Video :: Common Performs in Chicago

Here’s footage of Common performing at Chicago’s Moet Rose Lounge.

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    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: May 19, 2005NASA’s launch team readied the shuttle Discovery today for a second fueling test Friday to help find the cause of two vexing problems that cropped up during a similar test in April. Other shuttle engineers, meanwhile, are assessing a clearance issue between the shuttle’s main Ku-band TV antenna and a new on-orbit inspection boom that could delay the transmission of post-launch images of the ship’s redesigned external tank.As part of NASA’s post-Columbia safety upgrade program, a 50-foot-longboom equipped with a television camera and laser sensors was installed onthe right, or starboard, side of Discovery’s cargo bay. The boom, picked upby the shuttle’s robot arm in orbit, will be used to inspect Discovery’swing leading edge panels and heat shield tiles for any signs of launchimpact damage.The Orbiter Boom Sensor System is located on the right wall of the shuttle’s payload bay. 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The currently-installed bipod heaters will be on for partof the test and then turned off to find out whether the heaters influencethe operation of the pressure relief valve.Here is a tanking test timeline (all times in EDT):May 1908:00 p.m….Rotating service structure retraction11:30 p.m….Final loading preps begin May 2002:30 a.m….Pad cleared of personnel04:00 a.m….Mission management team meets for go/no-go decision04:30 a.m….Begin a 1-hour built-in hold05:30 a.m….Resume countdown05:30 a.m….Begin propellant line chilldown (fueling begins)08:30 a.m….Fueling complete; stable replenish mode begins08:30 a.m….Begin a 1-hour 45-minute built-in hold10:15 a.m….Resume countdown with bipod heater on01:35 p.m….Countdown is stopped at T-minus 31-second mark01:35 p.m….Recycle countdown to T-minus 20-minute mark01:45 p.m….Resume countdown with bipod heater off02:45 p.m….Final cutoff at T-minus 31-second mark02:45 p.m….Begin propellant drain back and boiloff May 2103:00 p.m….Rotating service structure moved back around shuttleThe launch team plans to test fire one of Discovery’s three auxiliarypower units, which generates the ship’s hydraulic power, on May 23. 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    Posted: October 22, 2008T-00:00LiftoffThe Delta 2 rocket’s main engine and twin vernier steering thrusters are started moments before launch. The four strap-on solid rocket motors are ignited at T-0 to begin the mission.T+01:04.0SRB BurnoutThe ground-start Alliant TechSystems-built solid rocket motors consume all their propellant and burn out.T+01:22.5Jettison SRBsThe spent solid rocket boosters are jettisoned to fall into the Pacific Ocean. The spent casings remained attached until the vehicle passed into preset drop zone, clear of offshore oil platforms.T+01:25.0Begin Dog-legAfter initially flying from Vandenberg along a 196-degree flight azimuth, the rocket begins steering itself to obtain the desired orbital inclination. This dog-leg maneuver continues for 35 seconds.T+04:24.0Main Engine CutoffAfter consuming its RP-1 fuel and liquid oxygen, the Pratt & Whitney Rocketdyne RS-27A first stage main engine is shut down. The vernier engines cut off moments later.T+04:32.0Stage SeparationThe Delta rocket’s first stage is separated now, having completed its job. The spent stage will fall into the Pacific Ocean.T+04:37.5Second Stage IgnitionWith the stage jettisoned, the rocket’s second stage takes over. The Aerojet AJ118-K liquid-fueled engine ignites for the first of two firings needed to place the COSMO 3 spacecraft into the proper orbit.T+04:41.5Jettison Payload FairingThe 10-foot diameter payload fairing that protected the COSMO 3 cargo atop the Delta 2 during the atmospheric ascent is jettisoned is two halves.T+11:25.1Second Stage Cutoff 1The second stage engine shuts down to complete its first firing of the launch. The rocket and attached spacecraft are now in a long coast period before the second stage reignites. The orbit achieved should be 348 nautical miles at apogee, 100 miles at perigee and inclined 97.8 degrees.T+53:27.0Second Stage RestartDelta’s second stage engine reignites for a short firing to raise the orbit’s perigee.T+53:39.4Second Stage Cutoff 2The second stage shuts down after a 12-second burn. The orbit achieved should be 341.0 nautical miles at apogee, 334.7 miles at perigee and inclined 97.86 degrees.T+58:00.0Payload SeparationThe Italian COSMO-SkyMed radar Earth-imaging satellite is released from the Delta 2 rocket, completing the launch.Data source: ULA.John Glenn Mission PatchFree shipping to U.S. addresses!The historic first orbital flight by an American is marked by this commemorative patch for John Glenn and Friendship 7.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is available in our store. Get this piece of history!Celebrate the shuttle programFree shipping to U.S. addresses!This special commemorative patch marks the retirement of NASA’s Space Shuttle Program. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia’s historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard’s historic Mercury mission with this collectors’ item, the official commemorative embroidered patch.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Delta 338 launch timelineSPACEFLIGHT NOW

