What is the longitude of Mars?

Latitude and longitude coordinates are: 40.696518, -80.010857. Mars is a very small town located near Pittsburgh, the state of Pennsylvania, USA….Mars, PA, USA Lat Long Coordinates Info.

Country	United States
Longitude	-80.010857
DMS Lat	40° 41′ 47.4648” N
DMS Long	80° 0′ 39.0852” W
UTM Easting	583,569.47

Is Mars fully mapped?

Nearly 90\% of Mars’ surface has been mapped by the high-resolution stereo camera on ESA’s Mars Express, which celebrates ten years since launch this June.

What are the geographic features of Mars?

Its surface is rocky, with canyons, volcanoes, dry lake beds and craters all over it. Red dust covers most of its surface. Mars has clouds and wind just like Earth. Sometimes the wind blows the red dust into a dust storm.

Does Mars have a prime meridian?

Airy-0 is a crater inside the larger Airy Crater on Mars, whose location defined the position of the prime meridian of that planet. It is about 0.5 km (0.3 mile) across and lies within the dark region Sinus Meridiani, one of the early albedo features to be identified on Mars.

How is a point on Mars defined?

For Mars, the prime meridian was first defined by the German astronomers W. Beer and J. H. M dler in 1830-32. They used a small circular feature, which they designated ‘a,’ as a reference point to determine the rotation period of the planet.

Did Mars have continents?

There are differences, of course: Mars can support higher mountains because it has less gravity, and it overed with a thick layer of dust. Mars has continents, Pollack continued, it must have geological activity, too.

What are Earth’s galactic coordinates?

The Earth is on the galactic plane, so we are at 0o latitude. Instead of going from 0o to 180o east and 180o west, galactic coordinates simply go from 0o to 360o. There is no east/west or plus/minus in galactic longitude coordinates. 360o is the same as 2 x 180o, or 180o is half of 360o.

Does Mars have tectonic plates?

Mars, however, doesn’t have plate tectonics. After its formation, the planet was a searing mass of molten rock that eventually cooled to form a static crust around a rocky mantle, yet it’s unclear how hot the planet’s insides are today.