My Assistant
| Posted on: Jan 5 2019, 12:20 PM | |
![]() Newbie ![]() Group: Members Posts: 17 Joined: 15-August 15 Member No.: 7722 |
Actually, according to Alan Stern's post in "KBO encounters" thread, they will use LORRI to search for another targets : ) Owing to our remaining expected fuel supply we will have to search for small targets, which are more numerous. Calcs show this is most likely to be a flyby of a pristine comet nucleus. Such objects are about V=35 from Earth: hence undetectable, even with HST. So we would have to detect it with LORRI on New Horizons itself, which can see 3-10 km targets up to about 6 months ahead of us. Feasibility calcs will be done in 2019 (preliminary calcs are pessimistic but we really haven't scoured this to a solid conclusion). We'll see if this can work-- I hope so. It would be very cool to detect and target all from New Horizons with a "target of opportunity" flyby sometime n the 2020s! |
| Forum: New Horizons · Post Preview: #243211 · Replies: 294 · Views: 564367 |
| Posted on: Jan 2 2019, 06:53 PM | |
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Here are scientific papers available before the flyby: High-Precision Orbit Fitting and Uncertainty Analysis of (486958) 2014 MU69 (Locating Ultima Thule - The Planetary Mechanics Blog) Probing the Hill Sphere of (486958) 2014 MU69: HST FGS Observations During the July 17, 2017 Stellar Occultation The New Horizons Kuiper Belt Extended Mission Great Expectations: Plans and Predictions for New Horizons Encounter with Kuiper Belt Object 2014 MU69 (‘Ultima Thule’) The Color and Binarity of (486958) 2014 MU69 and Other Long-Range New Horizons Kuiper Belt Targets The HST Lightcurve of (486958) 2014 MU69 Crater Density Predictions for New Horizons flyby target 2014 MU69 How close were all the predictions? How many papers will come up during 2019? |
| Forum: New Horizons · Post Preview: #243001 · Replies: 294 · Views: 564367 |
| Posted on: Oct 14 2018, 07:08 AM | |
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There is new press release by DLR with some new images and details about MASCOT landing: Numerous boulders, many rocks, no dust: MASCOT's zigzag course across the asteroid Ryugu mcmcmc: That is very nice simulator! Thank you for that : ) |
| Forum: Hayabusa2 · Post Preview: #241454 · Replies: 983 · Views: 963083 |
| Posted on: Sep 27 2018, 09:21 AM | |
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| Forum: Hayabusa2 · Post Preview: #241163 · Replies: 75 · Views: 113591 |
| Posted on: Sep 12 2018, 07:42 AM | |
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According to update in japanese Hayabusa2 descended to 600 m above sufrace and then autonomous system stopped the descent and began to rise, probably due to unabillity to measure distance by LIDAR because Ryugu's surface have very low reflectivity. As for the spacecraft's shadow - it's clearly visible in several frames: ![]() /how can i reduce the size of inserted image? |
| Forum: Hayabusa2 · Post Preview: #240953 · Replies: 983 · Views: 963083 |
| Posted on: Aug 12 2018, 04:05 PM | |
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What bothers me about JAXA's latest findings is the dryness of Ryugu. JAXA were constantly saying, before arrival, that Ryugu had been chosen because it appears to be a water rich(?) asteroid. The reason must be remote spectroscopy unless it was just their wishfull thinking and unlss there are other means of guessing properties of asteroid surface. So, my guess is that remote spectroscopy across billion km is not at all reliable. Is that right? P There was some "suspected transient sublimation activity" as well. Curiously, the signature was observed when Ryugu was at aphelion. New candidates for active asteroids: main-belt (145) Adeona, (704) Interamnia, (779) Nina, (1474) Beira, and near-Earth (162173) Ryugu Possible sublimation and dust activity on primitive NEAs: Example of (162173) Ryugu |
| Forum: Hayabusa2 · Post Preview: #240695 · Replies: 983 · Views: 963083 |
| Posted on: Jul 18 2018, 08:07 PM | |
![]() Newbie ![]() Group: Members Posts: 17 Joined: 15-August 15 Member No.: 7722 |
