lundi 23 juin 2014

Hubble Sees a Dwarf Galaxy Shaped by a Grand Design












ESA - Hubble Space Telescope patch.

June 23, 2014


The subject of this Hubble image is NGC 5474, a dwarf galaxy located 21 million light-years away in the constellation of Ursa Major (The Great Bear). This beautiful image was taken with Hubble's Advanced Camera for Surveys (ACS).

The term "dwarf galaxy" may sound diminutive, but don't let that fool you — NGC 5474 contains several billion stars! However, when compared to the Milky Way with its hundreds of billions of stars, NGC 5474 does indeed seem relatively small.

NGC 5474 itself is part of the Messier 101 Group. The brightest galaxy within this group is the well-known spiral Pinwheel Galaxy (also known as Messier 101). This galaxy's prominent, well-defined arms classify it as a "grand design galaxy," along with other spirals Messier 81 and Messier 74.

Hubble orbiting the Earth

Also within this group are Messier 101's galactic neighbors. It is possible that gravitational interactions with these companion galaxies have had some influence on providing Messier 101 with its striking shape. Similar interactions with Messier 101 may have caused the distortions visible in NGC 5474.

Both the Messier 101 Group and our own Local Group reside within the Virgo Supercluster, making NGC 5474 something of a neighbor in galactic terms.

For images and more information about Hubble, visit: http://www.nasa.gov/hubble and http://www.spacetelescope.org/

Image, Video, Text, Credits: ESA / NASA.

Greetings, Orbiter.ch

From oldest to youngest: a line of star nurseries












ESA - Herschel Mission patch.

June 23, 2014

Star-forming regions in the molecular cloud W48

Just as children are sorted into age groups at school, so the seeds of new stars can also be found in ‘classes’ of others of similar ages. This is especially true when the birth of stars in a cloud of gas and dust is triggered by an external event, like the explosion of a nearby supernova.

This image from ESA’s Herschel space observatory shows a sequence of star-forming regions in the molecular cloud W48, some 10 000 light-years away in the constellation Aquila (the Eagle).

The blue, jellyfish-shaped cloud at the lower left is the oldest stellar nursery in the image. Young and massive stars embedded within it have shaped it into a bubble and heated the diffuse gas, making it shine at the longest wavelengths probed by Herschel.

To its right, another glowing cloud conceals clumps that will evolve into massive stars. These clumps, some of which are visible as bright blotches of light, are also lined up by their age: the older ones at the lower-left and the younger ones to the upper-right. The youngest in this sequence is the small cyan lump at the centre of the image, harbouring the seeds of future massive stars.

Astronomers believe that this sequence of stellar birth is the result of dozens of supernovas that exploded over 10 million years ago in a region called Aquila Supershell, beyond the left edge of this image. Compressing the surrounding material, these supernovas may have initiated a wave of star formation that sparked, one by one, these stellar cribs.

Herschel space observatory

The image is a composite of the wavelengths of 70 microns (blue), 160 microns (green) and 250 microns (red) and spans about one degree on the long side. North is to the upper-left and east is to the lower left. The data were acquired with Herschel’s PACS and SPIRE instruments in September 2010, as part of a larger map of the W48 molecular complex in the HOBYS Key Programme. This was first published in a paper by Q. Nguyen Luong, et al. 2011. A more detailed study of the star-forming regions shown in this image is presented in a paper by K.L.J. Rygl, et al. 2014.

For more information about Herschel, visit: http://www.esa.int/Our_Activities/Space_Science/Herschel

Images, Text, Credits: ESA/Herschel/PACS/SPIRE/HOBYS Key Programme consortium.

Best regards, Orbiter.ch

vendredi 20 juin 2014

QuikScat's Eye on Ocean Winds Lives On with RapidScat









NASA - QuikScat Mission patch.

June 20, 2014


Image above: Using data from NASA’s QuikScat, weather forecasters were able to predict hazardous weather events over oceans 6 to 12 hours earlier than before these data were available. Orange areas show where winds are blowing the hardest and blue shows relatively light winds. Image Credit: NASA.

Today (June 19) marks the 15th anniversary of the launch of NASA's QuikScat, a satellite sent for a three-year mission in 1999 that continues collecting data. Built in less than 12 months, QuikScat has watched ocean wind patterns for 15 years and improved weather forecasting worldwide. Despite a partial instrument failure in 2009, it provides calibration data to international partners.

