Mars is puzzle . From rover and artificial satellite observations we sleep together that it once had quite a little of water on its surface , which normally suggests quick and wet conditions . On the other hand , evidence suggests the planet was always pretty chilly , even in the upstage past , but it ’s not a cold , dry desert either . These two idea are often at betting odds , but fresh enquiry suggest that they could both be true : ancient Mars was potential a frigid world both cold and soaked .
Researchers set out to make a model that can explain the perplexing features witnessed on the Red Planet . If the planet was n’t warm and plastered or cold and dry could there be a third option ? put out their findings inProceedings of the National Academy of Sciences , they believe that their cold and wet scenario can explain the cosmos of a vast swimming sea in the Northern Hemisphere of Mars , extending to its icy region .
However , the model call for to explain both the presence of a swimming ocean and ice - capped regions , like thepresence of glacial valleysand ice sheet in the southern highlands .
Planetary scientist studying Mars have found evidence ofancient tsunamisthat rocked the Red Planet . If the sea was frozen due to a very stale clime , these tsunami would not have hap . But a milder climate would have meant transferring piss from the sea to the land through precipitation . Cold and stiff condition , however , could have survive .
The team used an advanced universal circulation model to process out the necessary parametric quantity for this earthly concern . They calculated it was possible for an sea to be stable even if the mean temperature of Mars was below 0 ° nose candy ( 32 ° F ) , the freezing point of water , 3 billion years ago . They envisioned ice - covered plateaus in the south with glacier flowing across the plains and returning to the ocean . Rainfall would have been temperate around the shoreline . In this scenario , the sea surface could be up to 4.5 ° deoxycytidine monophosphate ( 40 ° F ) ; not tropical but enough for water to stay liquid .
The key to these conditions is all in the melody . The atmosphere of Mars today is about 1 per centum in density compare to Earth ’s own . But , if in the yesteryear it was roughly the same and was made of about 10 per centum atomic number 1 and the rest carbon dioxide , this scenario would in reality make . Previous analyses have retrieve strong evidence fora thick atmospherebefore it was ripped from the planet by the steady stream of particles from the Sun .
The framework is for certain compelling in explain the peculiarities of Mars , but of course , much more grounds is demand to understand what the Red Planet was really like billions of years ago .