Vesta departure and journey to Ceres, A new phase of Dawn adventure |
Vesta departure and journey to Ceres, A new phase of Dawn adventure |
Aug 26 2012, 05:45 AM
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#1
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
As suggested by "TheAnt", is time to start a new thread!
Due to lack of updates from "Mystic simulator", I asked directly to Marc Rayman for an update and he kindly sent me the following "unofficial" plots, showing evolution of distance, radial velocity and sub-spacecraft latitude (radius trend is splitted in two plots with different scales due to huge variation of the distance): I did not publish them immediately because I wanted to integrate them with my previous plots but, due to the lack of time in last week, I decided to post them directly with only minimal changes. As you can see, third engine stop occurred on Aug 8-18 at almost 2300km above Vesta while next (final) one is just started and, as reported by Marc in his latest journal, will be used to map North polar regions from 6000km distance. Thereafter thrust will resume and, based on plots, on Sept 5 total speed will overcome escape velocity (almost 45 m/s), so total energy balance will be zero; definitive exit from Vesta Hill sphere should occur after 20 days but consider that the times could slighty change due to orbit refinement and thrust plan changes. -------------------- I always think before posting! - Marco -
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Aug 26 2012, 11:17 AM
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#2
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Junior Member Group: Members Posts: 22 Joined: 23-August 11 From: France Member No.: 6134 |
Thanks Dilo for the updating. I was little worried. Last spice spk file (25 august) shows that Dawn will not escape form Vesta indicating an another problem. But it seems now that this file was only a test.
My little contribution with this video created thanks to spice data from NAIF. http://www.youtube.com/watch?v=EL5nbFU3xl8 Since SPICE doesn't indicate the states of engines, the orbital parameters are only "guessed" assuming a Vesta like a point mass of 2.59^20 kg. |
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Aug 26 2012, 05:18 PM
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#3
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Interplanetary Dumpster Diver Group: Admin Posts: 4404 Joined: 17-February 04 From: Powell, TN Member No.: 33 |
Departure was not supposed to happen until the 26th.
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Aug 26 2012, 11:41 PM
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#4
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Junior Member Group: Members Posts: 22 Joined: 23-August 11 From: France Member No.: 6134 |
Sorry, I meant the date of spk file releasing (25 august) not the date of depart which is scheduled on 5 september as dilo wrote.
The initial departure was planned on 26 august but after the problem with wheels reaction it was postponed as we know. But i remain concerned: the last spice ck file shows that the observation of Vesta to mapping north pole didn't occur |
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Aug 27 2012, 06:15 PM
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#5
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Junior Member Group: Members Posts: 22 Joined: 23-August 11 From: France Member No.: 6134 |
I must apologize for my previous post.
According to the spice files released today, there was an attempt to observe Vesta as planned. The ck file shows that the probe has problem to maintain her orientation but i don't know if this effect is due to the ck files (always under construction) or the problem of lack of one reaction wheels. From now, I will avoid any speculations useless alarmist and I will wait the official update of wonderfull Dawn journal and Dilo states plots (specially the states of engine propulsion ) (from Mystic or Marc). And of course hope of beautiful images of Vesta's north pole Again very sorry. |
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Aug 28 2012, 04:59 PM
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#6
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
I had a private comunication from Mark, he confirmed that they successfully imaged Vesta over the weekend.
Moreover, he said there wasn't any problem with the SPK file. As explained in several Dawn Journals (including November 29, 2011), they generate a reference trajectory that goes all the way to the next destination but then, as they fly along, they generate updated flight profiles to account for all the usual error sources (orbit determination accuracy, unmodeled perturbations from RCS, deviations in IPS thrust from the modeled value, etc.). Each time an updated thrust plan is sent to the spacecraft, they only send the next thrust segment, not the full reference trajectory; in this way, in case of failure, they don't have onboard ephemeris based on thrusting that didn't occur. So when they upload the new thrust segment, they upload a new ephemeris as well. Probably, SPK issue Sarunia found is for an isolated thrust segment which then is followed by a ballistic propagation... -------------------- I always think before posting! - Marco -
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Aug 31 2012, 07:48 AM
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#7
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
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Aug 31 2012, 08:52 PM
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#8
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Member Group: Members Posts: 495 Joined: 12-February 12 Member No.: 6336 |
Thank you for posting that one Explorer1.