On this anniversary, the mission's team is preparing to calibrate ISS-RapidScat, the successor that will maintain QuikScat’s unbroken data record. After its launch in a few months, RapidScat will watch ocean winds from the International Space Station (ISS) for a two-year mission.

Much like QuikScat, ISS-RapidScat was built in less than two years and at a fraction of its predecessor’s budget. Both missions are testaments to ingenuity, craftsmanship and speedy construction in the name of improving our understanding of Earth’s winds.

“Both ISS-RapidScat and QuikScat came about to react quickly to the failure of another spaceborne instrument,” said Ernesto Rodriguez, project scientist for the ISS-RapidScat mission at NASA’s Jet Propulsion Laboratory, Pasadena, California. “What differentiates these missions is cost and risk: RapidScat had to be built with a fraction of the QuikScat budget, and the mission accepted a much riskier approach,” Rodriguez said. RapidScat was constructed primarily from QuikScat’s spare parts and will be the first scatterometer to berth on the International Space Station.

Scatterometers help scientists estimate the speed and direction of winds at the ocean’s surface by sending microwave pulses to Earth’s surface. Strong waves or ripples scatter the microwaves, sending some of them back toward the scatterometer. Based on the strength of this backscatter, scientists can estimate the strength and direction of the wind at the ocean’s surface.

Scatterometer data are critical for observing global weather patterns. They also help ocean fishermen decide where to fish, ship captains choose shipping lanes and researchers track hurricanes, cyclones and El Niños.

“The usefulness of this wind measurement is enormous,” said JPL’s Jim Graf, who served as project manager for the QuikScat mission in the 1990s and is now the deputy director of JPL’s Earth Science and Technology Directorate. “One of the dominant factors in understanding the climate is to assess what is happening in the ocean circulation. And one of the dominant factors in ocean circulation is the wind at the surface, which is what scatterometers measure.”


Image above: QuikScat could detect differences in average wave height much smaller than inch (a centimeter) during its 15 years watching ocean winds. Image Credit: Wikimedia Commons.

NASA launched its first scatterometer satellite in 1978 and its second instrument, the NASA Scatterometer (NSCAT), on a Japanese satellite in 1996. Each lasted less than a year, but collected hundreds of times more data about ocean winds than ships or buoys and improved weather forecasts from the National Oceanic and Atmospheric Administration (NOAA).

But the spacecraft carrying NSCAT malfunctioned in 1997. Immediately, a team of JPL scientists and engineers raced to get a scatterometer satellite back into space.

“We had the idea that a partially developed spacecraft bus could be mated with an advanced version of the instrument that was already under development, and we could get something up quickly. So we went to NASA, and they said, ‘Okay, let’s give it a shot, but we want you to be ready to go one year from the go-ahead,’” Graf said. “And so we took off running, and we didn’t stop for a whole year.”

In that year, Ball Aerospace & Technologies Corp., Boulder, Colorado, built the QuikScat satellite bus while JPL finished the new SeaWinds scatterometer instrument. It launched in 1999. For the next decade, QuikScat made about 400,000 daily measurements of wind speed and direction. Over 15-mile (25-kilometer) segments of ocean, its measurements were detailed enough to estimate average wind speed within 6 feet (2 meters) per second.

The SeaWinds instrument on QuikScat used a rotating antenna to measure a swath of Earth’s surface 1,118 miles (1,800 kilometers) wide -- about the distance from Los Angeles to Seattle. As QuikScat flew, the rotations overlapped to cover more than 90 percent of Earth’s surface every day.

But by the end of 2009, long after the expected end of QuikScat’s mission, the lubricant coating the antenna’s bearings dried up. Instead of tracing a round swath on Earth’s surface, it pointed straight down and only watched the waves directly below it. Still, those data were sufficient to help calibrate newer satellites.

QuikScat satellite. Image Credit: NASA

“Since 2009, we’ve been able to keep QuikScat operating quite successfully,” said QuikScat Project Manager Rob Gaston of JPL. “We used QuikScat’s highly successful backscatter measurements, which were well understood and had demonstrated stability, as a calibration standard for many instruments, including other scatterometers.” The European Space Agency and Indian Space Research Organization have both used QuikScat data to calibrate scatterometers in the last five years.

