blog:articles:general:martian_weird_spring
Differences
This shows you the differences between two versions of the page.
Both sides previous revisionPrevious revision | Next revisionBoth sides next revision | ||
blog:articles:general:martian_weird_spring [2019/07/22 18:23] – [Southern Hemisphere] Phil Ide | blog:articles:general:martian_weird_spring [2019/07/22 18:23] – [Southern Hemisphere] Phil Ide | ||
---|---|---|---|
Line 440: | Line 440: | ||
Hellas Planitia, an incredibly large and deep impact basin in the southern hemisphere, is so deep that air pressure in its lowest areas is sufficient to sustain liquid water. At the moment, nearly all our experiments we've sent to the Martian surface, have landed in the northern hemisphere. The Curiosity rover is an exception to this, but it is wandering around inside Gale Crater, just south of the equator and only a few hundred kilometres from InSight. It will be very interesting to get on-sight weather data from deeper in the southern hemisphere, which we'll surely do as our ability to land on much more [[: | Hellas Planitia, an incredibly large and deep impact basin in the southern hemisphere, is so deep that air pressure in its lowest areas is sufficient to sustain liquid water. At the moment, nearly all our experiments we've sent to the Martian surface, have landed in the northern hemisphere. The Curiosity rover is an exception to this, but it is wandering around inside Gale Crater, just south of the equator and only a few hundred kilometres from InSight. It will be very interesting to get on-sight weather data from deeper in the southern hemisphere, which we'll surely do as our ability to land on much more [[: | ||
- | //images courtesy of Mars24, a freeware program | + | //images courtesy of [[https:// |
~~socialite~~ | ~~socialite~~ | ||
~~DISCUSSION~~ | ~~DISCUSSION~~ |