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Our NEOWISE mission detected comet C/2013 A1 Siding Spring on July 28, 2014, less than three months before this comet's close flyby of Mars on Oct. 19. NEOWISE took multiple images of the comet, combined here so that the comet is seen in four different positions relative to the background stars. The image also includes, near the upper right corner, a view of radio galaxy Fornax A (NGC1316). The observations help constrain estimates of dust and gas production as this comet from the outer solar system approaches Mars. NGC1316 has an active nucleus, as evidenced by a radio jet and a compact nuclear gas disk. It is thought to be the remnant of a merger between a large elliptical galaxy and a smaller spiral galaxy about 100 million years ago. Image credit: NASA/JPL-Caltech #nasa #space #comet #science; -
Aboard the International Space Station, Expedition 40 crew member Reid Wiseman posted this image and wrote, "Passing over India just now. Undoctored...unedited...unbelievable." Over the weekend, the station's astronauts and cosmonauts will take care of weekly housekeeping chores as they wipe down surfaces and vacuum dust. They also will continue their daily 2.5-hour workouts to stay fit and to prevent the loss of muscle mass and bone density that occurs in microgravity. Image Credit: NASA #nasa #spacestation #station #iss #exp40; -
The International Space Station's Expedition 40 crew closed out the work-week with preparations for the arrival of one space freighter and the departure of another, upgrades to the station's robotic crew member and a checkout of a pair of spacesuits for an upcoming spacewalk. One of the crew members aboard the space station, from an altitude of 221 nautical miles, photographed this image of Typhoon Halong at 08:02:41 GMT on Aug. 7, 2014. Image Credit: NASA #nasa #space #spacestation #exp40 #iss #halong; -
A globular cluster's age revisited: Globular clusters are big balls of old stars that orbit around their host galaxy. It has long been believed that all the stars within a globular cluster form at the about same time, a property which can be used to determine the cluster's age. For more massive globulars however, detailed observations have shown that this is not entirely true - there is evidence that they instead consist of multiple populations of stars born at different times. One of the driving forces behind this behaviour is thought to be gravity: more massive globulars manage to grab more gas and dust, which can then be transformed into new stars. IC 4499 is a somewhat special case. Its mass lies somewhere between low-mass globulars, which show a single generation build-up, and the more complex and massive globulars which can contain more than one generation of stars. By studying objects like IC 4499 astronomers can therefore explore how mass affects a cluster's contents. Credit: ESA/Hubble & NASA #nasa #hst #hubble #stars #science; -
Fishing LDSD Out of the Water: Divers retrieve the test vehicle for our Low-Density Supersonic Decelerator off the coast of the U.S. Navy's Pacific Missile Range Facility in Kauai, Hawaii. On June 28, 2014, the vehicle was lifted to near-space with the help of a balloon and rocket in order to test new Mars landing technologies. The divers, from the U.S. Navy's Explosive Ordnance Disposal team, retrieved the vehicle hours after the successful test. Image Credit: NASA/JPL-Caltech #nasa #ldsd #321techoff #space #nasatech;
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The Sun sported a very long filament (over 30 times the size of Earth) that angled diagonally across its surface for over a week (July 31 - Aug. 6, 2014). Filaments are clouds of cooler gas suspended above the Sun's surface by magnetic forces. They are notoriously unstable and often break apart in just hours or days. So far, this one has held together as it rotated along with the Sun for over a week. The images were taken in the 193 Angstrom wavelength of extreme ultraviolet light and were tinted red instead of its usual brown hue. Credit: NASA/Solar Dynamics Observatory #nasa #sdo #sun #filament #space #solar; -
In his newest film released recently, Dwayne Johnson is Hercules—the demigod who fights against evil and helps to end a civil war. But back in 2011, after playing the American astronaut Captain Chuck Baker in Planet 51, The Rock was touting the benefits of NASA technology for people here on earth. Video credit: NASA #TBT #321TechOff #nasa #space #spinoffs; -
Hurricanes Iselle and Julio Nearing the Hawaiian Islands In early August 2014, not one but two hurricanes were headed for the Hawaiian Islands. Storms arriving from the east are a relative rarity, and landfalling storms are also pretty infrequent. On Aug. 5, the Visible Infrared Imaging Radiometer Suite (VIIRS) sensor on the Suomi National Polar-orbiting Partnership (NPP) satellite captured natural-color images of both Iselle and Hurricane Julio en route to Hawaii. This image is a composite of three satellite passes over the tropical Pacific Ocean in the early afternoon. Note that Iselle’s eyewall had grown less distinct; the storm had descreased to category 2 intensity. The bright shading toward the center-left of the image is sunglint, the reflection of sunlight off the water and directly back at the satellite sensor. Image Credit: NASA image by Jeff Schmaltz, LANCE/EOSDIS Rapid Response. Caption Credit: Mike Carlowicz. #nasa #hurricane #earth #tropicalstorm #hawaii #pacificocean #pacific; -
