ESA Rosetta, news, updates and discussion |
ESA Rosetta, news, updates and discussion |
Apr 15 2005, 08:20 AM
Post
#1
|
|
Member Group: Members Posts: 563 Joined: 29-March 05 Member No.: 221 |
Well Rosetta isn't going to get to 67P/Churyumov-Gerasimenko (Chury) till 2014, but it's not to early to set up a thread. There are a bunch of earth fly-bys, a Mars encounter at 200km in 2007 and a few asteriod passes. Not to mention the mission to land on the comet itself.
Only another nine and a half years to go. |
|
|
Mar 2 2006, 08:56 AM
Post
#2
|
|
Senior Member Group: Members Posts: 1870 Joined: 20-February 05 Member No.: 174 |
The unusually high albedo measured with both polarimietry and with brightness + thermal infrared data (we need Spitzer measurements) really does seem to put this rock in the "e" category. I don't know how sure they currently are that this corresponds to rare and "weird" Enstatite chondrites. Is it the enstatite chondrites that have nearly identical oxygen isotope systematics to Earth and Moon rocks?
ANY opportunity to get a good look as something besides variations-on-a-theme of S type asteroids is extremely welcome. The only totally limited look we have of one is NEAR's nice flyby sequence of C type Mathilde, but it's just a nice sequence of pictures, mostly. The short 6-hour rotation rate of Steins will help get some rotational coverage, like Gaspra and Ida. |
|
|
Mar 2 2006, 09:35 AM
Post
#3
|
|
Senior Member Group: Members Posts: 3652 Joined: 1-October 05 From: Croatia Member No.: 523 |
What exactly will the closest approach distance to 2867 Steins be? I'll settle for an order-of-magnitude number if the distance is not precisely known yet.
-------------------- |
|
|
Mar 2 2006, 10:09 AM
Post
#4
|
|
Member Group: Members Posts: 563 Joined: 29-March 05 Member No.: 221 |
|
|
|
Mar 18 2006, 05:37 PM
Post
#5
|
|
Senior Member Group: Members Posts: 2488 Joined: 17-April 05 From: Glasgow, Scotland, UK Member No.: 239 |
And earlier still:
February 2007 - Rosetta Mars flyby (200km altitude) Bob Shaw -------------------- Remember: Time Flies like the wind - but Fruit Flies like bananas!
|
|
|
Mar 25 2006, 05:47 PM
Post
#6
|
|
Member Group: Members Posts: 124 Joined: 23-March 06 Member No.: 723 |
|
|
|
Mar 25 2006, 09:39 PM
Post
#7
|
|
Member Group: Members Posts: 370 Joined: 12-September 05 From: France Member No.: 495 |
I've heard nothing on this Mars flyby where does ESA release its press info ? Rosetta journey : http://www.esa.int/SPECIALS/Rosetta/ESA38F7708D_0.html Rosetta factsheet : http://www.esa.int/esaSC/SEMJ09374OD_0_spk.html Geometry of the flyby : http://www.space.irfu.se/rosetta/sci/mars/ |
|
|
Mar 28 2006, 06:03 PM
Post
#8
|
|
Senior Member Group: Members Posts: 2454 Joined: 8-July 05 From: NGC 5907 Member No.: 430 |
Astrophysics, abstract
astro-ph/0603720 From: Jessica Agarwal [view email] Date: Mon, 27 Mar 2006 13:00:59 GMT (713kb) Imaging the Dust Trail and Neckline of 67P/Churyumov-Gerasimenko Authors: J. Agarwal (1), H. Boehnhardt (2), E. Gruen (1 and 3) ((1) MPI-K Heidelberg, (2) MPS Katlenburg-Lindau, (3) HIGP Honolulu) Comments: 4 pages, 3 figures, to be published in the proceedings book of the conference "Dust in Planetary Systems 2005" We report on the results of nearly 10 hours of integration of the dust trail and neckline of comet 67P/Churyumov-Gerasimenko (67P henceforth) using the Wide Field Imager at the ESO/MPG 2.2m telescope in La Silla. The data was obtained in April 2004 when the comet was at a heliocentric distance of 4.7 AU outbound. 67P is the target of the Rosetta spacecraft of the European Space Agency. Studying the trail and neckline can contribute to the quantification of mm-sized dust grains released by the comet. We describe the data reduction and derive lower limits for the surface brightness. In the processed image, the angular separation of trail and neckline is resolved. We do not detect a coma of small, recently emitted grains. http://arxiv.org/abs/astro-ph/0603720 -------------------- "After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance. I see that such intercourse long continued would make one thoroughly prosaic, hard, and coarse. But the longest intercourse with Nature, though in her rudest moods, does not thus harden and make coarse. A hard, sensible man whom we liken to a rock is indeed much harder than a rock. From hard, coarse, insensible men with whom I have no sympathy, I go to commune with the rocks, whose hearts are comparatively soft." - Henry David Thoreau, November 15, 1853 |
|
|
Lo-Fi Version | Time is now: 10th November 2024 - 06:11 PM |
RULES AND GUIDELINES Please read the Forum Rules and Guidelines before posting. IMAGE COPYRIGHT |
OPINIONS AND MODERATION Opinions expressed on UnmannedSpaceflight.com are those of the individual posters and do not necessarily reflect the opinions of UnmannedSpaceflight.com or The Planetary Society. The all-volunteer UnmannedSpaceflight.com moderation team is wholly independent of The Planetary Society. The Planetary Society has no influence over decisions made by the UnmannedSpaceflight.com moderators. |
SUPPORT THE FORUM Unmannedspaceflight.com is funded by the Planetary Society. Please consider supporting our work and many other projects by donating to the Society or becoming a member. |