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    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: October 26, 2004TIME (EDT)..IMAGES….RESOLUTION (miles/pixel)…………NAC/WAC…NAC/WAC…..EVENT/OBSERVATION TYPE10/2502:30 p.m…………………….Begin approach observations01:14 p.m…………………….Begin medium resolution observations10/2607:44 a.m…………………….Begin high resolution observations10:56 a.m…………………….Transition to thruster control11:17 a.m…………………….Turn HGA toward Titan11:29 a.m…………………….Begin inbound RADAR scatterometry11:59 a.m…………………….Turn cameras back to Titan12:32 p.m…………………….Turn INMS/HGA to Titan ram direction12:38 p.m…………………….Begin INMS atmospheric collection12:44 p.m…………………….Titan closest approach12:44 p.m…………………….Begin high-res RADAR/SAR imaging12:50 p.m…………………….Begin low-res RADAR/SAR imaging01:00 p.m…………………….Begin RADAR altimetry01:14 p.m…………………….Begin outbound RADAR scatterometry01:59 p.m…………………….Transition to reaction wheel control02:07 p.m…………………….Ascending ring plane crossing02:23 p.m…………………….Begin RADAR radiometry09:15 p.m…………………….Turn to Earthline09:40 p.m…………………….Begin A5 data playback (CRITICAL)09:41 p.m…10/00…..1.7/16.8….ISS: Low resolution09:43 p.m…00/14…..1.3/13……ISS10:10 p.m…63/06…..1.2/11.8….ISS10:25 p.m…00/07…..0.87/8.7….ISS11:15 p.m…12/36…..0.37/3.7….ISS: Medium resolution10/2712:23 a.m…87/01…..0.25/2.5….ISS: Regional map12:51 a.m…87/01…..0.13/1.3….ISS: High resolution01:44 a.m…………………….Begin A4 playback science/engineering01:56 a.m…………………….Begin B4 playback02:28 a.m…23/23…..0.11/1.1….ISS: RADRCS02:32 a.m…………………….ISS: Waypoint turn02:40 a.m…18/29…..17’/755’….ISS: Highest resolution (17 ft/pixel)05:04 a.m…32/43…..0.62/6.2….ISS: Ultraviolet05:29 a.m…………………….Begin B4 playback science/engineering05:30 a.m…………………….Begin A5 data playback (CRITICAL)05:31 a.m…………………….Resume B4 playback05:22 a.m…………………….END TA playback07:33 a.m…………………….Saturn closest approach05:13 p.m…………………….Descending ring plane crossing | | | | 2014 Spaceflight Now Inc.Fresh crater on Rhea? CASSINI PHOTO RELEASEPosted: January 4, 2004Rhea has been heavily bombarded by impacts during its history. In this Cassini image the moon displays what may be a relatively fresh, bright, rayed crater near Rhea’s eastern limb. Rhea is 1,528 kilometers (949 miles) across. Credit: NASA/JPL/Space Science InstituteDownload larger image version This view is centered on the side of Rhea that faces away from Saturn as the moon orbits. The image was taken in visible light with the Cassini spacecraft narrow angle camera on Nov. 10, 2004, at a distance of 3.6 million kilometers (2.2 million miles) from Rhea and at a Sun-Rhea-spacecraft, or phase, angle of 86 degrees. North is up. The image scale is 21 kilometers (13 miles) per pixel. The image has been magnified by a factor of two and contrast enhanced to aid visibility of surface features. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.From Saturn’s dark side CASSINI PHOTO RELEASEPosted: December 11, 2004As Cassini swung around to the dark side of the planet during its first close passage after orbit insertion, the intrepid spacecraft spied three ring moons whizzing around the planet. Visible in this image are: Mimas (398 kilometers, or 247 miles across) brightest and above center; Janus (181 kilometers, or 112 miles across) second brightest at upper left; and Prometheus (102 kilometers, or 63 miles across) just above the main rings at upper left. Credit: NASA/JPL/Space Science InstituteDownload larger image version The normally bright B ring appears very dark from this vantage point. Regions with smaller concentrations of particles, such as the Cassini division (bright near center) transmit more sunlight and thus are brighter. The image was taken in visible light with the Cassini spacecraft wide angle camera at a distance of 757,000 kilometers (470,000miles) from Saturn. The image scale is about 42 kilometers (26 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Saturn’s ring gap CASSINI PHOTO RELEASEPosted: December 2, 2004An intriguing knotted ringlet within the Encke Gap is the main