Oh my! Those mosaics are absolutely stunning! I see lot of pockmarks (pits/craters) on that white surface, although gray material within linear troughs/chasms and around that flat elevated mesa at SW is rather smooth. Those bright fluvial features streaming down from flat-top mesa seems to be mixing with darker stuff which then covers underlaying bright deposits. I wonder, how amazing look would it be, standing down there next to central dome and looking SW at those streams! Streams and landslides within troughs seems to be the youngest geological features here. Or those pockmarks all around the bright stuff are not impacts, but rather some sublimation-pits or even cryovolcanic calderas?? Either way, it's crazy landscape.. |
| Forum: Dawn · Post Preview: #240375 · Replies: 79 · Views: 185733 |
| Posted on: Jul 11 2018, 10:20 PM | |
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| Forum: Hayabusa2 · Post Preview: #240267 · Replies: 983 · Views: 963083 |
| Posted on: Jul 2 2018, 06:20 PM | |
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Amazing! I really didn't expect we will see this thru Dawn's eyes. Trully extraordinary engineering and mission planning accomplishment. Reversed perspective of that mosaic makes more sense for my brain: ![]() Occator context image |
| Forum: Dawn · Post Preview: #240188 · Replies: 79 · Views: 185733 |
| Posted on: Jun 30 2018, 02:13 PM | |
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As i understand it, 7.6 hours isn't actually considered fast rotation. For asteroids this size it's rather slow. That's why i was proposing escaped-satellite scenario. Here are some ryugu-shaped fast rotators: ![]() Of those, only Bennu and 2008 EV5 have no known satellites. (And they have slowest rotation of this selection.) Didymos | 1994 CC | 1999 KW4 | 2001 SN263 | 2004 DC (Source of above image is Hayabusa2 press release from June 21.) |
| Forum: Hayabusa2 · Post Preview: #240166 · Replies: 983 · Views: 963083 |
| Posted on: Jun 28 2018, 08:43 PM | |
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... fast rotating rubble piles also seem to be the reason why a large percentage of near Earth asteroids have satellites of their own. Ryugu could have been fast rotator with its own moon in the past. But when that moon escaped, it took away lot of momentum from the system, which slowed down Ryugu to it's current 7,6 h rotation.. Or what else could shaped Ryugu like this except the fast rotation? |
| Forum: Hayabusa2 · Post Preview: #240149 · Replies: 983 · Views: 963083 |
| Posted on: Jun 23 2018, 08:55 AM | |
![]() Newbie ![]() Group: Members Posts: 17 Joined: 15-August 15 Member No.: 7722 |
They are definitely in Ryugu's sphere of influence... the last maneouevre brought the velocity to 9 cm per second, and over the last day or so it accelerated to 10 and now 11 cm/s. That has to be the asteroid's gravity giving a slight speed boost, right? There is also acceleration due to solar radiation pressure which has to be accounted for. Other effects (like Coriolis force and gravity of other bodies) should be negligible or not relevant at this point. |
| Forum: Hayabusa2 · Post Preview: #240025 · Replies: 983 · Views: 963083 |
| Posted on: Jun 19 2018, 08:49 AM | |
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Boom, there we have it! I see some equatorial craters as well as polar craters. Rotational bulge is very distinctive and equatorial ridge seems to be quite pronounced as well. Axis of rotation is almost perpendicular to ecliptic plane, but rotation is retrograde. Advantage is, that we'll gonna see whole Ryugu's surface, althogh landing spots may be limited to equator only.. (according to press release in japanese) ![]() |
| Forum: Hayabusa2 · Post Preview: #239915 · Replies: 983 · Views: 963083 |
| Posted on: Jun 15 2018, 06:36 AM | |
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| Forum: Dawn · Post Preview: #239830 · Replies: 79 · Views: 185733 |
| Posted on: Feb 2 2017, 10:38 PM | |
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Some flyby gifs: ![]() ![]() ![]() |
| Forum: Cassini's ongoing mission and raw images · Post Preview: #234420 · Replies: 90 · Views: 163195 |
| Posted on: Jan 18 2017, 07:41 PM | |
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Oh and look at this one! Wall of ice pillars emerging above ring plane.. ![]() |
| Forum: Cassini's ongoing mission and raw images · Post Preview: #234200 · Replies: 90 · Views: 163195 |
| Posted on: Nov 30 2016, 04:34 PM | |
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Yea! Right here : )) |
| Forum: Cassini's ongoing mission and raw images · Post Preview: #233574 · Replies: 90 · Views: 163195 |
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