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Description Here on the Gallery page you can find the very latest images, videos and products from the Cassini-Huygens mission to Saturn, including the spectacular launch, spacecraft assembly and the exciting trip to Saturn.
Full Description There were two flybys of Venus in Cassini's primary trajectory, on April 26, 1998 and June 24, 1999. This image shows the spacecraft near the cloud-enshrouded Venus. By David Seal (only available electronically).
Olympus Mons, 1998
title Olympus Mons, 1998
date 04.25.1998
description Olympus Mons is a mountain of mystery. Taller than three Mount Everests and about as wide as the entire Hawaiian Island chain, this giant volcano is nearly as flat as a pancake. That is, its flanks typically only slope 20 to 50. The Mars Orbiter Camera (MOC) obtained this spectacular wide-angle view of Olympus Mons on Mars Global Surveyor's 263rd orbit, around 10:40 p.m. PDT on April 25, 1998. In the view presented here, north is to the left and east is up. The spacecraft was traveling from north to south (left to right). Although the camera looks straight down (towards the nadir) and cannot be pointed to the side, the wide angle camera has such a large field of view (it sees from horizon to horizon) that, in effect, it provides side looking views. Unlike some other MOC images, that have had to be warped to provide a view as if seen from a certain direction and altitude, this image shows what the camera saw without additional processing. It is easy to imagine that you are looking out a window at the surface of Mars from about 900 km (560 miles) up. The image was taken on a cool, crisp winter morning. The west side of the volcano (lower portion of view, above) was clear and details on the surface appear very sharp. The skies above the plains to the east of Olympus Mons (upper portion of view) were cloudy. Clouds were lapping against the lower east flanks of this 26 kilometers (16 miles) high volcano, but the summit skies were clear. When Mars Global Surveyor attains its Mapping Orbit in March 1999, the MOC wide angle camera system will be used to make daily, global maps of martian clouds and weather systems. The wide angle images will resemble weather satellite pictures of Earth, and will help the Mars science teams plan their observations and test computer-driven Mars weather prediction models. Malin Space Science Systems and the California Institute of Technology built the MOC using spare hardware from the Mars Observer mission. MSSS operates the camera from its facilities in San Diego, CA. The Jet Propulsion Laboratory's Mars Surveyor Operations Project operates the Mars Global Surveyor spacecraft with its industrial partner, Lockheed Martin Astronautics, from facilities in Pasadena, CA and Denver, CO. Image Note: This color picture was made using MOC red wide angle image 26301 and blue wide angle image 26302. The green channel was synthesized by averaging the red and blue bands. Color is not the true color of Mars as it would appear to the human eye (the actual colors would be more pale and contrast more subdued) *Image Credit*: NASA/JPL/Malin Space Science Systems
Borrelly's Rugged Surface
title Borrelly's Rugged Surface
date 09.22.2001
description In this highest resolution view of the icy, rocky nucleus of comet Borrelly, (about 45 meters or 150 feet per pixel) a variety of terrains and surface textures, mountains and fault structures, and darkened material are visible over the nucleus's surface. This was the final image of the nucleus of comet Borrelly, taken just 160 seconds before Deep Space 1's closest approach to it. This image shows the 8-km (5-mile) long nucleus about 3417 kilometers (over 2,000 miles) away. Smooth, rolling plains containing brighter regions are present in the middle of the nucleus and seem to be the source of dust jets seen in the coma. The rugged land found at both ends of the nucleus has many high ridges along the jagged line between day and night on the comet. This rough terrain contains very dark patches that appear to be elevated compared to surrounding areas. In some places the dark material accentuates grooves and apparent faults. Stereo analysis shows the smaller end of the nucleus (lower right) is tipped toward the viewer (out of frame). Sunlight is coming from the bottom of the frame. Deep Space 1 completed its primary mission testing ion propulsion and 11 other advanced, high-risk technologies in September 1999. NASA extended the mission, taking advantage of the ion propulsion and other systems to undertake this chancy but exciting, and ultimately successful, encounter with the comet. More information can be found on the Deep Space 1 home page at http://nmp.jpl.nasa.gov/ds1/. Deep Space 1 was launched in October 1998 as part of NASA's New Millennium Program, which is managed by JPL for NASA's Office of Space Science, Washington, D.C. The California Institute of Technology manages JPL for NASA. *Image Credit*: NASA/JPL
