Rosetta wakes up for encounter with asteroid (2867) Steins / La sonda Rosetta pasará asteroide Steins el 5 de septiembre
Friday, July 04, 2008
Wow, just this morning I mentioned that Rosetta would be passing by the asteroid 2867 Šteins, and less then a day later there's an article on the craft at spaceref.com about how it has been dragged out of its slumber for the encounter:
Spacecraft controllers have just awoken Rosetta from hibernation to prepare for its encounter with asteroid (2867) Steins on 5 September. ESA's comet chaser will study the relatively rare asteroid as it flies by on its way to comet 67/P Churyumov-Gerasimenko.This is the first of two:
Rosetta has swung by Earth twice and Mars once, performing gravity-assist manoeuvres, that gave it the necessary boost to continue on its journey. The third and last Earth swing-by is scheduled for November 2009. The spacecraft will also fly by two asteroids and study them on the way: (2867) Steins in September this year and (21) Lutetia in June 2010. As it closes in on (2867) Steins in September, Rosetta will have travelled about 3700 million km and will be 2.1 AU from the Sun.Also, here are the objectives of the flyby:
The science objectives of the fly-by observations are as follows:
- To characterise the asteroid by studying its physical and chemical properties
- To study its kinematic properties (its rotation, for example)
- To study the asteroid's surface and to perform comparative studies with surfaces of other asteroids in order to understand differences between asteroid types
- To study the interaction between the solar wind and the asteroid
- To study the asteroid's environment, including the presence of natural satellites, the magnetic and electrical properties of the immediate environment, and gas or dust orbiting the asteroid
So what can we expect the flyby images to look like? One particularly notable flyby of an asteroid was that of 243 Ida in 1994 by Galileo as it was on its way to Jupiter. Here are some details to help imagine: Ida is 53.6×24.0×15.2 km in diameter, and has a moon named Dactyl that was discovered during the flyby that has a diameter of 1.4 km, and from a distance of 10,500 km out it looked like this:
So imagine the tiny moon on the right but two to three times as big, and taken from a distance some twelve times closer. I have no idea what sort of image resolution capabilities Rosetta has compared to Galileo though, so that's the one factor that I can't take into account.
Also, on the space.com forums my favourite poster has also commented on what the encounter should be like. Here's what he says:
This Asteroid 5535 Annefrank photograph was taken under these conditions (quoted from the poster just above the last one):It promises to be interesting, as we know virtually sod all about Asteroid 2867 Šteins.
Regarding sizes, a lot of it is assumption, based on brightness & spectra verses distance, other than those we have either seen up close (951 Gaspra, 243 Ida, 253 Mathilde, 433 Eros, 5535 Annefrank, etc) or those we have actually seen a shape for like 1 Ceres, 3 Juno, 4 Vesta, 511 Davida, etc.
So do not be surprised if 2867 Šteins turns out to be a completely different size to that expected. Because this willbe a relatively slow encounter, Rosetta should see much of 2867 Šteins during approach (earlier Rosetta obs suggests a rotational period of about 6 hours), as Galileo did with 243 Ida & 951 Gaspra.
AFAIK, the OSIRIS camera, also has a much higher resolution than did Stardust, so together with this & the much closer pass, the imagery & other data of 2867 Šteins, should be pretty spectacular. It is something to look forward to.
Also later on in July 2010 (IIRC), Rosetta encounters the much larger type M asteroid 21 Lutetia.
Best Stardust view of Asteroid 5535 Annefrank.
For comparison, we have this picture taken of asteroid 5535 Annefrank taken from a distance of 3,300 km. The asteroid has a of length 8 km (it was predicted to be of half of that).So, conclusion? This should be a very good flyby. Expect nice pictures.
8 comments:
Thank you very much mithridates, I did not realise that I was your favourite poster over at SDC. I'm quite blown away.
You too are high in my list of favourites. Our interests are remarkably similar, that helps :)
Regarding the upcoming 2867 Steins, despite being no larger than some mountains on Earth, 2867 Steins has much of interest to offer. The spectra so far obtained suggests a basaltic makeup, not too different in composition to the Earth's mantle or the surface of Mercury. We have not yet encountered such an asteroid, mostly type S types so far with 253Mathilde being the only C type seen up close (perhaps the Mars Moons Phobos & Deimos being D Types, very primitive). 2867 Steins is offering something very different. Also the asteroids record the history of their repective regions very well, depth of regolith, impact craters, boulders, etc. 2867 Steins will tell us very much. I am really looking forward to this actually & also only one month p[rior to MESSENGER's second Mercury encounter & a very close Cassini Enceladus encounter, not to mention that Phoenix on Mars should start detecting a change of season in the high northern latitude on Mars.
Once again mithridates, thank you so very much, you have made my day.
Your freind always,
Andrew Brown 3488.
Well, you're a veritable mine of information and never fail to enrich a thread so I'm willing to bet you're the favourite poster of a lot of the people there. Thanks for the extra information, as I don't know as much as I should about the difference between types of asteroids and you've reminded me of that.
It's nice to have these events to tide us over until the big event in 2015 (Dawn arriving at Ceres).
It appears that 2867 Steins is a very rare type of asteroid. Basalt rich ones like that are very rare. I wonder even, if 2867 Steins is actually a piece knocked off the giant asteroid 4 Vesta, that DAWN will survey first?
Any how, this is the first encounter with a very rare basalt asteroid & I am looking forward to it immensely.
Thank you again for your very kind comments about me & I will continueto post at SDC & also on here. This is a great blog you have here, lets hope others will chip in too.
I see you are in South Korea.
My Wife is from China, Zhanjiang City, Guangdong Province, just north of the island of Hainan, or two thirds of the way between Hong Kong & the border with Vietnam.