Next stop Ceres in 2015, so lets find out what that bright spot is then. |
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Sep 1 2012, 04:08 PM
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#9
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Senior Member Group: Members Posts: 1276 Joined: 25-November 04 Member No.: 114 |
It looks like a peak of a crater to me.
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Sep 2 2012, 02:39 AM
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#10
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Member Group: Members Posts: 311 Joined: 31-August 05 From: Florida & Texas, USA Member No.: 482 |
Looks like an informative Hasta La Vesta hangout:
"We’re celebrating this milestone with a live Google+ Hangout featuring the Dawn mission team September 8, 2012 at noon PDT. During the Hangout, moderated by Dawn’s education and public outreach (E/PO) liaison to the science team, Dr. Britney Schmidt, we’ll hear stories from Dawn scientists and engineers and get updates on latest mission findings. Pose the questions you’ve always wanted to ask. Submit your questions for the Dawn team by leaving them in the comments section below, on Dawn’s Facebook page, or by using the hashtag #HastaLaVesta on Twitter." |
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Sep 5 2012, 05:00 PM
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#11
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
Based on last Dr Rayman (unofficial) comunication, this morning at 6.45 UT, Dawn definitively leaved Vesta gravitational field when his speed exceeded escape speed (45 m/s at 18000 km height). Curiously, in the same hours MISTIC simulator went back online...
-------------------- I always think before posting! - Marco -
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Sep 6 2012, 01:17 AM
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#12
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Member Group: Members Posts: 813 Joined: 29-December 05 From: NE Oh, USA Member No.: 627 |
A Last Look Back at Vesta ....bye Vesta...
http://dawn.jpl.nasa.gov/feature_stories/d...parts_vesta.asp http://dawn.jpl.nasa.gov/multimedia/last_look_back.asp From Protoplanet to Dwarf Planet.... Ceres here we come. Craig |
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Sep 6 2012, 02:40 AM
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#13
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
The pole at last! I'm assuming it's in the largest crater, right?
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Sep 6 2012, 08:42 AM
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#14
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Member Group: Members Posts: 102 Joined: 29-January 10 From: Poland Member No.: 5205 |
Hi
I see some difference in Dawn - Vesta position at Mystic Simulator and Eyes of the Solar System Date and time is 9:43 UTC - 06 Sep 2012 See screens below. What's wrong ? What distance are good ? --------- Added: In HORIZONS JPL is 64 540 km http://ssd.jpl.nasa.gov/horizons.cgi --------- Also in Solar System simulator is 64 549 km http://space.jpl.nasa.gov -------------------- Adam Hurcewicz from Poland
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Sep 6 2012, 10:27 AM
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#15
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
I see some difference in Dawn - Vesta position at Mystic Simulator and Eyes of the Solar System Adam, I can say Mystic is perfectly in line with Marc Rayman plots, as showed in these plots where I merged the two sources: (consider that Mystic hiatus ended yesterday and lasted 1 month; moreover, you will not see distance/velocity modulations due to elliptic orbit during third engine stop because I reported only average info in this period). Moreover, both Marc/Mystic data are in agreement with last Nasa updates about Vesta depart milestone (see links from bellarophon1); in my plots (left/bottom in particular) you can see that total energy becomes positive only on Sptember,5 while, if Dawn really lies at 64500 km from Vesta, this means he surpassed this point many days ago and is already half-way to Vesta Hill sphere margin! -------------------- I always think before posting! - Marco -
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Sep 6 2012, 07:31 PM
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#16
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Junior Member Group: Members Posts: 22 Joined: 23-August 11 From: France Member No.: 6134 |
According to the last SPICE kernel (but based on predicted trajectory), Dawn was at 20600 km from Vesta at 9:43 UTC 06 september.
