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Scientists Solve the Mystery of Methane in Titan's Atmosphere |
| Guest_AlexBlackwell_* |
Mar 1 2006, 07:07 PM
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Scientists Solve the Mystery of Methane in Titan's Atmosphere
By Lori Stiles, UANews.org March 1, 2006 Scientists Solve the Mystery of Methane in Titan's Atmosphere By Lori Stiles, UANews.org March 1, 2006 This refers to the Tobie et al. paper in the March 2, 2006, issue of Nature. |
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Mar 2 2006, 12:55 AM
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![]() Senior Member ![]() ![]() ![]() ![]() Group: Moderator Posts: 3242 Joined: 11-February 04 From: Tucson, AZ Member No.: 23 |
We may have at least a preliminary answer to one of their test very soon thanks to Monday's Titan pass that included some Radio Science doppler experiments. From the paper:
"If a subsurface ammonia–water ocean and a rocky core are present, as predicted by our model, Titan's tidal secondary potential Love number k2 should be higher than 0.3 and its moment of inertia factor C/MR2 should be lower than 0.33; these quantities should be measured by the Radio Science Subsystem later in the mission" -------------------- &@^^!% Jim! I'm a geologist, not a physicist!
The Gish Bar Times - A Blog all about Jupiter's Moon Io |
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| Guest_AlexBlackwell_* |
Mar 2 2006, 01:00 AM
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#3
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We may have at least a preliminary answer to one of their test very soon thanks to Monday's Titan pass that included some Radio Science doppler experiments. From the paper: "If a subsurface ammonia–water ocean and a rocky core are present, as predicted by our model, Titan's tidal secondary potential Love number k2 should be higher than 0.3 and its moment of inertia factor C/MR2 should be lower than 0.33; these quantities should be measured by the Radio Science Subsystem later in the mission" It's possible but very tough with just the T11 data. I think RSS won't be comfortable with a Love number until all the gravity data come in (i.e., T22, T33, and T38). |
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Mar 2 2006, 01:03 AM
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#4
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![]() Senior Member ![]() ![]() ![]() ![]() Group: Moderator Posts: 3242 Joined: 11-February 04 From: Tucson, AZ Member No.: 23 |
It's possible but very tough with just the T11 data. I think RSS won't be comfortable with a Love number until all the gravity data come in (i.e., T22, T33, and T38). It makes wonder though if they could at least place some constraints with just the T11 data. they may not have a number they are comfortable with, I perfectly understand that. -------------------- &@^^!% Jim! I'm a geologist, not a physicist!
The Gish Bar Times - A Blog all about Jupiter's Moon Io |
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| Guest_AlexBlackwell_* |
Mar 2 2006, 01:12 AM
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#5
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It makes wonder though if they could at least place some constraints with just the T11 data. they may not have a number they are comfortable with, I perfectly understand that. Yes, my understanding is that the stand-alone T11 gravity data can give a rough, first-order estimate for k2, perhaps enough for hypothesis testing. On the other hand, T11 by itself should give pretty good estimates for the other gravity coefficients: GM, C20, and C22. |
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| Guest_AlexBlackwell_* |
Mar 3 2006, 05:19 PM
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#6
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Yes, my understanding is that the stand-alone T11 gravity data can give a rough, first-order estimate for k2, perhaps enough for hypothesis testing. On the other hand, T11 by itself should give pretty good estimates for the other gravity coefficients: GM, C20, and C22. From the Cassini Significant Events Report for for 02/23/06 - 03/01/06: QUOTE The focus then shifted to the Radio Science Subsystem (RSS). This was the first of four coordinated gravity field passes - the others occurring in T22, T33, and T38 - to determine the low degree coefficients of Titan's gravity field. This knowledge may help to answer the question of whether Titan possesses an internal ocean. The four passes require disparate geometries: two of these flybys must occur when Titan is near periapse along its orbit around Saturn and two flybys - of which T11 was one - must occur when Titan is close to its apoapse. For each of these two pairs, one flyby must be on a nearly equatorial orbit with respect to Titan as was T11, and the other on an orbit with an inclination as large as possible. Radio Science also had two Gravity Science Enhancement (GSE) passes occurring after the flyby. The GSE passes are crucial to de-correlate Titan's mass from the distance at closest approach. I guess this is why I'm a little hesitant about even a rough, first order estimate for Titan's Love number based on one flyby. On the other hand, maybe, as you suggest, some constraints on k2 could be placed, unless the number RSS generates is really flaky. We'll see. |
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AlexBlackwell Scientists Solve the Mystery of Methane in Titan's Atmosphere Mar 1 2006, 07:07 PM
BruceMoomaw Judging from the LPSC abstracts, Tobie's is ac... Mar 1 2006, 11:45 PM
The Messenger QUOTE (BruceMoomaw @ Mar 1 2006, 04:45 PM... Mar 2 2006, 03:55 PM
AlexBlackwell QUOTE (The Messenger @ Mar 2 2006, 03:55 ... Mar 2 2006, 04:35 PM
The Messenger QUOTE (AlexBlackwell @ Mar 2 2006, 09:35 ... Mar 2 2006, 07:13 PM
AlexBlackwell QUOTE (The Messenger @ Mar 2 2006, 07:13 ... Mar 2 2006, 11:04 PM
hendric QUOTE (AlexBlackwell @ Mar 1 2006, 07:12 ... Mar 2 2006, 04:19 AM
remcook a start...
http://www.spenvis.oma.be/spenvis/ecss... Mar 2 2006, 01:40 PM![]() ![]() |
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