attraction in this Cassini image. The Encke Gap is a small division near the outer edge of Saturn’s rings that is about 300 kilometers (190 miles) wide. The tiny moon Pan (20 kilometers, or 12 miles across) orbits within the gap and maintains it. Many waves produced by orbiting moons are visible. Credit: NASA/JPL/Space Science InstituteDownload larger image version The image was taken in visible light with the Cassini spacecraft narrow angle camera on Oct. 29, 2004, at a distance of about 807,000 kilometers (501,000 miles) from Saturn. The image scale is 4.5 kilometers (2.8 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Getting closer to Titan CASSINI PHOTO RELEASEPosted: June 25, 2004 Credit: NASA/JPL/Space Science InstituteDownload larger image version Irregular bright and dark regions of yet unidentified composition and character are becoming increasingly visible on Titan’s surface as Cassini approaches its scheduled first flyby of Saturn’s largest moon on July 2, 2004.This view represents an improvement in resolution of nearly three times over the previous Cassini images of Titan. Titan’s surface is difficult to study, veiled by a dense hydrocarbon haze that forms in the high stratosphere as methane is destroyed by sunlight. This image is different from previous Titan images by Cassini because it was taken through a special filter, called a polarizer, which is designed to see through the atmosphere to the surface. The superimposed coordinate system grid in the accompanying image at right illustrates the geographical regions of the moon that are illuminated and visible, as well as the orientation of Titan. North is up and rotated 25 degrees to the left. The yellow curve marks the position of the boundary between day and night on Titan. This image shows about one quarter of Titan’s surface, from 0 to 70 degrees West longitude, and just barely overlaps part of the surface shown in the previous Titan image release. Most of the visible surface in this image has not yet been shown in any Cassini image. The image was obtained with the narrow angle camera on June 14, 2004, at a phase, or Sun-Titan-spacecraft, angle of 61 degrees and at a distance of 10.4 million kilometers (6.5 million miles) from Titan. The image scale is 62 kilometers (39 miles) per pixel. The image was magnified by a factor of two using a linear interpolation scheme. No further processing to remove the effects of the overlying atmosphere has been performed. The observed brightness variations are real, on scales of one hundred kilometers or less. The image was obtained in the near-infrared (centered at 938 nanometers) through a polarizing filter. The combination was designed to reduce the obscuration by atmospheric haze. The haze is more transparent at 938 nanometers than at shorter wavelengths, and light of 938 nanometers wavelength is not absorbed by methane gas in Titan’s atmosphere. Light at this wavelength consequently samples the surface, and the polarizer blocks out light scattered mainly by the haze. This is similar to the way a polarizer, put on the front of a lens of a hand-held camera, makes distant objects more clear on Earth. Cassini will conduct a critical 96-minute burn before going into orbit around Saturn on June 30 (July 1 Universal Time), with its first scheduled flyby of Titan on July 2.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Giant landslide on Iapetus CASSINI PHOTO RELEASEPosted: January 9, 2004A spectacular landslide within the low-brightness region of Iapetus’s surface known as Cassini Regio is visible in this image from Cassini. Iapetus is one of the moons of Saturn. Credit: NASA/JPL/Space Science InstituteDownload larger image version The landslide material appears to have collapsed from a scarp 15 kilometers high (9 miles) that forms the rim of an ancient 600 kilometer (375 mile) impact basin. Unconsolidated rubble from the landslide extends halfway across a conspicuous, 120-kilometer diameter (75-mile) flat-floored impact crater that lies just inside the basin scarp. Landslides are common geological phenomena on many planetary bodies, including Earth and Mars. The appearance of this landslide on an icy satellite with low-brightness cratered terrain is reminiscent of landslide features that were observed during NASA’s Galileo mission on the Jovian satellite Callisto. The fact that the Iapetus landslide traveled many kilometers from the basin scarp could indicate that the surface material is very fine-grained, and perhaps was fluffed by mechanical forces that allowed the landslide debris to flow extended distances. In this view, north is to the left of the picture and solar illumination is from the bottom of the frame. The image was obtained in visible light with the Cassini spacecraft narrow angle camera on Dec. 31, 2004, at a distance of about 123,400 kilometers (76,677 miles) from Iapetus and at a Sun-Iapetus-spacecraft, or phase, angle of 78 degrees. Resolution achieved in the original image was 740 meters (2,428 feet) per pixel. The image has been contrast-enhanced and magnified by a factor of two to aid visibility. