... This page contains some of the best images taken by Mars Pathfinder. ... Sojourner Gets Her Rock This "movie" was generated from 23 separate frames taken by the Imager for Mars Pathfinder (IMP) and lasts approximately 8 seconds. ... Sojourner is visible in this image, one of the first taken by the deployed Imager for Mars Pathfinder (IMP) on Sol 3. ... Yogi, a rock taller than rover Sojourner, is the subject of this image, taken by the deployed Imager for Mars Pathfinder (IMP) on Sol 3. ... Mars . ...

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• Titan Press Release

Sagan Memorial Station (Pathfinder) . This page contains some of the best images taken by Mars Pathfinder. ... Sojourner Gets Her Rock This "movie" was generated from 23 separate frames taken by the Imager for Mars Pathfinder (IMP) and lasts approximately 8 seconds. ... Sagan Memorial Station Images . ... Yogi Rock ( JPEG ) . Yogi, a rock taller than rover Sojourner, is the subject of this image, taken by the deployed Imager for Mars Pathfinder (IMP) on Sol 3. ... Couch Rock ( JPEG ) . ...

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• Pathfinder Images
• The Surface of Mars as Scene by Viking
• Titan Press Release

... This portrait of Yogi Rock, a now famous boulder on Mars, was recorded on Sol 3 by the Imager for Mars Pathfinder (IMP). ... During the 7 month cruise to Mars aboard the Pathfinder spacecraft, Sojourner measured only seven inches tall in a stowed position but prowling the martian landscape it has stretched to its full height of 1 foot (30 centimeters). ... The six wheeled robot rover Mars Sojourner rolled onto the martian surface on July 5th (Sol 2) at about 10:40 PM Pacific Daylight Time. ... July ...

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... July 24, 1997 . Mars Pathfinder's Landing Site . ... Explanation: Where is Mars Pathfinder ? ... From the surface Mars appears covered with rocks, but from orbit Mars appears covered with craters. ... These hills are about one kilometer from the landing site, twice the planned range of Sojourner . Two craters loom nearby: a small one to the east not easily visible here, and a big one to the south of Pathfinder. ... About APOD > . ...

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• APOD: October 10, 1997 - Mars Pathfinder Super Pan
• APOD: July 4, 1999 - A Landing On Mars
• APOD: 2011 June 16 - Mercury's Surface in Exaggerated Color

... Bad Astronomy . ... On Thursday, February 15th 2001 (and replayed on March 19), the Fox TV network aired a program called ``Conspiracy Theory: Did We Land on the Moon?'', hosted by X-Files actor Mitch Pileggi. ... Dust around the lander . ... However, it appeals to our common sense: when the sky is black here on Earth, we see stars. ... Bad: The program claims that when the top half of the lander took off from the Moon to bring the astronauts back into orbit, there was no flame from the rocket. ...

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• Phil Plait's Bad Astronomy: Bitesize Astronomy
• Are Apollo Moon Photos Fake?

... It?s needs solution satellite?s orientation problem for defining location of sources of ionospheric emissions above Earth?s surface with necessary accuracy. There is possibility to define orientation of photometric devices by using TV images of star background. The CCD TV camera is designed for recording of images of star sky, Earth? limb and adjoining part of Earth? surface to fix the orbit point coordinates during the measurements by FAGOT and SICH-F devices. ...

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... The lava flow has visibly fewer impact craters than the background terrain, illustrating the general principle that crater numbers can reveal ages of surfaces. ... Dating Small Martian Features . ... The crater-counting system that scientists have used since the 1970s to determine the age of large geologic features on Mars will also allow them to date small features, such as riverbeds and lava flows, according to William K. Hartmann, a senior scientist at the Tucson-based Planetary Science Institute...

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• ASP: Mercury Magazine
• ASP: The Little Twisters' Impact: Dust Devils on Mars
• ASP: Miranda: A Jigsaw Puzzle World

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Mopra radio telescope . ... The antenna surface extension project involves replacing the existing outer perforated panels with solid panels, giving 22 metre reflectors useable to beyond 100 GHz. ... Following the preliminary investigations outlined in the 1997 MNRF annual report (PDF file) , the ATNF has successfully carried out a specification, tendering and tender evaluation process....

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• Australia Telescope National Facility
• MNRF Parkes conversion system
• MNRF Surface extension project

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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• Lecture IV.
• Galaxy Gallery Page III

... Orbiter . Payload of the Orbiter . ... the instruments . ... ORBITER . Index . Instrument . Mass (kg) . ARGUS . ... visible and IR mapping spectrometer . ... planetary IR Fourier spectrometer . ... mapping visible and thermal radiometer . ... mapping high-resolut. spectrophotometer . ... multichannel optical s spectrometer . ... quadrupole mass-spectrometer . ... fast omnidir. energy-mass ion analyzer . ... wave complex . ... platform for ARGUS instruments . ... MASS-MEM . ...

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• Lidar homepage - Project news
• Spacecraft Digital Imaging Cameras
• Auroral Images

... 1971) --- Astronaut David R. Scott, commander, gives a military salute while standing beside the deployed United States flag during the Apollo 15 lunar surface extravehicular activity (EVA) at the Hadley-Apennine landing site. ... This photograph was taken by astronaut James B. Irwin, lunar module pilot. While astronauts Scott and Irwin descended in the LM to explore the moon, astronaut Alfred M. Worden, command module pilot, remained in lunar orbit in the Command and Service Module (CSM). ...

