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Karl Henry Spitzer
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Karl Henry Spitzer
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Karl Henry Spitzer
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Karl Henry Spitzer
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Karl Heinrich Spitzer
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Richard Wagner and Daniel Spitzer
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The Eagle nebula. Spitzer Space Telescope.
The Eagle nebula. Spitzer Space Telescope.
The Eagle nebula. Spitzer Space Telescope.
False-coloured image by the Spitzer Space Telescope.
This swirling landscape of stars is known as the North America nebula. Spitzer.
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
A false-colour image of Cassiopeia A
The false-colour Spitzer images reveal a different side of the Trifid Nebula
This swirling landscape of stars is known as the North America nebula. Spitzer.
This swirling landscape of stars is known as the North America nebula. Spitzer.
Heinrich Spitzer from Bisenz in Moravia, 1848 (etching)
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Open cluster of Pleiades seen in infrared - The Pleiades open cluster seen in infrared - Clouds of dust in the Pleiades cluster seen in infrared by the Spitzer space telescope. The Pleiades star cluster contains about 500 stars formed 100 million years ago. It is located 440 light years from Earth, in the constellation Taurus. The Pleiades, located more than 400 light - years away in the Taurus constellation, is a star cluster born when dinosaurs still roamed the Earth, about 100 million years ago. It is significantly younger than our 5 - billion - year - old sun. The brightest members of the cluster, also the highest - mass stars, are known in Greek mythology as two parents, Atlas and Pleione, and their seven daughters, Alcyone, Electra, Maia, Merope, Taygeta, Celaeno and Asterope. There are thousands of additional lower - mass members, including many stars like our sun. Some scientists believe that our sun grew up in a crowded region like the Pleiades, before migrating to its present, more isolated home. The infrared image from Spitzer highlights the filaments, colored yellow, green and red in this view, made up of dust associated with the cloud through which the cluster is traveling. The densest portion of the cloud appears in yellow and red, and the more diffuse outskirts are shown in green hues. One of the parent stars, Atlas, can be seen at the bottom left, while six of the sisters are visible at top. Additional stars in the cluster are sprinkled throughout the picture in blue
South Pillar region of the star-forming region called the Carina Nebula
This image shows the Orion nebula, a nebula where stars are born. Spitzer.
This image shows the Orion nebula, a nebula where stars are born. Spitzer.
Spitzer Turm (Pointed Tower), Wertheim Am Main, Baden-Wurttemberg, Germany (photo)
This image shows the Orion nebula, a nebula where stars are born. Spitzer.
This swirling landscape of stars is known as the North America nebula. Spitzer.
This image shows the Orion nebula, a nebula where stars are born. Spitzer.
PROSECUTOR KURT SPITZER NEWS CONFERENCE, 2000-04-06 (photo)
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This swirling landscape of stars is known as the North America nebula. Spitzer.
Composite image of the Large Magellanic Cloud
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.
Spitzer Space Telescope infrared composite images how the Andromeda galaxy.
Star Formation in Cassiopee - Star Formation in Cassiopeia - This star-forming region, called W5, is located approximately 6500 light years ago in the constellation Cassiopee. Several generations of stars appear on this cliche; the older ones are the blue stars in the centre of the two cavities; the younger stars are grouped at the edges of these cavities and at the ends of the gas pillars or they appear like pink dots; the white areas are home to the very young stars in formation. In this infrared image, heated dust appears in red, dense gas clouds appear in green. Composite image obtained by the Spitzer space telescope in 2006 and 2007. Generations of stars can be seen in this infrared portrait from Nasa's Spitzer Space Telescope. In this wispy star - forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant - trunk - like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds. W5 spans an area of sky equivalent to four full moons and is about 6,500 light - years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours. Like other massive star - forming regions, such as Orion and Carina, W5 contains large cavities that were carved out by radiation and winds from the region's most massive stars. According to the theory of triggered star - formation, the carving out of these cavities pushes gas together, causing it to ignite into successive generations of new stars. This image contains some of the best evidence yet for the triggered star - formation theory. Scientists analyzing the photo have been able to sho
Infrared view of the Andromeda galaxy - Composite of three different wavelengths 24 microns (blue), 70 microns (green), and 160 microns (red). Using these three bands, we can know the temperature differences of the dust: the warmest are the brightest at 24 microns and the coldest shine at 160 microns. The blue/white areas contain the hottest dust. View obtained by Spitzer space telescope on 25 August 2004. The multi - wavelength view of Andromeda combines images taken at 24 microns (blue), 70 microns (green), and 160 microns (red). Using all three bands from the multiband imaging photometer allows astronomers to measure the temperature of the dust by its color. The warmest dust is brightest at 24 microns while the coolest is most evident at 160 microns. The blue/white areas have the hottest dust, as seen in the bulge and in the star - forming areas along the arms. The cooler dust floating further out in the ring and arms are in the redder regions. The data were taken on August 25, 2004 by Spitzer space telescope