For checking Dawn in real time, Mystic seems to be better than another simulator with extra information that SPICE haven't (like engine status). I think that the administrators of "Eyes of Solar System" and others just didn't updated the new data. Dilo, could you ask Marc if the remaining reaction wheels were turned off during the last observation of Vesta ? |
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Sep 6 2012, 08:22 PM
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#17
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Founder Group: Chairman Posts: 14433 Joined: 8-February 04 Member No.: 1 |
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Sep 6 2012, 08:37 PM
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#18
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Member Group: Members Posts: 311 Joined: 31-August 05 From: Florida & Texas, USA Member No.: 482 |
Marc just updated his excellent blog:
http://blogs.jpl.nasa.gov/tag/marc-rayman/ So the reaction wheels are nominal and it was simply a programming error that was trying to deactivate them earlier? That is excellent news! C'mon Ceres... are we there yet? [:-p] |
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Sep 6 2012, 09:05 PM
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#19
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Member Group: Members Posts: 913 Joined: 4-September 06 From: Boston Member No.: 1102 |
My reading of Marc's blog didn't indicate things were "nominal" with the reaction wheels--rather that one malfunctioned and all were turned off a week earlier than they were going to turn them off. I believe they started with 3 and 1 backup and have now lost 2. That is not good and will have to be worked around at Ceres when the space craft will need to do lots of turning for imaging and other science. Where did you hear it was an software/programming error rather than a hardware failure?
-------------------- |
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Sep 6 2012, 09:55 PM
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#20
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Founder Group: Chairman Posts: 14433 Joined: 8-February 04 Member No.: 1 |
In a talk by Marc last week for the EPO folk on lab - he echoed what you describe Floyd. Marz - I think you have things wrong.
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Sep 6 2012, 10:32 PM
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#21
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Member Group: Members Posts: 311 Joined: 31-August 05 From: Florida & Texas, USA Member No.: 482 |
In a talk by Marc last week for the EPO folk on lab - he echoed what you describe Floyd. Marz - I think you have things wrong. darn! Here's the quote from the blog, with italics around the statement I misinterpreted and bold in the phrase I used to jump to conclusions. "on August 8 ... one of the reaction wheels experienced an increase in internal friction. ... Protective software quickly detected the event and correctly responded by deactivating that wheel and the other two that were operating, switching to the small jets that are available for the same function, and reconfiguring other systems, including powering off the ion thrust and turning to point the main antenna to Earth. A routine communications session the next day revealed to mission controllers what had occurred. They had planned long ago to turn the wheels off for the flight from Vesta to Ceres, so having them off a few weeks early was not a significant change. The team soon restored the spacecraft to normal operations and reformulated the departure plan, and on August 17 Dawn resumed its ascent. Because of the hiatus in thrusting, escape shifted from August 26 to September 4. The flexibility in the mission timeline provided by ion propulsion made this delay easy to accommodate." The next paragraph hints that the reaction wheels are potentially out, since hydrazine is now a precious resource: "In order to conserve the hydrazine propellant that the jets use, the bonus departure observations described before were curtailed, as they were not a high priority for the mission." Hopefully we can find out more details on the reaction wheels on the Sept 8th hangout. |
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Sep 8 2012, 10:54 AM
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#22
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
Update on departure progress:
(Note1: I smooted all previous phases in order to show only averaged distance/speed/energy without elliptic-orbit related modulations; Note2: interpolations in top/right plot are simply 2nd order empiric curves without geometric/gravitational considerations behind). -------------------- I always think before posting! - Marco -
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Sep 11 2012, 01:09 PM
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#23
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
I just received some informations from Dr Rayman which shed more light on the reaction wheel issue.
