Maped visuals of planets.

Part seventeen show detailed maps of mars as they become available to all using mars maps. It will show every inch of this stunning terrain as new images of Mars for centuries' ‘Grand

Canyon’ have been captured in 3D by the European Space Agency’s (ESA’s) Mars Express.The deep valley, named Hebes Chasma, is a strange 196-mile (315km) scar that sits almost right in the middle of the Martian equator on the northern edge of the Valles Marineris canyon.It is an enclosed, almost 8 km-deep trough stretching 315 km in an east–west direction and 125 km from north to south at its widest point. Mars in 3D: Stunning images reveal red planet's 'Grand Canyon' in unprecedented detail - and provide clues to its volcanic beginnings. 
Hebes Chasma is a 196-mile scar that sits close to the Martian equator. Origin is associated with tectonic shifts from the volcanic Tharsis Region. The debris that fills the canyon floor shows that enormous landslides also played a key role in shaping. The deep valley, named Hebes Chasma, is a strange 196-mile (315km) scar that sits almost right in the middle of the Martian equator on the northern edge of the Valles Marineris canyon. Layers with Carbonate Content Inside McLaughlin Crater on Mars This view of layered rocks on the floor of McLaughlin Crater shows sedimentary rocks that contain spectroscopic evidence for minerals formed through interaction with water.

Here is an example of space garden below, so when water misbehaves its amazing this reveals how super-high temperatures cause droplets to travel uphill in even small carved indents.This is because of something known as the 'Leidenfrost Effect'. The effect causes the water to levitate on the evaporated gas vapour . Movement can be changed by adjusting the surface texture and temperature. The skittering of water occurs because a surface is about twice as hot as the liquid's boiling point. 
This causes the water to levitate on the evaporated gas vapour which acts a barrier that keeps the droplet and the hot surface separated. Researchers at Bath University have found that water droplets can be made to climb up a steep incline using the Leidenfrost effect – the sharper the teeth of the surface, the steeper incline they were able to climb The Leidenfrost Maze guides water droplets in different directions using specially-arranged grooved hotplates Here is an example of a flat shuttle interpreted version of the a concorde.

Numerous grooves are etched into the mountain, suggesting the material is weak and easily eroded  A similar feature is visible at the opposite end of the mound, as seen in the full-colour image. Other landslide deposits are seen all over the floor of Hebes Chasma, many coming from the main canyon walls.The canyon walls and the mesa feature a number of grooves, suggesting the material is weak and easily eroded.In another image, a band of darker material is seen between two layers of light material. 

It also make a lot of sense to use robotic aerial platforms to explore other planets in our solar system, and in the case of Mars, a rocket powered airplane although rely on satellites these should be able to deploy looking cave structures with small metal round ball, called investigative insects could be put out to give an optimum configuration. With this type of mission, we could bridge the gap between small "local" scale measurements of lander and rovers and large "global" scale measurements of orbiters. By covering hundreds of kilometers in a short amount of time, an airplane could obtain a whole new class of atmospheric and geological data from Mars. Just think about the way airplanes have changed the way we live on Earth, and you can start to understand how they could revolutionize our exploration of other planets.