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1984Best.-Nr. 011296Washington D.C.: U.S. Government Printing Office 1984 317 numbered pp.; HB. Pages: clean bright tight off-white eps; no defects. Cover: green reverse artwork front reverse titles front/spine; minimal shelfwear mild bump head. Includes: Aseroids Comets and Planet Formation; Mercury; Venus; Earth; Moon; and Mars. Includes maps of each terrestrial planet. Edited by Michael H. Carr. U.S. Government Printing Office hardcover
2009Best.-Nr. 67232Moffett FIeld CA: United States National Aeronautics and Space Administration 2009. Reprint. Second Printing. Wraps. Very good. Includes: illustrations diagrams. Various paginations approximately 125 pages. References. From Wikipedia: "The Stratospheric Observatory for Infrared Astronomy SOFIA is a joint project of NASA and the German Aerospace Center DLR to construct and maintain an airborne observatory. NASA awarded the contract for the development of the aircraft operation of the observatory and management of the American part of the project to the Universities Space Research Association USRA in 1996. The DSI Deutsches SOFIA Institut manages the German parts of the project which are primarily science and telescope related. SOFIA's telescope saw first light on May 26 2010. SOFIA is the successor to the Kuiper Airborne Observatory.SOFIA is based on a Boeing 747SP wide-body aircraft that has been modified to include a large door in the aft fuselage that can be opened in flight to allow a 2.5 meter diameter reflecting telescope access to the sky. This telescope is designed for infrared astronomy observations in the stratosphere at altitudes of about 41 000 feet about 12 km. SOFIA's flight capability allows it to rise above almost all of the water vapor in the Earth's atmosphere which blocks some infrared wavelengths from reaching the ground. At the aircraft's cruising altitude 85% of the full infrared range will be available. The aircraft can also travel to almost any point on the Earth's surface allowing observation from the northern and southern hemispheres. Once ready for use the expectation is for observing flights to be flown 3 or 4 nights a week for the next 20 years. SOFIA is now based at NASA's Dryden Aircraft Operations Facility at LA/Palmdale Regional Airport California while staff at NASA Ames Research Center in Mountain View California operate the SOFIA Science Center where astronomical observation missions are planned for the flying observatory. The NASA logo reflected in SOFIAs 2.5-meter primary mirror. SOFIA uses a 2.5-meter reflector telescope which has an oversized 2.7 meter diameter primary mirror as is common with most large infrared telescopes. The optical system uses a Cassegrain reflector design with a parabolic primary mirror and a remotely configurable hyperbolic secondary. In order to fit the telescope into the fuselage the primary is shaped to an f-number as low as 1.3 while the resulting optical layout has an f-number of 19.7. A flat tertiary dichroic mirror is used to deflect the infrared part of the beam to the Nasmyth focus where it can be analyzed. An optical mirror located behind the tertiary mirror is used for a camera guidance system. The telescope looks out of a large door in the side of the fuselage near the airplane's tail and will initially carry nine instruments for infrared astronomy at wavelengths from 1 655 micrometres and high-speed optical astronomy at wavelengths from 0.3 1.1 micrometres. The main instruments are the FLITECAM a near infrared camera covering 1 5 micrometres; FORCAST covering the mid-infrared range of 5 40 micrometres and HAWC which spans the far infrared in the range 42 210 micrometres. The other four instruments include an optical photometer and infrared spectrometers with various spectral ranges. SOFIA s telescope is by far the largest ever to be placed in an aircraft. For each mission one interchangeable science instrument will be attached to the telescope. Two groups of general purpose instruments are available. In addition an investigator can also design and build a special purpose instrument. On April 17 2012 two upgrades to HAWC were selected by NASA to increase the field of view with new detector arrays and to add the capability of measuring the polarization of dust emission from celestial sources. The open cavity housing the telescope will be exposed to high-speed turbulent winds. In addition the vibrations and motions of the aircraft introduce observing difficulties. The telescope was designed to be very lightweight with a honeycomb shape milled into the back of the mirror and polymer composite material used for the telescope. United States, National Aeronautics and Space Administration paperback