Using NASA’s Hubble Space Telescope, a team of astronomers has spotted a star system that could have left behind a “zombie star” after an unusually weak supernova explosion. A supernova typically obliterates the exploding white dwarf, or dying star. On this occasion, scientists believe this faint supernova may have left behind a surviving portion of the dwarf star -- a sort of zombie star. While examining Hubble images taken years before the stellar explosion, astronomers identified a blue companion star feeding energy to a white dwarf, a process that ignited a nuclear reaction and released this weak supernova blast. This supernova, Type Iax, is less common than its brighter cousin, Type Ia. Astronomers have identified more than 30 of these mini-supernovas that may leave behind a surviving white dwarf. Seen here is an inset panel with a pair of before-and-after Hubble Space Telescope images of Supernova 2012Z in the spiral galaxy NGC 1309. The white X at the top of the galaxy image marks the location of the supernova. The 2005 and 2006 panel shows what astronomers believe to be a helium star transferring material to a white dwarf, causing the supernova in the 2013 panel. The team plans to use Hubble again in 2015 to observe the area, giving time for the supernova’s light to dim enough to reveal any possible surviving ”zombie star” and helium companion. Credit: NASA, ESA, C. McCully and S. Jha (Rutgers Univ.), and R. Foley (Univ. of Illinois) #nasa #hubble #zombie #zombies #stars #universe #hst #space; -
After a decade-long journey chasing its target, ESA’s Rosetta has today become the first spacecraft to rendezvous with a comet, opening a new chapter in Solar System exploration. This image, taken by Rosetta’s Onboard Scientific Imaging System (OSIRIS) on August 6, 2014, shows close up detail of comet 67P/Churyumov-Gerasimenko, focusing on a smooth region on the ‘base’ of the ‘body’ section of the comet. The image clearly shows a range of features, including boulders, craters and steep cliffs. The image was taken from a distance of 80 miles (130 kilometers) and the image resolution is 8 feet (2.4 meters) per pixel. The three U.S. instruments aboard the spacecraft are the Microwave Instrument for Rosetta Orbiter (MIRO), an ultraviolet spectrometer called Alice, and the Ion and Electron Sensor (IES) are part of a suite of 11 science instruments aboard the Rosetta orbiter. U.S. scientists are partnering on several non-U.S. instruments and are involved in seven of the mission's 21 instrument collaborations. NASA's Deep Space Network is supporting ESA's Ground Station Network for spacecraft tracking and navigation. Launched in March 2004, Rosetta was reactivated in January 2014 after a record 957 days in hibernation. Composed of an orbiter and lander, Rosetta's objectives upon arrival at comet 67P/Churyumov-Gerasimenko in August are to study the celestial object up close in unprecedented detail, prepare for landing a probe on the comet's nucleus in November, and track its changes as it sweeps past the sun. Comets are time capsules containing primitive material left over from the epoch when the sun and its planets formed. Rosetta's lander will obtain the first images taken from a comet's surface and will provide the first analysis of a comet's composition by drilling into the surface. Rosetta also will be the first spacecraft to witness at close proximity how a comet changes as it is subjected to the increasing intensity of the sun's radiation. Observations will help scientists learn more about the origin and evolution of our solar system and the role comets may have played in seeding Earth with water, and perhaps even life. Credit: ESA/Rosetta/MPS for OSIRIS;
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Two Years Ago, Curiosity Rover Lands on Mars, Captures Image of Mount Sharp This image was captured by NASA's Mars rover Curiosity shortly after it landed on the Red Planet on the evening of Aug. 5, 2012 PDT (morning of Aug. 6 EDT), near the foot of a mountain three miles tall and 96 miles in diameter inside Gale Crater. The image shows the rover's main science target, Mount Sharp. The rover's shadow can be seen in the foreground, and the dark bands beyond are dunes. Rising up in the distance is Mount Sharp, whose peak is 3.4 miles (5.5 kilometers) high, taller than Mt. Whitney in California. The actual summit is not visible from this vantage point -- the highest elevation seen in this view is about 2.5 miles (4 kilometers) above the rover. On June 24, 2014, Curiosity completed one Martian year -- 687 Earth days -- having accomplished the mission's main goal of determining whether Mars once offered environmental conditions favorable for microbial life. One of Curiosity's first major findings after landing in August 2012 was an ancient riverbed at its landing site. Nearby, at an area known as Yellowknife Bay, the mission met its main goal of determining whether the Martian Gale Crater ever was habitable for simple life forms. The answer, a historic "yes," came from two mudstone slabs that the rover sampled with its drill. Analysis of these samples revealed the site was once a lakebed with mild water, the essential elemental ingredients for life, and a type of chemical energy source used by some microbes on Earth. If Mars had living organisms, this would have been a good home for them. Image Credit: NASA/JPL-CalTech #2YearsOnMars #Landiversary #JourneyToMars #MarsCuriosity #Mars #Planet #RedPlanet #SolarSystem #Rover; -
