<p>That map of Mars is a composite of <em>many</em> different images that were taken at different times during Mars' year.  Mars' arctic circles are very similar to Earth's, and during that hemisphere's winter, that terrain is in permanent shadow, allowing seasonal frost to form.</p>
<p>Even though Hellas is equatorward of the antarctic circle, it gets cold enough, days are short enough, and it is low enough in elevation so the atmosphere is thick enough to allow seasonal frost to form on Hellas.  It is highly variable year-to-year, but it typically covers much of the floor of Hellas.</p>
<p>So, what you are seeing in the first map is southern summer and northern summer for the poles (or probably late spring given the extent of the south polar ice), and then very early spring near Hellas.  I would guess that those were the best images they could find from Viking to make that particular mosaic.</p>
<p>That is in contrast with the 2nd picture, which probably better matched seasons for a more smooth mosaic and one that better represents late spring / early summer at most pixels.</p>

CC BY-SA 4.0
2021-04-06T00:33:29.970Z
2021-04-06T07:49:38.827Z
2021-04-06T07:49:38.827Z
Stuart Robbins
<p>One map of Mars I see a lot is this colourized map: the Viking colourized global mosaic (<a href="https://astrogeology.usgs.gov/search/map/Mars/Viking/MDIM21/Mars_Viking_MDIM21_ClrMosaic_global_232m" rel="nofollow noreferrer">Source</a>):</p>
<p><a href="https://i.sstatic.net/Wt96Q.jpg" rel="nofollow noreferrer"><img src="https://i.sstatic.net/Wt96Q.jpg" alt="Mars Viking Colorized Global Mosaic v2" /></a></p>
<p>But one thing which strikes me as odd is just how white the Hellas Basin is (the white patch which is not on the poles, just in the middle of the lower right half of the above image)</p>
<p>On the older version of the Viking mosaic, the basin doesn't look that white. Here the <em>Mars Viking Colorized Global Mosaic v1</em>
(<a href="https://astrogeology.usgs.gov/search/map/Mars/Viking/Color/Mars_Viking_ClrMosaic_global_925m" rel="nofollow noreferrer">Source</a>, <a href="https://astropedia.astrogeology.usgs.gov/download/Mars/Viking/Color/thumbs/Mars_Viking_ClrMosaic_global_1024.jpg" rel="nofollow noreferrer">link to image</a>):</p>
<p><a href="https://i.sstatic.net/WFO7O.jpg" rel="nofollow noreferrer"><img src="https://i.sstatic.net/WFO7O.jpg" alt="Screenshot of the Image" /></a></p>
<p>It certainly still looks at least paler than the surrounding areas, but nowhere near as much as on the first map (on the first map it is about as white as the poles, on the second it is not).</p>
<p>So: Is the Hellas basin <em>really</em> as white as the first map suggests? And if yes why?</p>

CC BY-SA 4.0
2020-06-09T19:02:50.070Z
Could simply be clouds. Hellas basin is the lowest point on Mars, so cloud formation will be most efficient there through accumulation of water vapour, depending on the martian seasons.
AtmosphericPrisonEscape
<mars>
Why does Hellas Basin look white on some maps?
Nikolaj
# Why does Hellas Basin look white on some maps?

(Asked by: username_0 on 2020-06-09)

One map of Mars I see a lot is this colourized map: the Viking colourized global mosaic ([Source](https://astrogeology.usgs.gov/search/map/Mars/Viking/MDIM21/Mars_Viking_MDIM21_ClrMosaic_global_232m)):

[![Mars Viking Colorized Global Mosaic v2](https://i.sstatic.net/Wt96Q.jpg)](https://i.sstatic.net/Wt96Q.jpg)

But one thing which strikes me as odd is just how white the Hellas Basin is (the white patch which is not on the poles, just in the middle of the lower right half of the above image)

On the older version of the Viking mosaic, the basin doesn't look that white. Here the *Mars Viking Colorized Global Mosaic v1*
([Source](https://astrogeology.usgs.gov/search/map/Mars/Viking/Color/Mars_Viking_ClrMosaic_global_925m), [link to image](https://astropedia.astrogeology.usgs.gov/download/Mars/Viking/Color/thumbs/Mars_Viking_ClrMosaic_global_1024.jpg)):

[![Screenshot of the Image](https://i.sstatic.net/WFO7O.jpg)](https://i.sstatic.net/WFO7O.jpg)

It certainly still looks at least paler than the surrounding areas, but nowhere near as much as on the first map (on the first map it is about as white as the poles, on the second it is not).

So: Is the Hellas basin *really* as white as the first map suggests? And if yes why?

**Tags:** mars

> **Comments:**
> **username_1**: Could simply be clouds. Hellas basin is the lowest point on Mars, so cloud formation will be most efficient there through accumulation of water vapour, depending on the martian seasons.  

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## 1 answers

### Answer by username_2 on 2021-04-06. Score: 1

That map of Mars is a composite of *many* different images that were taken at different times during Mars' year. Mars' arctic circles are very similar to Earth's, and during that hemisphere's winter, that terrain is in permanent shadow, allowing seasonal frost to form.

Even though Hellas is equatorward of the antarctic circle, it gets cold enough, days are short enough, and it is low enough in elevation so the atmosphere is thick enough to allow seasonal frost to form on Hellas. It is highly variable year-to-year, but it typically covers much of the floor of Hellas.

So, what you are seeing in the first map is southern summer and northern summer for the poles (or probably late spring given the extent of the south polar ice), and then very early spring near Hellas. I would guess that those were the best images they could find from Viking to make that particular mosaic.

That is in contrast with the 2nd picture, which probably better matched seasons for a more smooth mosaic and one that better represents late spring / early summer at most pixels.


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