The wheels were all turned off on August 8, when the software detected the increase in friction, and were left off since then, including for the departure observations. They restored spacecraft to normal operations, but one of "normal operational modes" is to fly with all wheels off (they flew that way from August 2010 to May 2011 and they intend to do so for the journey from Vesta to Ceres). So, "wheels off" is a normal operational mode and future Ceres exploration plan will be based on the use of the two reaction wheel + RCS "hybrid" control capability, installed on the spacecraft in April 2011. Marc highlighted that most of these information were available in previous Dawn journal articles and that he will write more about the reaction wheels, RCS control, hybrid control, and hydrazine in future Dawn Journals (although not the next one). Herebelow an update on departure plots, showing also a brief engine stop occurred yesterday: In the bottom/right, I substituted the "Energy ratio" plot with a more interesting plot showing the angle between Vesta-Dawn distance vector and Dawn velocity vector, calculated from total velocity and distance informations in Mystic Simulator (or radial velocity + distance in Marc plots). As you can see, Dawn trajectory is going from a "quasi-orbital" situation (with perpendicular vectors) to a more straightforward escape trajectory (zero angle). The spread of points in the September 5-9 interval is due to the poor precision in calculated distance differences; situation improved when I realized that this page gives more precise figures... -------------------- I always think before posting! - Marco -
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Sep 13 2012, 06:13 AM
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#24
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
Marc confirmed there was a programmed engine stop on September,10 for communication with Earth (they do this each week but probably frequence will be relaxed during the journey to Ceres). Effect is clearly visible in velocity and orientation plots (right):
Based on my interpolations, Dawn should reach Hill sphere border on September,24 around 8:00 UTC, with 140m/s speed. -------------------- I always think before posting! - Marco -
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Sep 14 2012, 05:29 PM
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#25
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
Update:
Based on new data points and improved interpolation, Hill sphere crossing date forecast is anticipated to September,23 17:40 UTC, if no further stops will occur... -------------------- I always think before posting! - Marco -
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Sep 16 2012, 03:36 PM
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#26
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
Update:
No major changes on Hill sphere crossing date from interpolation; I ran also a simulation using constant engine orientation and thrust (5.1e-5 N/kg) and forecast time is only slightly different (September,23 15:30 UTC)... -------------------- I always think before posting! - Marco -
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Sep 16 2012, 05:36 PM
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#27
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
It's amazing how symmetrical Vesta's hemispheres are on the global scale, on this topographic map that includes the far north.
But the northern basin isn't from a giant impact, is it? http://dawn.jpl.nasa.gov/multimedia/imageo...p?date=20120911 |
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Sep 16 2012, 06:51 PM
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#28
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
Explorer1, the northern basin isn't a crater and blue color is due to oblate spheroid shape of Vesta.
In fact, text underline that colors represent distance relative to Vesta's center (or height relative to a sphere with 500km diameter); most important, scale of the two maps isn't the same because lower (violet) points in Northern emisphere are only 22km below such sphere while South depressions reach -38km. Anyway, the presence of spiral patterns in both polar regions (with opposite orientations) is very intriguing... PS: I like very much the Giordano Bruno statement in your signature! -------------------- I always think before posting! - Marco -
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Sep 16 2012, 07:05 PM
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#29
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Senior Member Group: Members Posts: 3419 Joined: 9-February 04 From: Minneapolis, MN, USA Member No.: 15 |
Yes, the spiral patterns resemble, more than anything else, the pattern of modification one sees at Mars' poles. But... Vesta couldn't possibly have ever had enough atmosphere to support ice caps, could it?
-the other Doug -------------------- “The trouble ain't that there is too many fools, but that the lightning ain't distributed right.” -Mark Twain
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Sep 17 2012, 01:18 PM
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#30
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Member Group: Members Posts: 656 Joined: 20-April 05 From: League City, Texas Member No.: 285 |
It would be really helpful to have a 3D rendered globe of Vesta -- much would be come clear, I think.
