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

[dvandorn]

One reason Martian craters are hard to see from Earth-based telescopes is that, as with most cratered bodies, they aren't very obvious except near the terminator. And we very, very rarely see much in the way of a terminator on Mars. Most of the Mars views from Earth are nearly full-disk, the terminator fuzzed by being viewed through the maximum amount of Mars atmosphere it's possible to have between us and the Martian surface, and by foreshortening.

The human eye has far better naked-eye resolution of the Moon than we had of Mars through telescopes for hundreds of years, and even so, lunar craters weren't really identified as such until people started looking at the Moon through telescopes. And we get very good terminator views of the Moon from Earth. So, even if we were able to see Mars with a terminator crossing mid-disk through cratered terrain, it wouldn't be surprising if we missed craters...

-the other Doug