Mission: Hayabusa 2 |
Mission: Hayabusa 2 |
Jun 26 2018, 02:46 PM
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#406
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Member Group: Members Posts: 238 Joined: 15-January 13 Member No.: 6842 |
I am neither a chemist nor a geologist, but I think carbonates would require liquid water to form. on the subject of the number of craters, on the latest image I can count only one bona fide crater, plus 3 or 4 suspect circular features, possibly subdued craters. Two very strong eroded crater candidates centre and just above the equator: (image enhanced by me to show features better) P.S. any chance to make a 3D model based on rotation images providing a stereo view? -------------------- Curiosity rover panoramas: http://www.facebook.com/CuriosityRoverPanoramas
My Photosynth panoramas: http://photosynth.net/userprofilepage.aspx...;content=Synths |
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Jun 26 2018, 03:00 PM
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#407
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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 |
I was thinking about these two. Plus a possible darker area near the limb at 4 o'clock.
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Jun 27 2018, 12:37 AM
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#408
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Member Group: Members Posts: 817 Joined: 17-April 10 From: Kamakura, Japan Member No.: 5323 |
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Jun 27 2018, 02:59 AM
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#409
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Forum Contributor Group: Members Posts: 1372 Joined: 8-February 04 From: North East Florida, USA. Member No.: 11 |
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Jun 27 2018, 03:22 AM
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#410
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Junior Member Group: Members Posts: 80 Joined: 18-October 15 From: Russia Member No.: 7822 |
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Jun 27 2018, 03:32 AM
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#411
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Senior Member Group: Members Posts: 2086 Joined: 13-February 10 From: Ontario Member No.: 5221 |
Wow! It really does look a bit brighter at the pole. Press conference soon (stereo image here: https://brianmay.com/brian/brianssb/brianssbjun18.html#29 )
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Jun 27 2018, 03:34 AM
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#412
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Member Group: Members Posts: 817 Joined: 17-April 10 From: Kamakura, Japan Member No.: 5323 |
Isn't the boulder shining at the top pole (apparently, south pole) a rare mineral, not the same kind making
up the rest of Ryugu?. I mean, something hard and slicky on surface, like diamond? P |
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Jun 27 2018, 03:54 AM
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#413
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Senior Member Group: Members Posts: 2086 Joined: 13-February 10 From: Ontario Member No.: 5221 |
As Phil said earlier in the thread when it first became visible, it might only be reflecting more sunlight, and not actually be any different in composition from the rest of the surface. But with more pixels, it does seem like it's not the only spot that seems slightly brighter. Itokawa was a lot more uniform from what I can recall.
Might be an intriguing target for one of the landers, or maybe even the impactor.... |
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Guest_mcmcmc_* |
Jun 27 2018, 07:54 AM
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#414
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Guests |
Ongoing press conference in japanese on youtube:
https://www.youtube.com/watch?v=Zmya363w010 |
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Guest_mcmcmc_* |
Jun 27 2018, 09:56 AM
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#415
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Guests |
Japanese press release is online:
http://fanfun.jaxa.jp/jaxatv/files/20180627_hayabusa2.pdf They announced they will also release English version. Facts sheet too: http://fanfun.jaxa.jp/countdown/hayabusa2/...sat33_fs_22.pdf 3d pictures: http://win98.altervista.org/hayabusa2/3d.html |
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Guest_mcmcmc_* |
Jun 27 2018, 10:25 AM
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#416
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Guests |
Interesting detail on page 91 of fact sheet about next approaching phase: for whole path from 20 km to 0 km it will be used ONC-W1 camera, but from 20km to 30m there will be the contribution from LIDAR (1 single laser beam), and from 50m to 0 the contribution of LRF (4 laser beams). Last 30 meters will have also contribution from light-reflection from target-marker-balls, reflecting lite from onboard LEDs.
They will also use a 3d digital model ("Ryuguoid"?). Further details on p.94 Align to surface linear speed at 100m. Switch from LIDAR to LRF at 40m (previous slide shows overlapping). Target balls released at 30m. Switch to autonomous mode and target-markers tracking at 15 meters. Free fall starting from 5-10 m, landing close to the ball. After shooting SCI bullet, precise landing into the crater will be allowed by using multiple target markers. |
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Guest_mcmcmc_* |
Jun 27 2018, 10:30 AM
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#417
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Guests |
Schedule:
End of July - Medium altitude observation 1 (altitude 5 km) Late August - gravity measurement descent (altitude 1 km) Late August - scheduled landing site September - October - Touchdown operation slot 1 September - October - Rover Drop Operation Slot 1 (which one of 4 rovers?) March-april 2019: shooting of SCI July 2019: rover Drop Operation Slot 2 (which one of 4 rovers?!?) |
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Jun 27 2018, 01:58 PM
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#418
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Member Group: Members Posts: 540 Joined: 17-November 05 From: Oklahoma Member No.: 557 |
3d pictures: http://win98.altervista.org/hayabusa2/3d.html The first picture, the cross eyed version, is inverted. The asteroid looks inside-out. |
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Guest_mcmcmc_* |
Jun 27 2018, 02:22 PM
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#419
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Guests |
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Jun 27 2018, 09:03 PM
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#420
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Administrator Group: Admin Posts: 5172 Joined: 4-August 05 From: Pasadena, CA, USA, Earth Member No.: 454 |
Wouldn't it be much easier landing on a static pole rather than on a moving equator? You would think so, but Dante Lauretta explained to me why not. It has to do with the challenges of navigating in the gravity field around the object. If you fly in from the top toward a pole, small imprecision in your understanding of the gravity field gets greatly amplified into where your spacecraft flies. Whereas if you are orbiting and you match velocities as you descend to the surface, it's a much easier situation to describe, physically, and the effect of small errors is much less. (Not sure if this makes sense.) OSIRIS-REx will also be selecting a landing site away from the poles. -------------------- My website - My Patreon - @elakdawalla on Twitter - Please support unmannedspaceflight.com by donating here.
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