THE STAR CRADLE

FROM: NASA
A Nearby Stellar Cradle
The Milky Way and other galaxies in the universe harbor many young star clusters and associations that each contain hundreds to thousands of hot, massive, young stars known as O and B stars. The star cluster Cygnus OB2 contains more than 60 O-type stars and about a thousand B-type stars. Deep observations with NASA’s Chandra X-ray Observatory have been used to detect the X-ray emission from the hot outer atmospheres, or coronas, of young stars in the cluster and to probe how these fascinating star factories form and evolve. About 1,700 X-ray sources were detected, including about 1,450 thought to be stars in the cluster. In this image, X-rays from Chandra (blue) have been combined with infrared data from NASA’s Spitzer Space Telescope (red) and optical data from the Isaac Newton Telescope (orange).

Image Credit: NASA

THE OLDEST EXAMPLE OF A SUPERNOVA

FROM:  NASA
All That Remains


Infrared images from NASA's Spitzer Space Telescope and the Wide-field Infrared Survey Explorer, or WISE, were combined in this image of RCW 86, the dusty remains of the oldest documented example of an exploding star, or supernova. It shows light from both the remnant itself and unrelated background light from our Milky Way galaxy. The colors in the image allow astronomers to distinguish between the remnant and galactic background, and determine exactly which structures belong to the remnant.

Dust associated with the blast wave of the supernova appears red in this image, while dust in the background appears yellow and green. Stars in the field of view appear blue. By determining the temperature of the dust in the red circular shell of the supernova remnant, which marks the extent to which the blast wave from the supernova has traveled since the explosion, astronomers were able to determine the density of the material there, and conclude that RCW 86 must have exploded into a large, wind-blown cavity.

Image Credit-NASA-JPL-Caltech-UCLA

NASA'S SPITZER FINDS ALIEN "SUPER EARTH"

FROM:  NASA
News Releases
May 8, 2012 RELEASE : 12-138  NASA's Spitzer Sees the Light of Alien "Super Earth"  WASHINGTON -- NASA's Spitzer Space Telescope has detected light emanating from a "super-Earth" planet beyond our solar system for the first time. While the planet is not habitable, the detection is a historic step toward the eventual search for signs of life on other planets.

"Spitzer has amazed us yet again," said Bill Danchi, Spitzer program scientist at NASA Headquarters in Washington. "The spacecraft is pioneering the study of atmospheres of distant planets and paving the way for NASA's upcoming James Webb Space Telescope to apply a similar technique on potentially habitable planets."

The planet, called 55 Cancri e, falls into a class of planets termed super Earths, which are more massive than our home world but lighter than giant planets like Neptune. Fifty-five Cancri e is about twice as big and eight times as massive as Earth. The planet orbits a bright star, called 55 Cancri, in a mere 18 hours.

Previously, Spitzer and other telescopes were able to study the planet by analyzing how the light from 55 Cancri changed as the planet passed in front of the star. In the new study, Spitzer measured how much infrared light comes from the planet itself. The results reveal the planet is likely dark and its sun-facing side is more than 2,000 Kelvin (3,140 degrees Fahrenheit), hot enough to melt metal.

The new information is consistent with a prior theory that 55 Cancri e is a water world: a rocky core surrounded by a layer of water in a "supercritical" state where it is both liquid and gas, and topped by a blanket of steam.

"It could be very similar to Neptune, if you pulled Neptune in toward our sun and watched its atmosphere boil away," said Michaël Gillon of Université de Liège in Belgium, principal investigator of the research, which appears in the Astrophysical Journal. The lead author is Brice-Olivier Demory of the Massachusetts Institute of Technology in Cambridge.

The 55 Cancri system is relatively close to Earth at 41 light-years away. It has five planets, with 55 Cancri e being the closest to the star and tidally locked, so one side always faces the star. Spitzer discovered the sun-facing side is extremely hot, indicating the planet probably does not have a substantial atmosphere to carry the sun's heat to the unlit side.

NASA's James Webb Space Telescope, scheduled to launch in 2018, likely will be able to learn even more about the planet's composition. The telescope might be able to use a similar infrared method as Spitzer to search other potentially habitable planets for signs of molecules possibly related to life.

"When we conceived of Spitzer more than 40 years ago, exoplanets hadn't even been discovered," said Michael Werner, Spitzer project scientist at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif. "Because Spitzer was built very well, it's been able to adapt to this new field and make historic advances such as this."