Lunar Prospector in Clean Ro …
Title Lunar Prospector in Clean Room
Full Description The fully assembled Lunar Prospector spacecraft is shown mated atop the Star 37 Trans Lunar Injection module. Lunar Prospector represented the first NASA spacecraft to revisit the Moon in 25 years. In December of 1972 Apollo 17 astronauts Gene Cernan and Harrison Schmitt were the last humans to set foot upon the Moon and the last NASA mission to visit the lunar frontier. On January 6, 1998 at 9:28 p.m., Lunar Prospector was launched from Cape Canaveral, Florida aboard a Lockheed Martin Athena II rocket. Also onboard were the ash remains of astrogeologist Eugene M. Shoemaker. A scientist from the U.S. Geological Survey, he was detailed to NASA and helped train Apollo astronauts in lunar geology. However, as co- founder of a "rogue string" of comet fragments, his name will forever be linked to the much hearlded Shoemaker-Levy 9 cometary impact of the planet Jupiter in 1995. Lunar Prospector mapped the Moon's elemental composition, gravity fields, magnetic fields and resources. Prospector provided insights into the origin and evolution of the Moon. One of the most significant finds by Lunar Prospector was confirmation that there could be as much as 10 billion tons of subsurface frozen water near the Moon's polar region. The Lunar Prospector mission came to a creative and daring conclusion when on July 31, 1999 at 2:52:00.8 a.m. PDT Mission Control Ames directed the spacecraft to a crash landing into a deep crater near the Moon's South pole. The hope was that the impact might release trapped water vapor. However no visible debris plume was detected by numerous observatories monitoring the event. This lack of direct evidence has not diminished the hope or belief that subsurface frozen water does exist.
Date 01/01/1997
NASA Center Ames Research Center
Mars Climate Orbiter
Title Mars Climate Orbiter
Full Description The Mars Surveyor '98 Climate Orbiter is shown here during acoustic tests that simulate launch conditions. The orbiter was to conduct a two year primary mission to profile the Martian atmosphere and map the surface. To carry out these scientific objectives, the spacecraft carried a rebuilt version of the pressure modulated infrared radiometer, lost with the Mars Observer spacecraft, and a miniaturized dual camera system the size of a pair of binoculars, provided by Malin Space Science Systems, Inc., San Diego, California. During its primary mission, the orbiter was to monitor Mars atmosphere and surface globally on a daily basis for one Martian year (two Earth years), observing the appearance and movement of atmospheric dust and water vapor, as well as characterizing seasonal changes of the planet's surface. Imaging of the surface morphology would also provide important clues about the planet's climate in its early history. The mission was part of NASA's Mars Surveyor program, a sustained program of robotic exploration of the red planet, managed by the Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, DC. Lockheed Martin Astronautics was NASA's industrial partner in the mission. Unfortunately, Mars Climate Orbiter burned up in the Martian atmosphere on September 23, 1999, due to a metric conversion error that caused the spacecraft to be off course.
Date 05/27/1998
NASA Center Jet Propulsion Laboratory
Ion Engine Test Firing
Title Ion Engine Test Firing
Full Description This image of a xenon ion engine, photographed through a port of the vacuum chamber where it was being tested at NASA's Jet Propulsion Laboratory, shows the faint blue glow of charged atoms being emitted from the engine. The ion propulsion engine is the first non-chemical propulsion to be used as the primary means of propelling a spacecraft. The first flight in NASA's New Millennium Program, Deep Space 1 is designed to validate 12 new technologies for scientific space missions of the next century. Ion propulsion was first proposed in the 1950s and NASA performed experiments on this highly efficient propulsion system in the 1960s, but it was not used aboard an American spacecraft until the 1990s. Deep Space 1 was launched in October 1998 as part of NASA's New Millennium Program, which is managed by JPL for NASA's Office of Space Science, Washington, DC. The California Institute of Technology in Pasadena manages JPL for NASA. The almost imperceptible thrust from the ion propulsion system is equivalent to the pressure exerted by a sheet of paper held in the palm of your hand. The ion engine is very slow to pick up speed, but over the long haul it can deliver 10 times as much thrust per pound of fuel as more traditional rockets. Unlike the fireworks of most chemical rockets using solid or liquid fuels, the ion drive emits only an eerie blue glow as ionized (electrically charged) atoms of xenon are pushed out of the engine. Xenon is the same gas found in photo flash tubes and many lighthouse bulbs.
