... The predictive power of current models (the so-called meteor forecasting) has given us the exact timing of the Leonid storms of 2001 and 2002 to the nearest hour and are now used to predict the arrival times of major annual showers such as the Perseids . ... Towards this goal, the Observatory has installed a sky-monitoring system, consisting of one medium angle (MA) and two wide-angle (WA) video cameras linked to software designed to detect motion. ... Bright Taurid Meteor . ... Meteors on Mars . ...

GRANAT is the Russian x-ray sattelite launched to the high apogee orbit (200,000 km) and operated almost for 10 years (1989 -1999) , carrying out four major instruments: French SIGMA coded-mask hard x-ray telescope (30-1000 keV), Soviet ART-P coded-mask telescope (2??-60?? keV), all-sky monitor WATCH (6-150 keV), and a gamma-burst detector PHEBUS . ... Since September 1994, GRANAT is in the survey mode. ... Explore pages devoted to individual GRANAT instruments (including main scientific results): . ...

... Launch Date: 1970-11-10 . ... Luna 17 was launched from an earth parking orbit towards the Moon and entered lunar orbit on November 15, 1970. ... Lunokhod 1 was a lunar vehicle formed of a tub-like compartment with a large convex lid on eight independently powered wheels. Lunokhod was equipped with a cone-shaped antenna, a highly directional helical antenna, four television cameras, and special extendable devices to impact the lunar soil for soil density and mechanical property tests. ...

My wife and I received a Casio QV-300 digital camera as a wedding gift. ... Searching the web, we were able to find software called qvplay that enabled us to download the pictures onto our Sun. ... I could only get the lowest speed to work (about 60 seconds per picture), but it was adequate. ... I was excited about using the camera with the laptop, because the Sun only has 8-bit color, and an extremely lousy monitor. Copying pictures from the Sun to the laptop, sure enough they looked fantastic. ...

... Connecting the planned observations and the actual status of the Chandra X-ray Observatory is the observation interval determination pipeline ( OBIDET ). This collection of tools allows the Chandra X-Ray Center Data System automated processing to process the data through the necessary pipelines based on what was actually observed. ... In the case of the Chandra X-ray Observatory, the observation interval determination pipeline ( OBIDET ) is used for this task. ...

... Alta E6 Imaging area 1024 x 1024 array, 24 x 24 micron pixels (actual size) 1 MHz 16-bit digitization and 1.4 MHz 12-bit digitization to 24Mbyte camera memory 100bT Ethernet interface: up to 300 kHz throughput TCP/IP or UDP protocols DHCP or fixed IP addressing No plug in cards or external controllers Programmable , intelligent cooling to 50° C below ambient · Astronomy Binning up to 10 Horizontal x ... Pixel Binning Exposure Time Frame Sizes Cooling Dark Current (nom.) ...

. Album : asv-album :: Travels to distant places and countries :: 1997/08 Kyoto, Nara (Japan) :: 23/08 Ryoanji Temple and around . Up . << Prev . A bug which produces loud high-pitched noise. The actual length is about 5-6 cm. Next >> . Created with the tool album generator a MarginalHack by David on Tue Jun 23 14:46:19 2015 .

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

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... Р?С?С?С?Р?Р?Р?Р?РеС?Р?С?Р?РеР? ... Launched on February 17, 1996, the Near Earth Asteroid Rendezvous (NEAR) mission is to be the first of NASA's Discovery missions, a series of small-scale spacecraft designed to proceed from development to flight in under three years for a cost of less than $150 million. ... The ultimate goal of the mission is to rendezvous with and achieve orbit around the near Earth asteroid 433 Eros in February, 1999, and study the asteroid for approximately one year. ...