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• JSC Celebrates 40 Years
• as15-85-11514

Next: Basic Properties Up: R Coronae Borealis Stars Previous: Introduction . RCB stars are named after a star just visible to the naked eye in the constellation of Corona Borealis. RCrB was discovered by Edward Pigott, an English amateur astronomer, who had been observing a star in the `Northern Crown' for over a decade. ... Since 1795, other RCB stars have been discovered and their properties have been carefully observed. ...

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• HISTORICAL BACKGROUND
• Armagh Observatory
• Titania Ireland Mini-Campaign: Information and Documentation

... Edward L. (Ned) Wright received his AB and PhD degrees from Harvard University, and was a Junior Fellow in the Society of Fellows. ... Prof. Wright is interested in infrared astronomy and cosmology. ... He has been working on the COsmic Background Explorer ( COBE ) since 1978. ... Wright, E. L. 2000, ApJ submitted, "DIRBE Minus 2MASS: Confirming the Cosmic Infrared Background at 2.2 Microns" . ... The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background: II. ...

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• Telescope optics
• Fiber Input Model

... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . ... Astronomy for Kids . ... On the martian surface, would the moons Deimos and Phobos be visible to the unaided eye? ... Mars moons are easily visible at night from the surface of the Red Planet. ... From the Curiosity rover s point of view, on some evenings Phobos rises out of the slowly fading blue-gray twilight in crescent phase, transits as a quarter moon, and sets as a gibbous moon. ... Get instant access to subscriber content on Astronomy.com! ...

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• Bright planets meet at dusk | Astronomy.com
• Sojourner: lost and found | Astronomy.com

Главная Проекты Mars Exploration Rover . ... With far greater mobility than the 1997 Mars Pathfinder rover, these robotic explorers will be able to trek up to 100 meters (about 110 yards) across the surface in a Martian day. ... The rovers will be identical to each other, but will land at different regions of Mars. ... Where Pathfinder had scientific instruments on both the lander and the small Sojourner rover, these larger rovers will carry all their instruments with them. ...

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... Surface Brightness of Background Light . Home . ... Data . ... WFPC2 Home . ... Instrument Home . WFPC2 History . ... LRF Data . ... Data Analysis Home . ... Instrument Handbook . Data Handbook . ... Input the surface brightness in magnitudes per square arcsecond. ... Galaxy U-B and B-V colors are drawn from Longo and deVaucouleurs 1983 for representative objects;V-R and R-I are estimated from WFPC2 Handbook Table 6.1. ... AB_xxxxx are AB magnitudes at the standard WFPC2 filter bands. ...

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• Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
• Optical Distortion
• Surface Brightness Profiles

Электронная библиотека астронома-любителя. ... архив RSN . ... Апрель 1998 . ... Дата: 10 апреля 1998 (1998-04-10) От: Alexander Bondugin Тема: Galileo Update - April 9, 1998 Привет всем! ... Дата: 10 апреля 1998 (1998-04-10) От: Alexander Bondugin Тема: Mars Global Surveyor Update - April 9, 1998 Привет всем! ... The feature known as the "Face on Mars" in the Cydonia region was imaged quite successfully on April 5th and its image was released in raw form and in an enhanced form on April 6th. ...

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• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 01 июля
• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 27 марта

Журнал ПОВЕРХНОСТЬ публикует оригинальные статьи и обзоры по наиболее актуальным проблемам изучения поверхностных явлений. ... Редакция журнала 'Поверхность. ... Англоязычная версия журнала Journal of Surface Investigation . X-Ray, Synchrotron and Neutron Techniques выходит 6 раз в год . The Journal of Surface Investigation. X-ray, Synchrotron and Neutron Techniques ( Poverkhnost '. ... X-ray, Synchrotron and Neutron Techniques is abstracted and/or indexed in (Impact Factor 0.359): . ...

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• http://www.issp.ac.ru/iao/apao/2014/problems/pages01-02_ap14_t_en_a.pdf
• LSSS - Staff
• LEK - Info

Next: Particle Background Rejection Up: Detection Efficiency Previous: Front Illumination . ... The method requires that the CCD substrate be etched from the rear towards the depletion layer boundary. The device can be illuminated through this rear surface, which has a much thinner dead layer than the electrode side. ... The corresponding detection efficiency data are presented in Figure 7, and compared with the predicted data for a 20 m thick depletion layer. ...

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• Contrasting optical and X-ray applications
• rgsregions
• XMM-Newton Trainee Project 2004

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... des pages consacr?йes ?а la publication de vos photos Mais c'est aussi une vraie communaut?й avec laquelle partager votre passion et nourrir votre curiosit?й. Accueil Images de la com?иte Tempel 1 : le crat?иre de Deep Impact invisible . ... Les images rapproch?йes de la com?иte Tempel 1 prises par la sonde Stardust permettent de reconna?оtre la r?йgion o?? s'est ?йcras?й l'impacteur de Deep Impact en 2005. ... Etat du ciel . ...

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• La photo la plus pr?йcise de la surface du Soleil | Ciel et Espace
• Les ast?йro?пdes percutent Jupiter plus souvent que pr?йvu | Ciel et Espace
• Vid?йo : la surface solaire en plein bouillonnement | Ciel et Espace