Future Venus Missions Options

[Phil Stooke]

Oh well, might as well start that new topic since it's already well advanced in the Juno area...

My perspective on landers is as follows. All the landers we've had so far were dropped blind onto an essentially unknown surface. Any future landers can be targeted for specific terrains. It really is not true that we have had representative landings. Even a descent image or two, a panoramic photo plus a bit of surface composition, from a simple Venera-class lander just updated a bit, would be useful if we could put several down at well chosen targets. My choices would be:

Examples of the main plains units (smooth, fractured, ridged)

tesserae

high elevation radar-bright tesserae

large fresh lava flow unit ('fluctus')

crater dark parabola

crater ejecta outflow unit

dunes area.

And I have always assumed, rightly or wrongly, that it would be relatively easy to put these down, so they ought to be fairly inexpensive as planetary landers go.

Phil

[edstrick]

There was a full set of preliminary science papers from the Venus balloon experiments and I'm pretty sure a followup set of primary science results, published first <I think> in Science, then maybe in JGR <Journal of Geophysical Research, not sure which series>.

Regarding the whole craters on Mars surprise. Remember that essentially up to the Mariner 4 Mission, the best estimates for the martian surface pressure were around 1/10 th atmosphere, not 1/100 th. Improved precision spectroscopy had just shown a pretty solid measure of C02 surface pressure of 1/100 or 1/200 atmosphere, but nitrogen or argon were undetectable. The new figures had gotten attention, but not universal acceptance. So the whole vague arm-waving ideas of Martian geology were implicetly assuming a more active geology and surface environment.

We STILL were caught flat-footed. Sometimes EVERYBODY misses the obvious, including the people who didn't miss it but didn't keep screaming... "Hey.. this is important".