QuikScat’s final task will be to calibrate its successor, RapidScat. The satellite will continue collecting data until April 2015, when it will be decommissioned after nearly 16 years in orbit.

RapidScat, like QuikScat, was built in a fraction of the timeline for most missions. The two missions even share hardware: JPL engineers used SeaWinds test parts to build much of RapidScat, which also uses a rotating dish antenna.

RapidScat will launch aboard a SpaceX Dragon resupply mission this summer. Flying in the space station’s orbit means RapidScat will spend more time observing Earth's tropics than previous scatterometer satellites, which orbited farther north and south.

“RapidScat will be able to, for the first time, map the evolution of winds as the day progresses, which is important for understanding how clouds and precipitation develop, especially in the tropics, which are key regions in Earth's climate system,” Rodriguez said. “It will provide a common reference to tie all of these measurements together.”

Together with scatterometers managed by India and Europe, RapidScat will maintain the continuous climate record QuikScat began while adding its own unique perspective from orbit.

For more information about ISS-RapidScat, visit: http://winds.jpl.nasa.gov/missions/RapidScat/

For more information about QuikScat, visit: http://winds.jpl.nasa.gov/missions/quikscat/

NASA monitors Earth's vital signs from land, air and space with a fleet of satellites and ambitious airborne and ground-based observation campaigns. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records and computer analysis tools to better see how our planet is changing. The agency shares this unique knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.

For more information about NASA's Earth science activities in 2014, visit: http://www.nasa.gov/earthrightnow

Images (mentioned), Text, Credits: NASA.

Greetings, Orbiter.ch

Science and spacewalks on Space Station












ESA - Blue Dot Mission patch.

20 June 2014

Flying over Earth

Three weeks into ESA astronaut Alexander Gerst’s Blue Dot mission on the International Space Station and the new arrival is now spending more time on scientific research in the microgravity laboratory.

Alexander has worked on controlled fires in space and continuously monitored his sleep patterns, at the same time as making sure the orbital outpost is working at full capacity.

Apart from continuing the long-term studies on eyes and headaches in space, Alexander recorded his temperature and hormones over 36 hours to understand his sleep patterns.

Columbus laboratory

Astronauts on the Station witness 16 sunrises and sunsets each day – whereas on Earth our bodies rely on sunlight to kick-start hormone production that make us sleepy or wake us up.

Researchers are interested to see how the unique 90-minute days influence sleep. Aside from making sure astronauts feel awake at critical moments, this research in space allows sleep specialists to test theories that they couldn’t anywhere else.

Alexander acted as a weightless firestarter and firefighter this week when he ignited small samples of fuels safely contained in ESA’s glovebox to see how they burn in space. He volunteered as a fireman before becoming an astronaut, so the experiment was in good hands.

This research will improve computer models for fire detectors and extinguishers, both in space and on Earth. He explained the experiment via Twitter: “Burning things in space for better fire safety on Earth.”

Burning fuel in space

Elsewhere, Alexander took samples of his blood and saliva and collected data on his eyes, his skin and his body so researchers can understand how astronauts react to weightlessness.

Other notable experiments included the harvesting of space-grown salads – unfortunately for the astronauts, they are not allowed to eat them.

Spacewalk

Yesterday, cosmonauts Oleg Armetyev and Alexander Skvortsov spent over six hours working outside the Station to install an antenna, take samples and move experiments. Meanwhile the four astronauts inside continued their science activities.

Checking spacesuit

Earlier, Alexander thoroughly checked a newly arrived US spacesuit. Before being declared ready for use, he had to make sure it had survived its climb into space.

Spacewalk

Image above: Russian cosmonauts Alexander Skvortzov and Oleg Artemyev spent over six hours working outside the International Space Station on 19 June 2014. This picture was taken by ESA astronaut Alexander Gerst from inside the orbital outpost.

Alexander even had time this week for educational activities for Earth Guardian, inspiring children to observe geographical features such as oceans, rivers, landscapes, mountains and forests in their areas during the summer holidays.

Related links:

All about Blue Dot: http://www.esa.int/Our_Activities/Human_Spaceflight/Blue_dot

Connect with Alexander Gerst: http://alexandergerst.esa.int/

Where is the International Space Station?: http://www.esa.int/Our_Activities/Human_Spaceflight/International_Space_Station/Where_is_the_International_Space_Station

Images, Text, Credits: ESA / NASA.

