PPT-Spacecraft help us explore beyond Earth.

Before you learned The motions of planets and other nearby objects are visible from Earth Light and other forms of radiation carry information about the universe Now you will learn How astronauts explore space near Earth . Thermal balance and control.. Introduction [See F&S, Chapter 11]. We will look at how a spacecraft gets heated. How it might dissipate/generate heat. The reasons why you want a temperature stable environment within the spacecraft.. Space. Exosphere- starts at an altitude of 640 . kM. and reaches to 64,000 . kM.. The air gets progressively thinner and dwindles into nothingness. Everything above this layer is considered outer space . Dr Mark Price . (. mcp2@star.kent.ac.uk. ) , . Prof Mark Burchell (convener), Prof Richard Holdaway (CCLRC), Dr Vicky Fitzgerald.. Spring 2011.. Dr. Mark Price. Room 103C . E-mail: . mcp2@star.kent.ac.uk. . Spaceship . global cooperation . Name of the Team. :. Aliens023. Team members’ names. :. . Dejana. , Kristina. Coach’s name. :. . Tanja. . Radovanov. Spaceship. . A . spacecraft. (or . spaceship. Ritualistic Science. Frazer proponed that scientific inquiry [e.g. Astronomy] sprung from elements of rituals, religious doctrine/or philosophy, i.e. . human sacrifice . (Messianic Monotheism) and . dying gods . Dr. Mark Price – Spring 2011. An understanding of the way in which space missions are configured both from the point-of-view of the constituent subsystems, mission profile (i.e., the project aims) including the influence of the space environment.. 4412. Dynamics and Control of Space Vehicles. Mrinal Kumar, Assistant Prof.. Mechanical and Aerospace Engineering. SYLLABUS…. EAS 4510:. . Keplerian. Mechanics --- Considers motion of two . particles. . . Anyone who has watched auto racing on TV is aware of the Doppler shift. . As a race car approaches the camera, the sound of its engine increases in pitch (frequency). . After the car passes the camera, the pitch of its engine decreases. . Lecture. Sun Facts. Sun Facts. A ball of hot gases . Made up of. 70% hydrogen. 28% helium. 1.5% carbon, nitrogen, and oxygen, and . 0.5% all other elements . Temperature: 10,000 degrees Fahrenheit at the surface . The Moon. International Space Station. Geostationary Orbit. 35,000 feet = 6.62 miles. 50 miles. 250 miles .  400 km. 22,236 . miles. 363,000 to 405,000 km. (. approx. 240,000 miles). This is the distance at which satellites orbiting the Earth complete one orbit every 24 hours. . Jacob Schneider . David . Sibeck. Magnetosphere. Solar wind constantly collides with Earth’s magnetic field creating a cavity. Extends about 15-25 Earth radii in different directions. Protects life on earth from harmful radiation. This work is protected by U.S. copyright laws and is provided solely for the use of instructors in teaching their courses and assessing student learning. Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The work and materials from it should never be made available to students except by instructors using the accompanying text in their classes. All recipients of this work are expected to abide by these restrictions and to honor the intended pedagogical purposes and the needs of other instructors who rely on these materials.. PRESS KIT/AUGUST 2011Press KitMedia ContactsDwayne BrownPolicy/Program202-358-1726dwaynecbrownnasagov WashingtonDC Agle Juno Mission818-393-9011Jet PropulsionLaboratoryPasadena CalifMaria Martinez Sci @. AstroBioProf. Associate Professor. Observatory Director. George Mason University. NASA/JPL Solar System Ambassador. What’s Happening in Space:. Space Exploration by NASA. at the. Nature Foundation of Wintergreen.