'Martian atmosphere' presentation slideshows

MARS

MARS. 3.934 g/cm 3. Similar to Earth. Viewing Mars. Earth-based observations of Mars are best made during favorable oppositions. The best Earth-based views of Mars are obtained when Mars is simultaneously at opposition and near perihelion. Earth-based Observations.

622 views • 45 slides

22.033 Final Design Presentation

22.033 Final Design Presentation. Vasek Dostal Knut Gezelius Jack Horng John Koser Joe Palaia Eugene Shwageraus And Pete Yarsky With the Help of Kalina Galabova Nilchiani Roshanak Dr. Kadak. Outline. Mission plan Space power system Surface power system Conclusions Future Work.

487 views • 42 slides

MHP SSG Atmosphere Focus Team

MHP SSG Atmosphere Focus Team. A Hazard Assessment from 11 Mars Atmospheric Scientists. W. Farrell NASA/GSFC Meteorological and Electrical Processes S. Rafkin SWRI Middle Atmosphere Dynamics S. Fuerstenau JPL Aeolian Electrostatic Processes

498 views • 37 slides

World of Robotics

World of Robotics. What is Robotics/A.I ?. Robotics is the study of the design, construction and use of robots.

508 views • 36 slides

Obstacles

Obstacles. Long Distance Long Duration Supplies Reliability Space Environment Known Effects on Humans Radiation Planetary Environment Martian Atmosphere Martian Surface.

437 views • 32 slides

Obstacles

Obstacles. Long Distance Long Duration Supplies Reliability Space Environment Known Effects on Humans Radiation Planetary Environment Martian Atmosphere Martian Surface.

331 views • 32 slides

SESSION 8

411 views • 28 slides

Mars Exploration

Mars Exploration. By Jacob Stinar. Water on Mars. Past, Present, and Future Missions to Mars. early on most missions to Mars failed 25 missions from 1960-1970 only 17 missions since. http://www.impactlab.com/wp-content/uploads/2009/10/Mars-mission-graphic.jpg.

1.05k views • 21 slides

Zou Ziming 1 Ma Wenzhen Li Lei Zhao Hua Wang Chi 1: mzou@cssar.ac

332 views • 17 slides

Terrestrial Planets Earth, Mercury, Venus, Mars

Terrestrial Planets Earth, Mercury, Venus, Mars. Objectives. Standards. (1a) Students know how the differences and similarities among the sun, the terrestrial planets, and the gas planets may have been established during the formation of the solar system.

625 views • 12 slides

Mars: some basics

203 views • 11 slides

The Terrestrial Planets

223 views • 8 slides

Team A Presentation One Dynamics and Control

Team A Presentation One Dynamics and Control. Anne DeLion 16 January 2001. Departure. Direct Launch Less propellant use. Simpler than launch to low Earth orbit (LEO) Launch to LEO Costs more propellant More Complex. Arrival at Mars. Direct Descent

56 views • 5 slides

Buried Carbonates at Mars

Buried Carbonates at Mars. Infrared observations from spacecraft orbiting Mars are used to determine the composition of minerals on the surface Impacts expose material previously buried below the surface

210 views • 4 slides

Methane in the Martian Atmosphere

46 views • 4 slides

Buried Carbonates at Mars

Buried Carbonates at Mars. Infrared observations from spacecraft orbiting Mars are used to determine the composition of minerals on the surface Impacts expose material previously buried below the surface

59 views • 4 slides