Greetings, Orbiter.ch

Beautiful Brazil












ESA - Proba-V Mission logo.

20/06/2014

Proba-V imaging Brazil

As football fans worldwide keep their eyes trained on Brazil, ESA’s Proba-V minisatellite captures the entire country in a single image.

The Andean Plateau, or Altiplano, of neighbouring Bolivia, including Lake Titicaca and the giant Salar Uyuni salt flat, are visible towards the scene’s western edge.

Proba is smaller than a cubic metre but its view spans a mighty 2250 km. It reveals details 300 m across but the central part of the image is sharper – down to 100 m – as demonstrated in the right-hand image, which shows a detail of the River Negro joining the mighty River Amazon.

Proba-V is a miniaturised ESA satellite tasked with a full-scale mission: to map land cover and vegetation growth across the entire planet every two days.

Artist's view of the Proba-V satellite

The camera’s continent-spanning field of view collects light in the blue, red, near-infrared and mid-infrared wavebands, ideal for monitoring plant and forest growth as well as inland water bodies.

Proba’s images are processed and distributed to hundreds of scientific end users by VITO, Belgium’s Flemish Institute for Technological Research, extending the coverage of previous generations of the Vegetation camera flown on the Spot-4 and Spot-5 satellites.

For more information about Proba-V, visit: http://www.esa.int/Our_Activities/Technology/Proba_Missions

Images, Text, Credits: ESA / BELSPO.

Cheers, Orbiter.ch

Spacewalk of the Russian cosmonauts completed













ISS - Expedition 40 Mission patch / ROSCOSMOS - Russian Cosmonaut patch.

20.06.2014

Roscosmos cosmonauts Alexander Skvortsov and Oleg Artemyev, exit hatch docking module "Pirs"

Exit hatch docking module "Pirs" closed, the crew members MKS-40/41 Roscosmos cosmonauts Alexander Skvortsov and Oleg Artemyev, completed a spacewalk.

Russian cosmonaut duo make first spacewalk outside ISS

Astronauts set to work in the open space in 18 hours 10 minutes Moscow time. During the exit 38 on the Russian segment of the ISS program have completed installation of the external unit AFAR for subsequent installation of communication with Earth via relay satellites of "Ray".

Roscosmos cosmonauts Alexander Skvortsov and Oleg Artemyev

The unit of PVK-2 experiment scientific equipment "decor" was moved in the direction of the instrument compartment of the service module "Zvezda "astronauts check the working condition of locks on the universal workplace implemented reinstallation monoblock TM / TC and SVPI farm carrying scientific equipment MPAC & SEED, and took samples from the outer surface of the window number 2 on the IV plane working compartment within the space experiment "Test".

Roscosmos cosmonaut Alexander Skvortsov

Exit hatch was closed June 20, 2014 at 1:00 34 minutes Moscow time. Alexander Skvortsov and Oleg Artemyev first performed the work in open space, the duration of extravehicular activity was 7:00 24 minutes.

ROSCOSMOS Press Release: http://www.federalspace.ru/20704/

Images, Video, Text, Credits: Roscosmos press service / ROSCOSMOS / Euronews / NASA TV / Translation: Orbiter.ch Aerospace.

Best regards, Orbiter.ch

Swiftly moving gas streamer eclipses supermassive black hole












ESA - Hubble Space Telescope logo.

20 June 2014

Astronomers have discovered strange and unexpected behaviour around the supermassive black hole at the heart of the galaxy NGC 5548. The international team of researchers detected a clumpy gas stream flowing quickly outwards and blocking 90 percent of the X-rays emitted by the black hole. This activity could provide insights into how supermassive black holes interact with their host galaxies.

The discovery of the unusual behaviour in NGC 5548 is the result of an intensive observing campaign using major ESA and NASA space observatories, including the NASA/ESA Hubble Space Telescope [1]. In 2013 and 2014 the international team carried out the most extensive monitoring campaign of an active galaxy [2] ever conducted.

There are other galaxies that show gas streams near a black hole, but this is the first time that a stream like this has been seen to move into the line of sight.