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Sep 17 2012, 03:02 PM
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#31
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Member Group: Members Posts: 140 Joined: 20-November 07 Member No.: 3967 |
Soon as Phil gives the okay, I'll get started on a fold-up map of the thing.
Phil . . . ? |
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Sep 18 2012, 05:43 PM
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#32
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
Update:
Last engine stop, yesterday, lasted about 9 hours based on speed data; as consequence, Hill sphere exit date shifted slightly ahead (Sep,23 around 20 UTC). PS: in the last posts, the two left plots (long term range/speed and Energy trends) weren't updated correctly, I'm sorry for this! -------------------- I always think before posting! - Marco -
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Sep 21 2012, 11:31 AM
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#33
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
-------------------- I always think before posting! - Marco -
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Sep 21 2012, 04:03 PM
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#34
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Solar System Cartographer Group: Members Posts: 10191 Joined: 5-April 05 From: Canada Member No.: 227 |
"Phil . . . ? "
OK Chuck - here I have taken those two polar maps of topography and reprojected them into simple cylindrical. There are a few very minor errors in this composite but nothing to worry you in your work. It should be easy to match this with published gridded maps to get crater names, lat and long etc. (a grid is faintly visible on this, from the originals). But this gives you the topography to locate your ridge lines etc. PS - apparent mismatch along the equator is caused by different illumination of the rendered shaded relief between the two halves. Phil -------------------- ... because the Solar System ain't gonna map itself.
Also to be found posting similar content on https://mastodon.social/@PhilStooke Maps for download (free PD: https://upload.wikimedia.org/wikipedia/comm...Cartography.pdf NOTE: everything created by me which I post on UMSF is considered to be in the public domain (NOT CC, public domain) |
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Sep 24 2012, 10:55 PM
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#35
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Senior Member Group: Members Posts: 2492 Joined: 15-January 05 From: center Italy Member No.: 150 |
This is my final update plot of Vesta departure:
Dawn is definitively out of Vesta sphere of influence, exact time depends on which Hill sphere radius you assume. In fact, while classic formula is based on average distance of the body from Sun, others reccomend to use pericenter distance, which gives a smaller radius; moreover, I calculated also the present Hill radius based on current heliocentric distance. Here below my results, based on interpolation of Mystic simulator distances (sorry for improper use of "code" format but table format appears problematic otherwise!): CODE Method (Sun distance) Distance from Vesta date/time UTC I tend to prephere last one, which occurrred few hours ago, probably during the weekly engine shutdown...
Periastron 113180 km Sep, 22 12:40 Average 124180 km Sep, 23 18:52 Current 134750 km Sep, 24 22:30 -------------------- I always think before posting! - Marco -
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Nov 3 2013, 05:57 PM
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#36
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
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Dec 7 2013, 03:39 AM
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#37
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
New info about Ceres plan, with details on hybrid control mode for low-altitude mapping orbit:
http://dawn.jpl.nasa.gov/feature_stories/D..._Dance_Card.asp |
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Dec 1 2014, 09:51 PM
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#38
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Member Group: Members Posts: 541 Joined: 17-November 05 From: Oklahoma Member No.: 557 |
According to the November 2014 Dawn Journal, today is the day that Dawn takes its first resolved photos of Ceres, nine pixels across. These are being taken mainly to calibrate the camera. Still a couple of months to go before they start getting the really good stuff.