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Hazy all over Titan CASSINI PHOTO RELEASEPosted: July 28, 2004Following its first flyby of Titan, Cassini gazed back at the smog-enshrouded moon’s receding crescent. This natural color view was seen by the spacecraft about one day after closest approach. The slight bluish glow of Titan’s haze is visible along the limb. Credit: NASA/JPL/Space Science InstituteDownload a larger version of image The superimposed coordinate system grid in the accompanying image at right illustrates the geographical regions of the moon that are illuminated and visible, as well as the orientation of Titan — lines of longitude converge on the South Pole near the moon’s eastern limb. The yellow curve marks the position of the boundary between day and night on Titan. Images taken through blue, green and red filters were combined to create this natural color view. The images were obtained with the Cassini spacecraft wide angle camera on July 3, 2004, from a distance of about 790,000 kilometers (491,000 miles) from Titan and at a Sun-Titan-spacecraft, or phase angle of 115 degrees. The image scale is 47 kilometers (29 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Herding the Saturn’s rings CASSINI PHOTO RELEASEPosted: September 26, 2004 Saturn’s moon Prometheus is seen shepherding the inner edge of Saturn’s F ring. Prometheus is 102 kilometers (63 miles) across and was captured in a close-up view by the Cassini spacecraft near the time of orbital insertion at Saturn. A number of clumps are visible here along the arcing F ring. Credit: NASA/JPL/Space Science InstituteDownload larger image version The image was taken with the Cassini spacecraft narrow angle camera at a distance of 8.2 million kilometers (5.1 million miles) from Saturn through a filter sensitive to visible green light. The image scale is 49 kilometers (33 miles) per pixel. Contrast was slightly enhanced to aid visibility. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Hovering over Titan CASSINI PHOTO RELEASEPosted: November 24, 2004A mosaic of nine processed images recently acquired during Cassini’s first very close flyby of Saturn’s moon Titan on Oct. 26, 2004, constitutes the most detailed full-disc view of the mysterious moon. Credit: NASA/JPL/Space Science InstituteDownload larger image version The view is centered on 15 degrees South latitude, and 156 degrees West longitude. Brightness variations across the surface and bright clouds near the south pole are easily seen. The images that comprise the mosaic have been processed to reduce the effects of the atmosphere and to sharpen surface features. The mosaic has been trimmed to show only the illuminated surface and not the atmosphere above the edge of the moon. The Sun was behind Cassini so nearly the full disc is illuminated. Pixels scales of the composite images vary from 2 to 4 kilometers per pixel (1.2 to 2.5 miles per pixel). Surface features are best seen near the center of the disc, where the spacecraft is looking directly downwards; the contrast becomes progressively lower and surface features become fuzzier towards the outside, where the spacecraft is peering through haze, a circumstance that washes out surface features. The brighter region on the right side and equatorial region is named Xanadu Regio. Scientists are actively debating what processes may have created the bizarre surface brightness patterns seen here. The images hint at a young surface with, no obvious craters. However, the exact nature of that activity, whether tectonic, wind-blown, fluvial, marine, or volcanic is still to be determined. The images comprising this mosaic were acquired from distances ranging from 650,000 kilometers (400,000 miles) to 300,000 kilometers (200,000 miles). The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Cassini posterJust in time for the Cassini spacecraft’s arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12×12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA’s Mars Exploration Rover is now available from the Astronomy Now Store.Columbia ReportThe official accident investigation report into the loss of the space shuttle Columbia and its crew of seven. Includes CD-ROM. Choose your store: | | | | 2014 Spaceflight Now Inc.Huygens carrier signal ‘solid’ for more than two hours BY WILLIAM HARWOOD

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