shows). Nevertheless I'll post it in this thread. It shows some clouds near the horizon:
Illustrating my point about the different motions of SS and the stars, a flicker gif between the two (similarly processed) frames.
You can see the 4 or 5 stars rising in the east, but SS moving to the left (north) relative to the stars. This agrees with the SS path for Oppy's sky from Joe.
http://www.midnightplanets.com/web/MSL/sol/00783.html. I didn't see a comet in my first pass through them -- can any of you find it?
http://www.nasa.gov/jpl/mer/nasa-rover-opportunity-views-comet-near-mars/
I tried to look if the Oppy's image shows Siding-Springs' tail but it probably doesn't.
But it shows coma on this denoised image.
Shooting from the hip, I'd guess that az/el is referenced to the camera's boresight with respect to the rover & not Martian true north or the horizon...?
We've seen temporary incorrect coordinates before. They'll hopefully be updated soon.
I see no sign of a tail in the release images, but maybe a hint of elongation away from the sun.
What we've all been waiting for:
http://www.uahirise.org/releases/siding-spring/
The small size gives the 'comets start out bright and turn black with time' hypothesis some validity. From pristine snowball to a lump of coal (though not this one; probably never coming back again after perihelion?)
Accoding to http://astrogeology.usgs.gov/news/astrogeology/sols-785-786-update-on-curiosity-from-usgs-scientist-lauren-edgar-comet-siding-spring
HiRISE got it.
http://www.jpl.nasa.gov/spaceimages/details.php?id=PIA18618
-the other Doug (With my shield, not yet upon it)
ps -- and now I see I was scooped by two hours. Sigh. Gotta get off these painkillers, dammit...
It's alright Doug! I wasn't particularly coherent myself after a wisdom tooth got pulled...
So in terms of image data, all that's left for release is from Mars Express, correct? All the spectra, dust flux, and other non-imagery results from other spacecraft will be at the December conference?
Wasn't MOD looking for shooting stars in Mars' night atmosphere? I haven't seen anything from that, yet, either. (Of course, the raw jpegs might not show a whole lot on this, it might take some real heavy image processing to find those.)
-the other Doug (With my shield, not yet upon it)
This image from Opportunity just showed up from the 19th of October:
Sequence of cleaned and 4x-brightened MSL Sol 783 MastcamLeft images:
Trying my hand at identifying stars in the noise (hats off to those who do this routinely), I think I identified Epsilon Boötis (aka Izar) in http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033840030204197C00_DXXX.jpg and find a potential candidate for Siding Spring:
I'd say these are good candidates for the comet
https://flic.kr/p/oNWLWM
https://flic.kr/p/pKvy3D
Checking it forth and back, I think the streaks (and smaller spots in low-exposure images) are all Izar (Epsilon Boo).
Izar has been well visible in earlier images. All kinds of cleaning, enhancement, registering, stacking I've been trying thus far revealed nothing else than noise, hot pixels and other camera artifacts, and the likely Izar. Things seem to be even more subtle; accurate stacking of the comet position, including rotation - once it's known - may help.
Edit: Identified at least 34 W Boo in http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033780030204181C00_DXXX.jpg:
http://imgur.com/STJrUTu
Playing with the HiRISE images a bit. I was disappointed not to get more pixels across the nucleus (i.e. I hoped they had previously underestimated its size rather than overestimated it) but reality intervenes once more (darn it). Still... I expect a rough shape will be determined from this, and maybe one or more specific active regions will be identified.
Phil
I asked Alfred what the phase angle was, and he said 110 degrees. So there's significant unilluminated comet nucleus in the photo, and coma is bright from forward scattering.
Any body has more information about this picture showing on spaceflightnow?
http://www.spaceflightnow.com/news/n1410/20sidingspring/sidingspring_large.jpg
Q for the better minds here: Was the trajectory of the comet's orbit greatly affected by the Mars encounter?
Like the sunrise sequence that was acquired on Sol-782, this one is another that I'm looking forward to when the full's come down. Here is a thumbnail preview of it just after sunset on Sol-783 during the comet imaging campaign.
https://flic.kr/p/oPjcyG
In the long run:
For an Oort object like C/2013 A1 even a small delta-v as provided by the rudimentary http://en.wikipedia.org/wiki/Gravity_assist makes a difference. In the current case it seems to slow down the comet a little bit, enough to reduce the orbital period down to a fraction (from "several millions years" to about 1 million years, according to http://en.wikipedia.org/wiki/C/2013_A1, which refers to http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2013A1). I'd think, Jupiter will also play some role, but I don't know the respective numbers.
The Sol-783 Sunset mosaic .
Starry Night shows that comet siding spring should be at the very top of the mosaic. I have identified two candidates. There is one faint dot at the very top-left edge of the mosaic which could also be the comet or could also be an artifact or something else...?
https://flic.kr/p/pu5cGK https://flic.kr/p/pLvsqe
Annotated
So any more observations of the comet still to roll in? So far Oppy and the HiRise seem to be the only two that successfully tagged it.
How about ESA/MEX?