In 2005, Spitzer became the first telescope to detect light from a planet beyond our solar system. To the surprise of many, the observatory saw the infrared light of a "hot Jupiter," a gaseous planet much larger than the solid 55 Cancri e. Since then, other telescopes, including NASA's Hubble and Kepler space telescopes, have performed similar feats with gas giants using the same method.

In this method, a telescope gazes at a star as a planet circles behind it. When the planet disappears from view, the light from the star system dips ever so slightly, but enough that astronomers can determine how much light came from the planet itself. This information reveals the temperature of a planet, and, in some cases, its atmospheric components. Most other current planet-hunting methods obtain indirect measurements of a planet by observing its effects on the star.

During Spitzer's ongoing extended mission, steps were taken to enhance its unique ability to see exoplanets, including 55 Cancri e. Those steps, which included changing the cycling of a heater and using an instrument in a new way, led to improvements in how precisely the tele

JPL manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate in Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology (Caltech) in Pasadena. Data are archived at the Infrared Science Archive housed at the Infrared Processing and Analysis Center at Caltech. Caltech manages JPL for NASA

NASA'S SPITZER FINDS GALAXY WITH SPLIT PERSONALITY

WASHINGTON -- While some galaxies are rotund and others are slender 
disks like our spiral Milky Way, new observations from NASA's Spitzer 
Space Telescope show that the Sombrero galaxy is both. The galaxy, 
which is a round, elliptical with a thin disk embedded inside, is one 
of the first known to exhibit characteristics of the two different 
types. The findings will lead to a better understanding of galaxy 
evolution, a topic still poorly understood. 

"The Sombrero is more complex than previously thought," said Dimitri 
Gadotti of the European Southern Observatory in Chile and lead author 
of a new paper on the findings appearing in the Monthly Notices of 
the Royal Astronomical Society. "The only way to understand all we 
know about this galaxy is to think of it as two galaxies, one inside 
the other." 

The Sombrero galaxy, also known as NGC 4594, is located 28 million 
light-years away in the constellation Virgo. From our viewpoint on 
Earth, we can see the thin edge of its flat disk and a central bulge 
of stars, making it resemble a wide-brimmed hat. Astronomers do not 
know whether the Sombrero's disk is shaped like a ring or a spiral, 
but agree it belongs to the disk class. 

"Spitzer is helping to unravel secrets behind an object that has been 
imaged thousands of times," said Sean Carey of NASA's Spitzer Science 
Center at the California Institute of Technology in Pasadena, Calif.. 
"It is intriguing Spitzer can read the fossil record of events that 
occurred billions of years ago within this beautiful and archetypal 
galaxy." 

Spitzer captures a different view of the galaxy than visible-light 
telescopes. In visible views, the galaxy appears to be immersed in a 
glowing halo, which scientists had thought was relatively light and 
small. With Spitzer's infrared vision, a different view emerges. 
Spitzer sees old stars through the dust and reveals the halo has the 
right size and mass to be a giant elliptical galaxy. 

While it is tempting to think the giant elliptical swallowed a spiral 
disk, astronomers say this is highly unlikely because that process 
would have destroyed the disk structure. Instead, one scenario they 
propose is that a giant elliptical galaxy was inundated with gas more 
than nine billion years ago. Early in our universe, networks of gas 
clouds were common, and they sometimes fed growing galaxies, causing 
them to bulk up. The gas would have been pulled into the galaxy by 
gravity, falling into orbit around the center and spinning out into a 
flat disk. Stars would have formed from the gas in the disk. 

"This poses all sorts of questions," said Rubén Sánchez-Janssen from 
the European Southern Observatory, co-author of the study. "How did 
such a large disk take shape and survive inside such a massive 
elliptical? How unusual is such a formation process?" 

Researchers say the answers could help them piece together how other 
galaxies evolve. Another galaxy, called Centaurus A, appears also to 
be an elliptical galaxy with a disk inside it. But its disk does not 
contain many stars. Astronomers speculate that Centaurus A could be 
at an earlier stage of evolution than the Sombrero and might 
eventually look similar. 

The findings also answer a mystery about the number of globular 
clusters in the Sombrero galaxy. Globular clusters are spherical 
nuggets of old stars. Ellipticals typically have a few thousand, 
while spirals contain a few hundred. The Sombrero has almost 2,000, a 
number that makes sense now but had puzzled astronomers when they 
thought it was only a disk galaxy. 

