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Super Typhoon Fengshen
Title Super Typhoon Fengshen
Description With sustained winds at 145 knots (167 miles per hour), Super Typhoon Fengshen reached Category 5 hurricane status?the most severe hurricane status?on Friday, July 19, 2002. This image was acquired by the Moderate Resolution Imaging Spectroradiometer (MODIS) on Monday, July 22, 2002, when the super typhoon was several hundred miles east of Iwo Jima at the southern tip of Kyushu, Japan. The storm is churning the sea into 35-foot waves, and winds have been gusting up to 170 knots (196 miles per hour). In this image, the storm occupies a rectangle roughly 1000 kilometers wide and 1150 kilometers tall. If the western side of this storm were aligned with Nashville, Tennessee, it would cover the United States all the way east to the Atlantic Ocean, as far north as Akron, Ohio, and as far south as the Georgia-Florida border. Fengshen has been tracking northwestward over the past 24 hours, and is expected to weaken only slightly as it makes its way toward Japan, which is still recovering from floods and wind damage caused by Typhoons Chataan and Halong, which hit the country the previous week. Please note that the high-resolution scene provided here is 500 meters per pixel. For a copy of the scene at the sensor's fullest resolution, visit the MODIS Rapid Response Image Gallery. Image courtesy Jacques Descloitres, MODIS Land Rapid Response Team at NASA GSFC
Super Typhoon Fengshen
Title Super Typhoon Fengshen
Description With sustained winds at 145 knots (167 miles per hour), Super Typhoon Fengshen reached Category 5 hurricane status?the most severe hurricane status?on Friday, July 19, 2002. This image was acquired by the Moderate Resolution Imaging Spectroradiometer (MODIS) on Monday, July 22, 2002, when the super typhoon was several hundred miles east of Iwo Jima at the southern tip of Kyushu, Japan. The storm is churning the sea into 35-foot waves, and winds have been gusting up to 170 knots (196 miles per hour). In this image, the storm occupies a rectangle roughly 1000 kilometers wide and 1150 kilometers tall. If the western side of this storm were aligned with Nashville, Tennessee, it would cover the United States all the way east to the Atlantic Ocean, as far north as Akron, Ohio, and as far south as the Georgia-Florida border. Fengshen has been tracking northwestward over the past 24 hours, and is expected to weaken only slightly as it makes its way toward Japan, which is still recovering from floods and wind damage caused by Typhoons Chataan and Halong, which hit the country the previous week. Please note that the high-resolution scene provided here is 500 meters per pixel. For a copy of the scene at the sensor's fullest resolution, visit the MODIS Rapid Response Image Gallery. Image courtesy Jacques Descloitres, MODIS Land Rapid Response Team at NASA GSFC
Nashville Four Planet Skylin …
Title Nashville Four Planet Skyline
Explanation So far this February, evening skies [ http://antwrp.gsfc.nasa.gov/apod/ap000504.html ] have been blessed with a glorious Moon and three bright planets, Venus [ http://www.library.utoronto.ca/utel/rp/poems/ longfe10.html ], Jupiter, and Saturn. But just last week, on January 30th, an extreme wide-angle lens allowed astrophotographer Larry Koehn to capture this twilight view of Moon and four planets above [ http://www.seds.org/nineplanets/nineplanets/ see.html ] Nashville, Tennessee, USA. These major solar system [ http://space.jpl.nasa.gov/ ] bodies lie along the ecliptic plane [ http://antwrp.gsfc.nasa.gov/apod/ap001014.html ] and so follow a diagonal line through the picture. Starting near the upper left corner is bright Jupiter [ http://starchild.gsfc.nasa.gov/docs/StarChild/ solar_system_level2/jupiter.html ], which takes on a slightly triangular shape due to the lens distortion. Just below and right of Jupiter is Saturn [ http://www.jpl.nasa.gov/cassini/english/kids/ saturn_in_sky.html ]. Continuing along the diagonal toward the lower right is an overexposed, six day old Moon [ http://www.inconstantmoon.com/ ] and brilliant Venus seemingly embedded in clouds. The fourth planet pictured is Mercury. Notoriously hard to see from planet Earth because it never wanders far from the Sun, Mercury is [ http://antwrp.gsfc.nasa.gov/apod/ap991111.html ] visible just above the lower right corner. The line from Jupiter to Mercury spans about 92 degrees across the Nashville sky.