Date 01/01/1999
NASA Center Jet Propulsion Laboratory
Utraviolet Light Source in a …
Title Utraviolet Light Source in an Old Galaxy
Full Description Hubble Space Telescope's exquisite resolution has allowed astronomers to resolve, for the first time, hot blue stars deep inside an elliptical galaxy. The swarm of nearly 8,000 blue stars resembles a blizzard of snowflakes near the core (lower right) of the neighboring galaxy M32, located 2.5 million light-years away in the constellation Andromeda. Hubble confirms that the ultraviolet light comes from a population of extremely hot helium-burning stars at a late stage in their lives. Unlike the Sun, which burns hydrogen into helium, these old stars exhausted their central hydrogen long ago, and now burn helium into heavier elements. The observations, taken in October 1998, were made with the camera mode of the Space Telescope Imaging Spectrograph (STIS) in ultraviolet light. The STIS field of view is only a small portion of the entire galaxy, which is 20 times wider on the sky. For reference, the full moon is 70 times wider than the STIS field-of-view. Thirty years ago, the first ultraviolet observations of elliptical galaxies showed that they were surprisingly bright when viewed in ultraviolet light. Before those pioneering UV observations, old groups of stars were assumed to be relatively cool and thus extremely faint in the ultraviolet. Over the years since the initial discovery of this unexpected ultraviolet light, indirect evidence has accumulated that it originates in a population of old, but hot, helium-burning stars. Now Hubble provides the first direct visual evidence.
Date 10/26/1999
NASA Center Hubble Space Telescope Center
View of the ISS during Flyar …
Title View of the ISS during Flyaround
Full Description Backdropped against white clouds and blue ocean waters, the International Space Station (ISS) moves away from the Space Shuttle Discovery. The U.S.- built Unity node (top) and the Russian-built Zarya or FGB module (with the solar array panels deployed) were joined during a December 1998 mission. A portion of the work performed on the May 30 space walk by astronauts Tamara E. Jernigan and Daniel T.Barry is evident at various points on the ISS, including the installation of the Russian-built crane (called Strela).
Date 06/03/1999
NASA Center Johnson Space Center
Hubble Views of Dust Disks a …
Title Hubble Views of Dust Disks and Rings Surrounding Young Stars Yield Clues
General Information What is an American Astronomical Society Meeting release? A major news announcement issued at an American Astronomical Society meeting, the premier astronomy conference. NASA's Hubble Space Telescope has given astronomers their first views of a dust ring around the star HR 4796A and a dark gap dividing an immense dust disk around the star HD 141569. These images may provide important clues to possible planet formation. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1999/03/text/ ]
Looking Down a Barrel of Gas …
Title Looking Down a Barrel of Gas at a Doomed Star
General Information What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Astronomers using the Hubble telescope have obtained the sharpest view yet of a glowing loop of gas called the Ring Nebula (M57), first cataloged more than 200 years ago by French astronomer Charles Messier. The pictures reveal that the "Ring" is actually a cylinder of gas seen almost end-on. Such elongated shapes are common among other planetary nebulae, because thick disks of gas and dust form a waist around a dying star. This "waist" slows down the expansion of material ejected by the doomed object. The easiest escape route for this cast-off material is above and below the star. This photo reveals dark, elongated clumps of material embedded in the gas at the edge of the nebula, the dying central star is floating in a blue haze of hot gas. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1999/01/text/ ]
Combined Deep View of Infrar …
Title Combined Deep View of Infrared and Visible Light Galaxies
The Trifid Nebula: Stellar S …
Title The Trifid Nebula: Stellar Sibling Rivalry
Very Long Baseline Array Rev …
Title Very Long Baseline Array Reveals Formation Region of Giant Cosmic Jet Near a Black Hole
The "Rotten Egg" Nebula: A P …
Title The "Rotten Egg" Nebula: A Planetary Nebula in the Making
Very Long Baseline Array Rev …