HUBBLE CELEBRATES 22 YEARS IN ORBIT

FROM:  NASA
To celebrate its 22nd anniversary in orbit, the Hubble Space Telescope released a dramatic new image of the star-forming region 30 Doradus, also known as the Tarantula Nebula because its glowing filaments resemble spider legs. A new image from all three of NASA's Great Observatories--Chandra, Hubble, and Spitzer--has also been created to mark the event. The nebula is located in the neighboring galaxy called the Large Magellanic Cloud, and is one of the largest star-forming regions located close to the Milky Way. At the center of 30 Doradus, thousands of massive stars are blowing off material and producing intense radiation along with powerful winds. The Chandra X-ray Observatory detects gas that has been heated to millions of degrees by these stellar winds and also by supernova explosions. These X-rays, colored blue in this composite image, come from shock fronts--similar to sonic booms--formed by this high-energy stellar activity. The Hubble data in the composite image, colored green, reveals the light from these massive stars along with different stages of star birth, including embryonic stars a few thousand years old still wrapped in cocoons of dark gas. Infrared emission data from Spitzer, seen in red, shows cooler gas and dust that have giant bubbles carved into them. These bubbles are sculpted by the same searing radiation and strong winds that comes from the massive stars at the center of 30 Doradus. Image Credits: X-ray: NASA/CXC/PSU/L.Townsley et al.; Optical: NASA/STScI; Infrared: NASA/JPL/PSU/L.Townsley et al.

22ND ANNIVERSARY OF HUBBLE SPACE TELESCOPE

FROM:  NASA
To celebrate its 22nd anniversary in orbit, the Hubble Space Telescope has released a dramatic new image of the star-forming region 30 Doradus, also known as the Tarantula Nebula because its glowing filaments resemble spider legs. A new image from all three of NASA's Great Observatories - Chandra, Hubble, and Spitzer - has also been created to mark the event.

30 Doradus is located in the neighboring galaxy called the Large Magellanic Cloud, and is one of the largest star-forming regions located close to the Milky Way . At the center of 30 Doradus, thousands of massive stars are blowing off material and producing intense radiation along with powerful winds. The Chandra X-ray Observatory detects gas that has been heated to millions of degrees by these stellar winds and also by supernova explosions. These X-rays, colored blue in this composite image, come from shock fronts -- similar to sonic booms -- formed by this high-energy stellar activity.

The Hubble data in the composite image, colored green, reveals the light from these massive stars along with different stages of star birth including embryonic stars a few thousand years old still wrapped in cocoons of dark gas. Infrared emission from Spitzer, seen in red, shows cooler gas and dust that have giant bubbles carved into them. These bubbles are sculpted by the same searing radiation and strong winds that comes from the massive stars at the center of 30 Doradus.

Credits: X-ray: NASA/CXC/PSU/L.Townsley et al.; Optical: NASA/STScI; Infrared: NASA/JPL/PSU/L.Townsley et al.

NASA RELEASES NEW VIEW OF THE ORION NEBULA

The photo and excerpt below are from the NASA website:
This new view of the Orion Nebula highlights fledgling stars hidden in the gas and clouds. It shows infrared observations taken by NASA's Spitzer Space Telescope and the European Space Agency's Herschel mission, in which NASA plays an important role. Stars form as clumps of this gas and dust collapses, creating warm globs of material fed by an encircling disk. These dusty envelopes glow brightest at longer wavelengths, appearing as red dots in this image. In several hundred thousand years, some of the forming stars will accrete enough material to trigger nuclear fusion at their cores and then blaze into stardom. Spitzer is designed to see shorter infrared wavelengths than Herschel. By combining their observations, astronomers get a more complete picture of star formation. The colors in this image relate to the different wavelengths of light, and to the temperature of material, mostly dust, in this region of Orion. Data from Spitzer show warmer objects in blue, with progressively cooler dust appearing green and red in the Herschel datasets. The more evolved, hotter embryonic stars thus appear in blue. Infrared data at wavelengths of 8.0 and 24 microns from Spitzer are rendered in blue. Herschel data with wavelengths of 70 and 160 microns are represented in green and red, respectively. This image was released on Feb. 29, 2012. Image Credit: NASA/ESA/JPL-Caltech/IRAM