é |
é |
![]() |
. |
. |
, |
. |
![]() |
Starwatchers Picture of the Week Aurora Watch |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
Tru News Helpful Hints BPE T&E Mars BPE T&E Starwatch BPE T&E Egypt BPE T&E Meds |
My Album Fairies & Fantasies Loving Rusti's Corner Thought for Today Winter at Home |
Astronomy with Tru set by true masked wabbit |
![]() |
image by Ben Nicholson, Armstrong, British Columbia, CanadaMar. 18 |
March 29 2006 |
NASA Shares Solar Eclipse With the World nasa |
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
Star Map for April with Zoom click and pan until desired location |
NASA prepares for Space Exploration in Undersea Lab |
During the mission, called the NASA Extreme Environment Mission Operations (NEEMO) project, new long-distance medical techniques that could help keep spacefarers healthy will be practiced. Doctors thousands of miles away will guide aquanauts as they perform surgeries on a patient simulator. Doctors also will remotely control robotic instruments to do the work. The procedures simulated in Aquarius may one day be used to respond to emergencies on the International Space Station, the moon or Mars. [Read More] |
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ |
![]() |
NASA gave people a front row seat to today's total solar eclipse, thanks to a partnership with the University of California at Berkeley and the Exploratorium. A streaming webcast brought the eclipse -- visible along a path from South America to Africa to Asia -- to schools and museums and computer desktops worldwide. |
Wallpaper for your desktop by cosmic_castaway |
for more wallpaper got to Hubble Picture Gallery |
Wallpaper for your desktop by cosmic_castaway right click on pic above and save target as then set as background |
On 13 Mar 2006 there were 773 known Potentially Hazardous Asteroids March 2006 Earth-asteroid encounters |
Potentially Hazardous Asteroids (PHAs) are space rocks larger than approximately 100m that can come closer to Earth than 0.05 AU. None of the known PHAs is on a collision course with our planet, although astronomers are finding new ones all the time. |
![]() |
By request from some of you who regularly come to the Star Watch site I have returned the message link to leave a message. I sincerely thank you for your patronage |
ASTEROID DATE(UT) MISS DISTANCE MAG. SIZE(meters) 2000 PN9 March 6 7.9 LD 12 ~2 km 2006 EH1 March 7 2.0 LD 18 ~20 m 2006 EC March 8 0.7 LD 16 ~19 m |
Notes: LD is a "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU. MAG is the visual magnitude of the asteroid on the date of closest approach. |
![]() |
![]() |
![]() |
![]() |
The eclipse coverage was part of Sun-Earth Day, celebrated every year to help everyone better understand how our sun interacts with the Earth and other planets in the solar system. This year's theme, "Eclipse: In a Different Light" shows how eclipses have inspired people to observe and understand the Sun-Earth-Moon system. |
Image above: The sun's corona, or outer atmosphere, is visible during totality -- when the sun is totally obscured by the moon's shadow. Credit: NASA TV |
![]() |
NASA and Libyan scientists also conducted joint scientific activities in Libya to observe and study the event. . A total solar eclipse is very rare because all parts of this puzzle must line up correctly in order for it to occur. The moon must be in its new phase for a solar eclipse to take place. The moon's shadow has two parts—a central region called the umbra and an outer region called the penumbra. The part of the moon’s shadow which passes over you determines what kind of eclipse you will see. |
Image above: Left: The sun creates a "diamond ring" effect as it emerges after totality. Right: Solar flares, or "prominences" are visible at the edge of the moon's shadow. Credit: NASA TV |
![]() |
Image above: Left: The moon's shadow falls on Earth, as seen from the International Space Station 230 miles above. Expedition 13, the next space station crew, launches from Kazakhstan tonight |
This eclipse's path begins in Brazil and extends across the Atlantic Ocean, Northern Africa, and Central Asia where it ends at sunset in Northern Mongolia. A partial eclipse path, within the much broader path of the moon's penumbral shadow, includes the northern two thirds of Africa, Europe, and Central Asia. In a total eclipse like this one, the entire central portion of the Sun is blocked out. The sky darkens as though it is nighttime and -- for the only time -- you can see the Sun’s corona, or outer atmosphere. Total solar eclipses are of special interest to astronomers because it's the only time they can study the corona. Scientists still don't understand why the corona is so hot. Its temperature is 1 to 2 million degrees Fahrenheit while the Sun's bright surface is only 10,000° F. Careful measurements and experiments made during a total eclipse can help to unravel this enigma.This year's eclipse is also special because the total phase lasts over 4 minutes at the center of the path. This is quite long for a total solar eclipse since most last just a minute or two. The next total eclipse,on August 1, 2008, will be seen in northern Canada, Greenland, Siberia, Mongolia and northern China. It will last about 2 minutes. The next total eclipse visible from the United States won’t happen until August 21, 2017. |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
|
||||||||
. |