Title Very Long Baseline Array Reveals Formation Region of Giant Cosmic Jet Near a Black Hole
Hubble Finds Many Bright Clo …
Title Hubble Finds Many Bright Clouds on Uranus
Movies from Hubble Show the …
Title Movies from Hubble Show the Changing Faces of Infant Stars
'Survivor' Planets: Astronom …
Title 'Survivor' Planets: Astronomers Witness First Steps of Planet Growth - and Destruction
'Survivor' Planets: Astronom …
Title 'Survivor' Planets: Astronomers Witness First Steps of Planet Growth - and Destruction
'Survivor' Planets: Astronom …
Title 'Survivor' Planets: Astronomers Witness First Steps of Planet Growth - and Destruction
'Survivor' Planets: Astronom …
Title 'Survivor' Planets: Astronomers Witness First Steps of Planet Growth - and Destruction
'Survivor' Planets: Astronom …
Title 'Survivor' Planets: Astronomers Witness First Steps of Planet Growth - and Destruction
A Butterfly-Shaped "Papillon …
Title A Butterfly-Shaped "Papillon" Nebula Yields Secrets of Massive Star Birth
A Change of Seasons on Satur …
Title A Change of Seasons on Saturn
General Information What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Back to top [ #top ]
Hubble Unveils a Galaxy in L …
Title Hubble Unveils a Galaxy in Living Color
'Survivor' Planets: Astronom …
Title 'Survivor' Planets: Astronomers Witness First Steps of Planet Growth - and Destruction
'Survivor' Planets: Astronom …
Title 'Survivor' Planets: Astronomers Witness First Steps of Planet Growth - and Destruction
Cosmic Collisions - European …
Title Cosmic Collisions - European HST Scientists Catch Merging Galaxies in the Act
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Star Clusters Born in the Wr …
Title Star Clusters Born in the Wreckage of Cosmic Collisions
Starry Bulges Yield Secrets …
Title Starry Bulges Yield Secrets to Galaxy Growth
General Information What is a Space Science Update? Major Hubble discoveries on NASA television ... Astronomers explain their Hubble discoveries at a press conference, called a Space Science Update (SSU), broadcast on NASA television. The SSU includes a question and answer session with members of the media. The Hubble telescope is uncovering important new clues to a galaxy's birth and growth by peering into its heart ? a bulge of millions of stars resembling a bulbous center yolk in the middle of a disk of egg white. Astronomers have combined information from the Hubble telescope's visible- and infrared-light cameras to show the heart of four spiral galaxies peppered with ancient populations of stars. The top row of pictures, taken by a ground-based telescope, represents complete views of each galaxy. The blue boxes outline the regions observed by the Hubble telescope. The bottom row represents composite pictures from Hubble's visible- and infrared-light cameras. Astronomers combined views from both cameras to obtain the true ages of the stars surrounding each galaxy's bulge. The Hubble telescope's sharper resolution allows astronomers to study the intricate structure of a galaxy's central region. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1999/34/text/ ]
A Grazing Encounter between …
Title A Grazing Encounter between Two Spiral Galaxies
General Information What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Back to top [ #top ]
Hubble Hunts Down Binary Obj …
Title Hubble Hunts Down Binary Objects at the Fringe of Our Solar System
Hubble Hunts Down Binary Obj …
Title Hubble Hunts Down Binary Objects at the Fringe of Our Solar System
Hubble Hunts Down Binary Obj …
Title Hubble Hunts Down Binary Objects at the Fringe of Our Solar System
Hubble Hunts Down Binary Obj …
Title Hubble Hunts Down Binary Objects at the Fringe of Our Solar System
Hubble Hunts Down Binary Obj …
Title Hubble Hunts Down Binary Objects at the Fringe of Our Solar System
Hubble Hunts Down Binary Obj …
Title Hubble Hunts Down Binary Objects at the Fringe of Our Solar System
Hubble Hunts Down Binary Obj …
Title Hubble Hunts Down Binary Objects at the Fringe of Our Solar System
Movies from Hubble Show the …
Title Movies from Hubble Show the Changing Faces of Infant Stars
Movies from Hubble Show the …
Title Movies from Hubble Show the Changing Faces of Infant Stars
Movies from Hubble Show the …
Title Movies from Hubble Show the Changing Faces of Infant Stars
Movies from Hubble Show the …
Title Movies from Hubble Show the Changing Faces of Infant Stars
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