X-Andrew-Authenticated-as: 7997;andrew.cmu.edu;Ted Anderson
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In article <1990Nov13.104319.11134@irisa.fr>, hthomas@irisa.fr (Henry Thomas) writes:
|> In article <7034.273fd310@abo.fi>, mlindroos@abo.fi writes:
|> |> In article <1990Nov11.001924.10302@jato.jpl.nasa.gov>, baalke@mars.jpl.nasa.gov (Ron Baalke) writes:
[deleted]
|> |> 30 minutes! Why can't we send an advanced long-life, Viking-style probe
|> |> to Titan instead?! The Viking lander was "only" about twice as heavy as the
|> |> Huygens probe will be so the lack of a powerful-enough launcher surely cannot
|> |> be the reason? Is this just because of financial considerations again, or...?
|>
|> The reason is maybe that we have NO data of the condition down there:
|> - Is there any *solid* ground ?
|> - pressure ?
|> - temperature ?
|> So with no information, it seems difficult to design a long-life probe.
|> A similar(?) problem occured on Venus, where the probes Venera 11-14 lasted only a few hours. The first ones didn't reached the ground because theirs parachutes where destroyed by the acid atmosphere.
|> On mars, the informations where much more complete, because the ground had been observed by many orbital probes: it was visible.
|>
|> There was an excellent article in the ESA journal (?), some month ago about "Cassini Probe Huygens Entry techniques" .
|>
Here are some excerpts from this article
ESA Journal 1989, vol 13 pp 175--190 "Cassini/Huygens Entry and Descent Technologies" G Scoon, G, Whitcomb, M Eiden, A. Smith
"The main objectives of the probe's mission will be the determination of the chemical composition of the atmosphere and the measurement of winds and temperature and pressure profiles from an altitude of 170 km down to the surface" ... " Althoug