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Dec 1 2014, 11:34 PM
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#39
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Senior Member Group: Admin Posts: 3108 Joined: 21-December 05 From: Canberra, Australia Member No.: 615 |
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Dec 5 2014, 03:33 PM
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#40
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Senior Member Group: Members Posts: 1729 Joined: 3-August 06 From: 43° 35' 53" N 1° 26' 35" E Member No.: 1004 |
the Max Planck Institute has a release (i n German) with the first, distant images of Ceres:
http://www.mps.mpg.de/3867888/PM_2014_12_0..._eine_neue_Welt |
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Dec 5 2014, 03:41 PM
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#41
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Member Group: Members Posts: 541 Joined: 17-November 05 From: Oklahoma Member No.: 557 |
Here is a link to the picture on the Dawn web site: Dawn snaps Ceres
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Dec 5 2014, 07:25 PM
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#42
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Junior Member Group: Members Posts: 31 Joined: 3-August 14 From: Germany Member No.: 7229 |
the Max Planck Institute has a release (i n German) with the first, distant images of Ceres: From the Max Planck release: "up to today, the sharpest images of Ceres were acquired by HST. Starting end of January 2015, the Framinc Camera images will match and exceed that resolution. From that moment on, we'll enter a new Land." -------------------- space scout
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Dec 6 2014, 10:51 AM
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#43
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Member Group: Members Posts: 568 Joined: 20-April 05 From: Silesia Member No.: 299 |
Without a doubt, Ceres is significantly larger than Vesta.
In three or four weeks should start to reveal the first surface details. -------------------- Free software for planetary science (including Cassini Image Viewer).
http://members.tripod.com/petermasek/marinerall.html |
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Dec 6 2014, 12:05 PM
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#44
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Junior Member Group: Members Posts: 95 Joined: 5-September 07 Member No.: 3662 |
This is exciting! Can't wait to see Ceres close up. Almost looks like albedo differences in the photo, but could just be phase effects.
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Dec 6 2014, 12:45 PM
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#45
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Member Group: Members Posts: 813 Joined: 8-February 04 From: Arabia Terra Member No.: 12 |
Exciting... but in a bittersweet way. This finishes the initial reconnaissance of the rocky terrestrial worlds in our local neighbourhood. If we want fresh terra incognita after this we have to go way, way out to the solar system's frigid fringes.
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Dec 6 2014, 11:55 PM
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#46
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Administrator Group: Admin Posts: 5172 Joined: 4-August 05 From: Pasadena, CA, USA, Earth Member No.: 454 |
I'd like to see Pallas and Hygeia! I want to see how the biggies transition down to the small ones we've seen. Also, while I'm wishing for things, I want much better imaging of Deimos. And heck let's go visit some Trojans too.
-------------------- My website - My Patreon - @elakdawalla on Twitter - Please support unmannedspaceflight.com by donating here.
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Dec 7 2014, 12:27 AM
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#47
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
Hektor especially would be a great destination: a contact binary an order of magnitude bigger than 67P and with a moon (always a bonus). We know practically nothing about that region...
Now to wait until the next round of Discovery proposals. |
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Dec 7 2014, 03:00 AM
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#48
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Senior Member Group: Members Posts: 1074 Joined: 21-September 07 From: Québec, Canada Member No.: 3908 |
It would be interesting also to visit a large metallic asteroid.
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Dec 7 2014, 03:30 AM
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#49
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
Yep, the team proposing a Psyche mission agrees:
http://www.planetary.org/blogs/guest-blogs...llic-world.html |
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Dec 7 2014, 05:23 PM
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#50
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Interplanetary Dumpster Diver Group: Admin Posts: 4404 Joined: 17-February 04 From: Powell, TN Member No.: 33 |
I'd like to see Pallas and Hygeia! I want to see how the biggies transition down to the small ones we've seen. Also, while I'm wishing for things, I want much better imaging of Deimos. And heck let's go visit some Trojans too. Pallas has always seemed particularly interesting as a transitional world. -------------------- |
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Dec 7 2014, 05:57 PM
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#51
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Member Group: Members Posts: 813 Joined: 8-February 04 From: Arabia Terra Member No.: 12 |
I'm sure these are all fascinating in their own right. But there's something special about seeing the curving limb of a gravitationally relaxed body- Ganymede, Enceladus, Triton... these all seem like places to me in a way that Vesta never quite did.