Here is the CRISM view:
http://mars.nasa.gov/news/whatsnew/index.cfm?FuseAction=ShowNews&NewsID=1743
Phil
here you go! Siding Spring from the HRSC on MEX
http://dlr.de/dlr/en/desktopdefault.aspx/tabid-10081/151_read-11946/year-all/#/gallery/16991
MSL/Mastcam: http://mars.nasa.gov/comets/sidingspring/images/?ImageID=6725
Very nice! The contrast with the comet in the big banner up top couldn't be more stark though (I'm not blaming the poor intern who had to do it!)
Great! Deimos, what was the 'guide star' (the bright streak)?
That's Izar, and a little fainter at the lower left of Izar, http://en.wikipedia.org/wiki/34_Bo%C3%B6tis.
(Good to know, that I haven't been too far away a few posts above.)
Really good work of the team members, who planned the takes, and those, who brought it out this clear, despite the challenging conditions. Congrats!
Must have taken a lot of massaging, denoising, etc. I looked at the raw images in the timeframe cited (sol783) and don't see much of anything in the JPGs.
It's no way easy, even after a couple of routine cleaning and enhancement steps:
http://imgur.com/d6wiFgQ
Izar is clearly visible after subtracting hot pixels, but then it's going to get increasingly sophisticated.
JPG compression of the available images may be a (poor?) excuse. Fortunately they took some lossless images; not sure, whether it has been much easier with the latter.
If you have dark and bias fields all that noise goes away like magic
Telecon with first results tomorrow morning:
http://www.jpl.nasa.gov/news/news.php?feature=4362
Here's a very quick and dirty attempt at stacking 8 of the press release mastcam images:
Hi all, long time reader and big fan of all the image processing and discussion that goes on in these forums. I haven't yet found a treatment of the following sequence of MSL M100 sub-frames in these forums or elsewhere, and I would love to see what you guys/gals can do with this set. The comet is first visible in 0783MR003377 at row 282, col 565, and scoots toward lower right in successive frames. Forgive me if this sequence has already been discussed.
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033770000204176E01_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033780020204180E01_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033790000204182E01_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033800000204184E01_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033810020204188E01_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033820000204190E01_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033830000204192E01_DXXX.jpg
http://mars.jpl.nasa.gov/msl-raw-images/msss/00783/mcam/0783MR0033840020204196E01_DXXX.jpg
Cheers
-Ryan
Apparently there may have been quite a meteor shower associated with passage of the comet. Unfortunately, the rovers aren't equipped to observe such an event:
http://www.nytimes.com/2014/11/08/science/space/bright-specks-of-comet-dust-light-up-martian-sky.html?_r=0
Yes, it was mentioned in the telecon this morning, along with a possible bright yellow glow in the night sky (from the sodium in the coma). The human eye would be far more subtle a detector than any mechanical camera, they mentioned.
That was one of the bits of the conference where there may have been a little disagreement on the panel. It was Nick Schneider saying there would've been a couple of tons of material entering Mars' atmosphere, which would result in a 1000s of meteors per hour storm. I forget who commented later about the particle size being smaller.
If the 1-3 mm size predictions were right (http://cometcampaign.org/tony/orbiter-results), the 'storm' would have produced a lot of meteors bright enough for normal human vision in dark skies, and many could have been bright enough for one of the rovers to see (in dark skies). If it had been partitioned into 1 g chunks, the rovers' cameras could have seen 1 every few minutes. If smaller, then it could have been human-visible but not visible to the current rover cameras (that's one area the sensitivities are not similar). But of course the prime reasons the rovers couldn't have seen it are not instrumental: daylight and (for MSL) 1000s of km of Mars.
Given the high speeds, the meteors might have become daytime visible (to a person) at a few grams, but short exposure times would have meant that 1000s of images would be needed to see one in a Pancam image--not to mention skipping the comet images. If close approach had been during the time Opportunity actually took images, there might have been not only a streaking comet, but 'noctilucent' illuminated trails left behind the meteors. But again, much smaller than this is expected for comet dust.
I was going to add some tidbits to the meteor matter, but Deimos beat me to it.
I link http://www.universetoday.com/116005/mind-blowing-meteor-shower-on-mars-during-comet-flyby-say-nasa-scientists/#more-116005.
Somewhat related, Mars Express had observations dedicated to meteor hunting, see pages 7-8 of http://mars.nasa.gov/files/mep/sidingspring/11_MEX_SS_Science_operations_WebEx.pdf
Since nothing from this showed up in their first image release, it seems like a safe bet they didn't get anything spectacular.
Without any atmosphere, Phobos and Deimos probably got a light peppering too. Would any craters even be more than a few cm across, or are they more like when tiny flecks of space junk do damage in LEO (i.e. microscopic)?
Great analysis, tolis, thanks! Doesn't sound like any detectable consequences at all, then.
However, the 'hide-the-orbiters' strategy still seems to have been a very prudent move. The odds of damage were pretty low, but definitely well above zero.
My http://planetimages.blogspot.com/2014/11/some-recent-views-of-mars-from-hubble.html post is largely based on the Hubble observations at the time of the climate flyby. It is unusual for it to look at Mars when it is so far away.
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