My email address: andrew.brown1969@btinternet.com
I have known you on SDC for some time now. I am very pleased that we have crossed paths.
Your freind, always.
Andrew Brown.
Thanks. I've always thought of subjects such as space, international auxiliary languages and the other ones I write about here as being closely related, as they all deal with progress, and the better communication / more peace / more economic growth the world has the easier it'll be to move into space permanently. As I suspected I'm getting a good amount of traffic to the blog, though considering all the subjects and languages it's extremely varied.
You might be interested in this page:
http://interlingua.planetology.org/
There's no new information there but it's an interesting example of how astronomical knowledge would look in an IAL, this one being Interlingua, one of the best for at-sight comprehension.
Yep, I know that area where your wife is from. Hainan's a big resort area. I've never been there but I've been as close as Taiwan. I see they now have regular flights between there and China too.
That reminds me, I don't suppose you know of a good source that shows how much help these flybys are in improving the accuracy of our observations from Earth? 2867 Steins is supposed to be around 2-5 km, and I assume after we have all the information from the flyby it'll be fed back into observations we have from here to make our estimations that much more accurate, but I have no idea by how much, and when we'll reach a point where we can make some really accurate guesses from Earth. I'm also curious about what the Vesta encounter will do for our observations of Ceres, once we've had a closeup look of an asteroid that massive. Basically I'm curious about whether we'll be able to get some better observations/estimates of Ceres before Dawn actually arrives, because 2015 still is a really long ways away and I hate waiting.
Hi Mithridates,
I wonder too if 4 Vesta will tell us anything about 1 Ceres. The two are very differnet, 4 Vesta is predominently basaly, huge chunk taken out of the south polar region as an enormous crater with a 13 KM high central mountain at the south pole (all gleaned from Hubble data), the rest of 4 Vesta appears reasonably spherical.
Perhaps Asteroid 2867 Steins is a chunk out of this crater?????
1 Ceres appears to be totally different, with hydrated minerals in the surface, possibly sub surface ice & maybe extinct cryovolcanoes, I suspect huge scarps are present as the interior cooled more slowlty than the crust, causing huge cliffs to form (maybe like Verona Rupes on the Uranus moon Miranda), also I suspect 1 Ceres may generally look like the Saturn moon Dione or the Uranus moon Ariel. Large number of impact craters I am sure are present also.
I will also push for a possible extended mission for DAWN to encounter the giant asteroid 2 Pallas, in a slow close flyby in December 2018, when 2 Pallas crosses the descending node in it's highly inclined solar orbit.
This plan involves an extended stay @ 1 Ceres, before departure as the distance between the pair decrease, so it's a great plan all around, but it is dependent on DAWN completing the primary mission at both 4 Vesta & 1 Ceres first.
Andrew Brown 3488.
Not long now, next Friday. Images of 2867 Steins should be available on Saturday. I just hope that ESA will release them at the post encounter briefing on Saturday 6th September 2008.
This will be very interesting, a basalt asteroid seen up close for the very first time. Some very good science will result from this encounter as well as some decent images. 2867 Steins is expected to be approx 340 pixels wide @ 15 metres per pixel resolution.
Will certainly be good enough to see the nature of this very rare type of asteroid.
I cannot wait.
Very interesting Autumn of events coming up with 2867 Steins being the first. Phoenix Mars Lander continues to send data from the high latitudes of Mars, change of season afoot there, Enceladus gets a very close brush past with Cassini & MESSENGER revisits the fascinating innermost planet Mercury.
Much to look forward to.
Andrew Brown 3488.
Hi mithridates,
The 2867 Steins encounter was very successful & a great deal of great data returned.
The only real disappointment was that the Narrow Angle Camera on Osiris went into Safe Mode Nine minutes prior to closest approach, but the other camera worked perfectly throughout & did take some wonderful images.
I cannot seem to post images on here, but I will say, that 2867 Steins was larger than expected, 5.9 KM longest axis by 4 KM through the poles.
The shape can only be described as a 'cut diamond' from one angle & triangular from another. A large 2.5 KM crater contains the North Pole & there is also a peculiar seven crater 'crater chain'.
There are many other craters as expected, but the asteroid is very angular, which seems to support my own theory that 2867 Steins could be a block knocked off from 4 Vesta, also the basaltic composition will also tend to make the asteroid 'blocky' in shape, exactly what Rosetta showed.
Will be interesting to compare the 2867 Steins spectra to that of 4 Vesta when NASA's DAWN arrives at the giant asteroid.
I have posted images on Space.com as you would expect.
Hope to see you soon, mithridates.
Andrew Brown 3488.
Thank you very much mithridates, I did not realise that I was your favourite poster over at SDC. I'm quite blown away.
You too are high in my list of favourites. Our interests are remarkably similar, that helps :)
Regarding the upcoming 2867 Steins, despite being no larger than some mountains on Earth, 2867 Steins has much of interest to offer. The spectra so far obtained suggests a basaltic makeup, not too different in composition to the Earth's mantle or the surface of Mercury. We have not yet encountered such an asteroid, mostly type S types so far with 253Mathilde being the only C type seen up close (perhaps the Mars Moons Phobos & Deimos being D Types, very primitive). 2867 Steins is offering something very different. Also the asteroids record the history of their repective regions very well, depth of regolith, impact craters, boulders, etc. 2867 Steins will tell us very much. I am really looking forward to this actually & also only one month p[rior to MESSENGER's second Mercury encounter & a very close Cassini Enceladus encounter, not to mention that Phoenix on Mars should start detecting a change of season in the high northern latitude on Mars.
Once again mithridates, thank you so very much, you have made my day.
Your freind always,
Andrew Brown 3488.
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