Moon, Mars, Venus, and Spica
Title Moon, Mars, Venus, and Spica
Explanation Gliding toward today's total eclipse [ http://sunearth.gsfc.nasa.gov/ eclipse/TSE2002/TSE2002.html ] of the Sun, the crescent Moon has been rising early, just before dawn. And as a prelude to its close solar alignment [ http://www.mreclipse.com/ Special/SEprimer.html ], the Moon also completed a lovely celestial triangle, closing with bright planets Mars and Venus [ http://antwrp.gsfc.nasa.gov/apod/ap020524.html ] on the morning of December 1. While [ http://antwrp.gsfc.nasa.gov/apod/ap021203.html ] the total solar eclipse can only [ http://profjohn.com/el/el2002/index.html ] be seen [ http://www.csiro.au/helix/eclipse/ ] from a [ http://astronomy.swin.edu.au/solar_eclipse_2002/ ] narrow corridor, skygazers around the globe could appreciate this [ http://www.spaceweather.com/planets/ gallery_01dec02.html ] lunar-planetary conjunction. This view is from near Nashville Tennessee, USA, and finds brilliant Venus at the lowest corner of the triangle with a much fainter Mars immediately to the right of the Moon. The Moon's sunlit crescent is overexposed, but details of the lunar night side are revealed by earthshine [ http://antwrp.gsfc.nasa.gov/apod/ap020419.html ]. Above and to the right of the trio is Spica [ http://www.astro.wisc.edu/~dolan/constellations/ hr/5056.html ], brightest star in the constellation Virgo.
A Sun Halo Over Tennessee
Title A Sun Halo Over Tennessee
Explanation Sometimes it looks like the Sun is being viewed through a large lens [ http://www.opticalres.com/kidoptx.html ]. In the above case, however, there are actually millions of lenses: ice crystals [ http://www.sundog.clara.co.uk/halo/crystals.htm ]. As water freezes in the upper atmosphere [ http://csep10.phys.utk.edu/astr161/lect/earth/atmosphere.html ], small, flat, six-sided, ice crystals might be formed. As these crystals [ http://www.its.caltech.edu/~atomic/snowcrystals/primer/primer.htm ] flutter to the ground, each crystal [ http://cst-www.nrl.navy.mil/lattice/ ] can act like a miniature lens, refracting sunlight into our view. The above image [ http://www.vydor.net/gallery/Nature/vydor_sun_halo_shrunk ] was taken near sunset last month near Nashville, Tennessee [ http://www.state.tn.us/ ], USA [ http://www.cia.gov/cia/publications/factbook/geos/us.html ]. Dramatically visible [ http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/halo.html ] behind neighborhood houses and trees and above the cloud deck is the 22 degree halo [ http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/halo22.html ] created by sunlight refracting [ http://www.sundog.clara.co.uk/halo/spole.htm ] off of atmospheric ice crystals.
Super Typhoon Fengshen: Natu …
nasa, nasanaturalhazards
With sustained winds at 145 …
Fengshen.TMO2002203
mediatype IMAGE
mediatype image
date 2002-07-22
creator NASA -- NASA Image Of The Day
identifier Fengshen.TMO2002203
Super Typhoon Fengshen: Natu …
nasa, nasanaturalhazards
With sustained winds at 145 …
Fengshen.TMO2002203
mediatype IMAGE
mediatype image
date 2002-07-22
creator NASA -- NASA Image Of The Day
identifier Fengshen.TMO2002203
Hubble-V
PIA04222
Wide Field Planetary Camera …
Title Hubble-V
Original Caption Released with Image Resembling curling flames from a campfire, a magnificent nebula in a nearby galaxy observed by NASA's Hubble Space Telescope provides new insight into the fierce birth of stars as it may have occurred in the early universe. The picture, taken by Hubble's Wide Field and Planetary Camera 2, is online at http://heritage.stsci.edu and http://oposite.stsci.edu/pubinfo/pr/2001/39 and http://www.jpl.nasa.gov/images/wfpc . The camera was designed and built by NASA's Jet Propulsion Laboratory, Pasadena, Calif. The glowing gas cloud, called Hubble-V, has a diameter of about 200 light-years. A faint tail of gas and dust trailing off the top of the image sits opposite a dense cluster of bright stars at the bottom of the irregularly shaped nebula. Hubble's resolution and ultraviolet sensitivity reveal a dense knot of dozens of ultra-hot stars nestled in the nebula. Each star glows 100,000 times brighter than our Sun. These 4-million-year-old stars, considered youthful in the cosmic time scale, are too distant and crowded together to be resolved from ground-based telescopes. The small, irregular host galaxy, called NGC 6822, is one of the Milky Way's closest neighbors. It lies 1.6 million light-years away in the direction of the constellation Sagittarius. The Hubble-V image data was taken by two science teams: C. Robert O'Dell of Vanderbilt University, Nashville, Tenn. and collaborators, and Luciana Bianchi of Johns Hopkins University, Baltimore, Md., and Osservatorio Astronomico, Torinese, Italy, and collaborators. This color image was produced by the Hubble Heritage Team at the Space Telescope Science Institute, Baltimore, Md. The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract with the Goddard Space Flight Center, Greenbelt, Md. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. JPL is a division of the California Institute of Technology in Pasadena. Additional information about the Hubble Space Telescope is available at http://hubble.stsci.edu. More information about the Wide Field and Planetary Camera 2 is available at http://wfpc2.jpl.nasa.gov
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