Supermassive black hole at the heart of NGC 5548

The researchers say that this is the first direct evidence for the long-predicted shielding process that is needed to accelerate powerful gas streams, or winds, to high speeds. “This is a milestone in understanding how supermassive black holes interact with their host galaxies,” says Jelle Kaastra of the SRON Netherlands Institute for Space Research, who led the research team [3]. “We were very lucky. You don’t normally see this kind of event with objects like this. It tells us more about the powerful ionised winds that allow supermassive black holes in the nuclei of active galaxies to expel large amounts of matter. In larger quasars than NGC 5548, these winds can regulate the growth of both the black hole and its host galaxy.”

As matter spirals down into a black hole it forms a flat disc, known as an accretion disc. The disc is heated so much that it emits X-rays, near to the black hole, and less energetic ultraviolet radiation further out. The ultraviolet radiation can create winds strong enough to blow gas away from the black hole, which otherwise would have fallen into it. But, the winds only come into existence if their starting point is shielded from X-rays.

Earlier observations had seen the effects of both X-rays and ultraviolet radiation on a region of warm gas for away from the black hole, but these most recent observations have shown the presence of a new gas stream between the disc and the original cloud. The newly discovered gas stream in the archetypal Seyfert galaxy NGC 5548 — one of the best-studied sources of this type over the past half-century — absorbs most of the X-ray radiation before it reaches the original cloud, shielding it from X-rays and leaving only the ultraviolet radiation. The same stream shields gas closer to the accretion disc. This makes the strong winds possible, and it appears that the shielding has been going on for at least three years.

Directly after Hubble had observed NGC 5548 on 22 June 2013, the team discovered unexpected features in the data. “There were dramatic changes since the last observation with Hubble in 2011. We saw signatures of much colder gas than was present before, indicating that the wind had cooled down, due to a strong decrease in the ionising X-ray radiation from the nucleus,” said team member Gerard Kriss of the Space Telescope Science Institute in Baltimore, USA.

After combining and analysing data from the six observatories involved, the team was able to put the pieces of the puzzle together. NGC 5548’s persistent wind, which has been known about for two decades, reaches velocities exceeding 3.5 million kilometres per hour. But, a new wind has arisen which is much stronger and faster than the persistent wind.

Artist’s impression of gas filament eclipsing a black hole

“The new wind reaches speeds of up to 18 million kilometres per hour, but is much closer to the nucleus than the persistent wind,” says Kaastra. “The new gas outflow blocks 90 percent of the low-energy X-rays that come from very close to the black hole, and it obscures up to a third of the region that emits the ultraviolet radiation at a distance of a few light-days from the black hole.”

Strong X-ray absorption by ionised gas has been seen in several other sources, and it has been attributed for instance to passing clouds. “However, in our case, thanks to the combined XMM-Newton and Hubble data, we know this is a fast stream of outflowing gas very close to the nucleus,” said team member Massimo Cappi, of INAF-IASF Bologna. “It may even originate from the accretion disc,” added team member Pierre-Olivier Petrucci, of CNRS, IPAG Grenoble.

These results are being published online in the 19 June issue of Science Express.

Notes:
[1] The observatories include ESA’s X-ray Multi-Mirror Mission (XMM-Newton), the NASA/ESA Hubble Space Telescope, NASA’s Swift, NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR), NASA’s Chandra X-ray Observatory, and ESA's International Gamma-Ray Astrophysics Laboratory (INTEGRAL).

[2] An active galaxy is a galaxy which hosts an active galactic nucleus (AGN). An AGN is a compact region at the centre of a galaxy that has a much higher than normal luminosity. The high level of radiation, sometimes across the whole of the electromagnetic spectrum, is thought to be a result the supermassive black hole at the centre pulling in mass from the surroundings.

[3] The interactions between black holes and their host galaxies are believed to have a fundamental importance on the way galaxies evolve.

Notes for editors:

The Hubble Space Telescope is a project of international cooperation between ESA and NASA.

Links:

Images of Hubble: http://www.spacetelescope.org/images/archive/category/spacecraft/

For images and more information about Hubble, visit: http://www.nasa.gov/hubble and http://www.spacetelescope.org/

Image, Text, Credits: ESA/Hubble and NASA/Acknowledgement: Davide de Martin/A. Feild (STScI).

Greetings, Orbiter.ch