Algae blooms are a regular occurrence on Lake Erie in summer. But it’s not every year that a bloom leads to the shutdown of water supplies in an American or Canadian city. The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite captured this natural-color view of an algae bloom in the west end of Lake Erie. The image of the coastal waters off of Ohio, Michigan, and southwestern Ontario was acquired at 2:50 p.m. Eastern Daylight Time (1850 Universal Time) on August 3, 2014. NASA's MODIS data is being incorporated into NOAA's Harmful Algal Bloom (HAB) alerts for Lake Erie and is supported by NASA's Earth Science Division's Applied Sciences Program. Image credit: NASA, LANCE/EOSDIS MODIS Rapid Response Team #nasa #space #earth #earthscience #lakeerie #algae #water #modis; -
The Eye of Saturn Like a giant eye for the giant planet, Saturn's great vortex at its north pole appears to stare back at Cassini as Cassini stares at it. Measurements have sized the “eye” at a staggering 1,240 miles (2,000 kilometers) across with cloud speeds as fast as 330 miles per hour (150 meters per second). The image was taken with the Cassini spacecraft narrow-angle camera on April 2, 2014 using a combination of spectral filters which preferentially admit wavelengths of near-infrared light centered at 748 nanometers. The view was obtained at a distance of approximately 1.4 million miles (2.2 million kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 43 degrees. Image scale is 8 miles (13 kilometers) per pixel. Credit: NASA/JPL-Caltech/Space Science Institute #nasa #cassini #saturn #solarsystem #space #planet; -
From above, Arctic ice looks quite different in summer than it does in winter. A sheen of white covers most surfaces in winter due to snowfall and frigid weather. As temperatures rise in the summer, turquoise splotches of color begin to speckle the ice surfaces. The splashes of blue are melt ponds, areas where snow has melted and pooled in low spots on glaciers and sea ice. A digital camera on NASA’s ER-2 airplane captured this top-down view of a melt pond atop a glacier in southeastern Alaska on July 16, 2014. Chunks of ice float on the pond’s turquoise water. When it took this photograph, the ER-2 was flying at 64,000 feet (20,000 meters), about twice as high as a commercial jet. In addition to the camera, the ER-2 was carrying the Multiple Altimeter Beam Experimental Lidar (MABEL). MABEL is a laser altimeter designed to measure the elevation of glaciers, mountains, forests, and other landforms below. Scientists are using MABEL’s measurements to design algorithms for the upcoming Ice, Cloud and land Elevation Satellite-2 (ICESat-2) mission. MABEL is similar to an instrument that will fly on ICESat-2, and scientists can use its measurements now to better understand how the instrument works and what the data will look like when they start making measurements from space. The 2014 MABEL campaign was launched, in part, to study melt ponds and other features of summer ice. Engineers added a new camera system that made it possible to match the MABEL measurements with a photographic glimpse of the ground. The digital camera took a picture every 3 seconds, with each frame capturing an area about 2.5 by 1.5 kilometers (1.6 by 0.9 miles). Credit: NASA/MABEL team; -
Hubble Eyes Galaxy as it Gets a Cosmic Hair Ruffling From objects as small as Newton's apple to those as large as a galaxy, no physical body is free from the stern bonds of gravity, as evidenced in this stunning picture captured by the Wide Field Camera 3 and Advanced Camera for Surveys onboard the NASA/ESA Hubble Space Telescope. Here we see two spiral galaxies engaged in a cosmic tug-of-war — but in this contest, there will be no winner. The structures of both objects are slowly distorted to resemble new forms, and in some cases, merge together to form new, super galaxies. This particular fate is similar to that of the Milky Way Galaxy, when it will ultimately merge with our closest galactic partner, the Andromeda Galaxy. There is no need to panic however, as this process takes several hundreds of millions of years. Not all interacting galaxies result in mergers though. The merger is dependent on the mass of each galaxy, as well as the relative velocities of each body. It is quite possible that the event pictured here, romantically named 2MASX J06094582-2140234, will avoid a merger event altogether, and will merely distort the arms of each spiral without colliding — the cosmic equivalent of a hair ruffling! These galactic interactions also trigger new regions of star formation in the galaxies involved, causing them to be extremely luminous in the infrared part of the spectrum. For this reason, these types of galaxies are referred to as LIRGs, or Luminous Infrared Galaxies. This image was taken as part of as part of a Hubble survey of the central regions of LIRGs in the local Universe, which also used the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) instrument. Credit: ESA/Hubble & NASA, Acknowledgement: Luca Limatola #nasa #hubble #universe #galaxy #galaxies #space;
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