QUOTE Then felt I like some watcher of the skies
When a new planet swims into his ken; Or like stout Cortez when with eagle eyes He star'd at the Pacific — and all his men Look'd at each other with a wild surmise — Silent, upon a peak in Darien. |
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Dec 10 2014, 08:37 AM
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#52
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
Google Hangout about the Hubble/Dawn imagery comparison coming up:
http://dawn.jpl.nasa.gov/dawncommunity/goo..._12_11_2014.asp It might also be time for a dedicated Ceres approach thread. |
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Dec 10 2014, 01:01 PM
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#53
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Member Group: Members Posts: 710 Joined: 28-September 04 Member No.: 99 |
Less than 1 million km now!!! So close!
I'm wondering though, if the ion-thrusters would fail right now, how close would the flyby be? Or could it still limp into orbit by using all the remaining conventional fuel? It might also be time for a dedicated Ceres approach thread. And a Ceres prediction thread. Could be fun to see who makes the right prediction. Will the surface look like Tethys? Callisto? Enceladus? |
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Dec 10 2014, 05:18 PM
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#54
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
I'd say Callisto or Mimas, just keeping expectations low (i.e. completely saturated with craters). That way everything else can be a pleasant surprise.
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Dec 12 2014, 11:42 PM
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#55
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Junior Member Group: Members Posts: 48 Joined: 10-September 06 Member No.: 1129 |
I'd say Callisto or Mimas, just keeping expectations low (i.e. completely saturated with craters). That way everything else can be a pleasant surprise. Its density is comparable to Ganymede and Callisto, but it's also warmer -- warmer than any icy moon. Plus we know there's some water vapor around it (outgassing? sublimation?) and that the surface is dark. So I think it could be quite a unique world even if it's not geologically active. |
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Dec 13 2014, 04:49 AM
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#56
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Member Group: Members Posts: 315 Joined: 1-October 06 Member No.: 1206 |
There was a paper published last year, in Icarus I think, that suggested the warmer surface of Ceres compared to the outer moons might result in VERY subdued crater topography (really all but small and fresh craters slump over geological time until they become mere albedo features) except right near the colder poles. So, even if its geologically 'boring', (and I hope it isnt!), I doubt Ceres is going to look like Callisto or Mimas.
P |
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Dec 13 2014, 04:33 PM
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#57
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Newbie Group: Members Posts: 9 Joined: 7-December 14 Member No.: 7360 |
Pallas has always seemed particularly interesting as a transitional world. The planetoid I want to see the most next is 24 Themis: http://en.wikipedia.org/wiki/24_Themis In a similar location to Ceres, 200 km in diameter, a surface with lots of water ice, and most importantly: Inclination 0.7595° So it orbits on exactly the same orbital plane as us. Very rare for an object of its type. |
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Dec 13 2014, 06:17 PM
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#58
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Founder Group: Chairman Posts: 14433 Joined: 8-February 04 Member No.: 1 |
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Dec 13 2014, 07:05 PM
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#59
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Senior Member Group: Members Posts: 2090 Joined: 13-February 10 From: Ontario Member No.: 5221 |
Huh, that's a tiny fraction of the tilt of Vesta and Ceres; its even smaller than Mars and Venus.
So many tempting targets out there for future missions (Dawn 2 anyone?). |
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Dec 13 2014, 08:48 PM
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#60
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Junior Member Group: Members Posts: 95 Joined: 5-September 07 Member No.: 3662 |
I would love to see a series of smallsats sent to asteroids. If successful, the Procyon satellite launched with Hayabusa-2 might encourage such missions. Imagine using a large booster to put dozens of these into the asteroid belt at the same time...
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Dec 14 2014, 06:43 AM
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#61
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Founder Group: Chairman Posts: 14433 Joined: 8-February 04 Member No.: 1 |
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Dec 14 2014, 10:34 AM
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#62
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Junior Member Group: Members Posts: 78 Joined: 20-September 14 Member No.: 7261 |
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Dec 14 2014, 10:44 AM
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#63
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Senior Member Group: Members Posts: 1729 Joined: 3-August 06 From: 43° 35' 53" N 1° 26' 35" E Member No.: 1004 |
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Dec 14 2014, 02:51 PM
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#64
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Member Group: Members Posts: 495 Joined: 12-February 12 Member No.: 6336 |
at which heliocentric distance? IIRC, the delta-V for plane change(for a solar orbit) depends on the heliocentri distance Indeed it does, lets say we are to launch one dedicated mission to study Pallas, the best idea would to launch the spacecraft at an inclined orbit around the Earth of 34.8° from the very start, and then to send it on its way with the upper stage. So as for expectations, I came to the same conclusion as antipode, without having read the paper in question. Meaning that with the relatively high daytime temperature I expect Ceres to be a quite flat around the equator, but with a bit more topography, more distinct crater rims etc, toward the poles. And with brighter poles, from hoarfrost that have settled there. |
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Jan 4 2015, 02:00 AM
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#65
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Member Group: Members Posts: 808 Joined: 10-October 06 From: Maynard Mass USA Member No.: 1241 |
While we wait for DAWN to snap more approach images of Ceres, I put the Dec 2014 Framing Camera image (PIA19049) through the deconvolution process. I hate going above 10x on an image, since we are pushing around noise, point spread functions of the camera, and other artifacts (such as working from a JPEG). But I ran this baby up to the max: 30x (!)
Don't try to see craters or such things other than a bright area on the right side (and a slightly darker 'depression' on the lower right --to be named the pdp8e abyss ). Most of the image is the deconvolver 'hallucinating' about what it thinks it sees... but it is fun! The size difference (not resolution) is about what Ceres would appear at roughly 25,000 miles away -------------------- CLA CLL
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Jan 4 2015, 10:27 PM
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#66
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Member Group: Members Posts: 495 Joined: 12-February 12 Member No.: 6336 |
@PDP8E: Yes it is really to early to see anything on Ceres yet.
But keep it up and in a little over a month we might get to see the first detail. Hubble images have hinted there is at least one surface feature that could be spotted even at the early approach. Now craters, if our current thinking is correct Ceres got a dusting of material on top, so larger (and more recent) craters might have a bright bottom. While I am at it, I am quite pessimistic on the outlook to find any satellite at Ceres for the same reason, any impact that might have sent material into orbit will be mostly be ice and might sublimate before it have time to coalescence, (which might be how the smaller satellites of Pluto came to be in that much colder environment.) There could be a very small rock in orbit, as for example one component of a binary asteroid that been captured and the small size made it escape detection in telescopic searches. |
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Jan 5 2015, 12:42 AM
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#67
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Junior Member Group: Members Posts: 78 Joined: 20-September 14 Member No.: 7261 |
"Very small rock" is a relative term - e.g. in this abstract the detection limit mentioned for various searches of Ceres' inner Hill Sphere is somewhere around 1-2 km at 4000 km, possibly bigger further in. And since Ceres' Roche limit even for the most porous of rubble piles is well below 2000 km...
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Jan 5 2015, 02:29 AM
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#68
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Member Group: Members Posts: 495 Joined: 12-February 12 Member No.: 6336 |
Yes "relative" is the word, I were aware of those searches mentioned in the paper and with a size of just one km or two it could be more suitable to name it 'rock' here than Moon which usually make people think of a more substantial object. =)
But yes it could be somewhat larger, especially if it is exceptionally dark. |
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Mar 12 2015, 12:58 PM
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#69
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Member Group: Members Posts: 107 Joined: 1-August 14 Member No.: 7227 |
Shouldn't this thread be closed now that Ceres finished its journey?
We are now talking about orbiting Ceres: http://www.unmannedspaceflight.com/index.p...mp;#entry218672 |
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