Posts Tagged ‘infrared’

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Three years of pioneering observation ends

April 30, 2013

by tte-77

Iconic image of ESA’s Herschel space observatory set against a background of stellar nursery W40, 1000 light-years away in the constellation Aquila. Image credit: ESA and SPIRE & PACS consortia, Ph. André (CEA Saclay) for Gould’s Belt Key Programme Consortia

ESA’s Herschel space observatory has as planned exhausted  its supply of liquid helium coolant forcing its optics offline. In effect, Herschel has gone blind which ends over three years of pioneering observations of the cool Universe.  Herschel was Launched in May 2009 and, with a primary mirror 3.5 m across, is/was the largest, most powerful infrared telescope flown in space.

Herschel observed near-infrared and sub-millimeter wavelengths that are abundant inside star-forming nebulae and young galaxies.  Running out of coolant has declared the mission officially over.  In order to be sensitive to the extreme wavelengths Herschel  needed to be cooled to near-absolute zero (-273 degrees Celsius or -459 F).

The space telescope was the most advanced of its kind making groundbreaking discoveries of the nature of our universe.  Although Herschel has died, other observatories are geared to observe in the sane wavelengths.  In Chile the ground-based ALMA array is now online and is able to access sub-millimeter wavelengths with the 747-mounted SOFIA telescope accessing near-infrared wavelengths.

So in three years how much data did Herschel collect.  “Herschel has exceeded all expectations, providing us with an incredible treasure trove of data that will keep astronomers busy for many years to come,” says Prof. Alvaro Giménez, ESA’s Director of Science and Robotic Exploration.

The figures are impressive.  Herschel has made over 35000 scientific observations, gathering more than 25000 hours of data from about 600 observing programmes with a further 2000 hours of calibration observations also contributing to the dataset.

“Although this is the end of Herschel observing, it is certainly not the end of the mission – there are plenty more discoveries to come,” says Dr Pilbratt.

“We will now concentrate on making our data accessible in the form of the best possible maps, spectra and various catalogues to support the work of present and future astronomers. Nevertheless we’re sad to see the end of this phase: thank you, Herschel!”

The thumbnail images below show just a snippet of views from Herschel over the last three years.  Make sure you visit the official ESA Space in Images page and search for Herschel for more ‘cool’ images.

All images copyrighted to ESA/Herschel, PAC and SPIRE

The image of Andromeda (M31) is awesome, it uses both the PACS (Photodetecting Array Camera and Spectrometer) and SPIRE (Spectral and Photometric Imaging Receiver) instruments to observe at infrared wavelengths of 70 um (blue), 100 um (green) and 160 um and 250 um combined (red).

Herschel will continue communicating with its ground stations now that the helium is exhausted, during which a range of technical tests will be performed.

Finally, in May, it will be propelled into its long-term stable parking orbit around the Sun.

Source: ESA

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ESO Top 100 Images – 5-1

December 31, 2011

by tte-77

So here we are with the final five images from the ESO Top 100 Images series. The 340-million pixel starscape from Paranal at number 4 is without doubt one of our favourite from the series (view as 1280px × 734px image here). We hope you have enjoyed viewing these 100 images over the last few months as much as we have. Enjoy!

NGC 2264 and the Christmas Tree cluster

# 5 - NGC 2264 and the Christmas Tree cluster - Credit: ESO

4 A 340-million pixel starscape from Paranal Credit:  ESO/S. Guisard (www.eso.org/~sguisard)

# 4 - A 340-million pixel starscape from Paranal - Credit: ESO/S. Guisard (www.eso.org/~sguisard)

VST image of the star-forming region Messier 17

# 3 - VST image of the star-forming region Messier 17 - Credit: ESO/INAF-VST/OmegaCAM. Acknowledgement: OmegaCen/Astro-WISE/Kapteyn Institute

The Helix Nebula

# 2 - The Helix Nebula - Credit: ESO

VISTA's infrared view of the Orion Nebula

# 1 - VISTA's infrared view of the Orion Nebula - Credit: ESO/J. Emerson/VISTA. Acknowledgment: Cambridge Astronomical Survey Unit

To view the previous images from the countdown visit the links below.
10-6 | 15-11 | 20-16 | 25-21 | 30-26 | 35-31 | 40-36 | 45-41 | 50-46 | 55-51 | 60-56 | 65-61 | 70-66 | 75-71 | 80-76 | 85-81 | 90-86 | 95-91 | 100-96

Subscribe via the WordPress tab (side panel) or follow on Twitter for weekly updates to this dedicated series of stunning shots.

* ESO Top 100 Images series positions correct at time of post.

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Confused galaxy spins both ways

June 20, 2011

by yaska77

This NASA/ESA Hubble Space Telescope image of NGC 7479 (released today) has been created from observations of both visible and near-infrared wavelengths.  The tightly wound arms of the spiral galaxy create an inverted ‘S’, as they spin in an anticlockwise direction.

NGC 7479 (click to enlarge in new tab) - Credit: ESA/Hubble/NASA

At radio wavelengths however, this galaxy (nicknamed the Propeller Galaxy) spins the other way, with a jet of radiation that bends in the opposite direction to the stars and dust in the arms of the galaxy.

Astronomers believe the radio jet in NGC 7479 was put into its strange backwards spin following a merger with another galaxy.

Star formation is reignited by such galactic collisions, and NGC 7479 is undergoing starburst activity, with many bright, young stars visible in the spiral arms and disc. The three brightest stars in the image are larger because they lie between NGC 7479 and Hubble.

Read the full article here

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Spitzer spies beautiful green ring nebula

June 17, 2011

by yaska77

The Spitzer Space Telescope has captured this stunning false colour image of a vast cloud of gas and dust where new stars have recently formed.

Astronomers believe rings like this are sculpted by the powerful light of giant “O” stars, the most massive type of star known to exist. Named RCW 120 this region of hot gas and glowing dust can be found by the tail of the constellation Scorpius.

The green ring of dust is actually glowing in infrared colors that our eyes can’t see, but show up brightly when viewed by Spitzer’s infrared detectors. At the center of the ring are a couple of giant stars whose intense ultraviolet light carved out the bubble, though they blend in with the other stars when viewed in infrared.

Credit: NASA/JPL-Caltech

Rings like this are so common in Spitzer’s observations that astronomers have even enlisted the help of the public to help find and catalog them all. Budding amateur astronomers interested in joining the search as a “citizen scientist” can visit “The Milky Way Project“, part of the “Zooniverse” of public astronomy projects.

The flat plane of our galaxy is located toward the bottom of the full picture (click above to enlarge, it’s the green haze seen at the bottom of the full image), with the ring is just above it.

Green Lantern‘s power ring perhaps?!

Source: NASA/JPL-Caltech

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NASA Image – James Webb Space Telescope

April 15, 2011

by yaska77

Despite the fact I keep wanting to call it the James Woods Space Telescope, this NASA “Image of the Day” is too cool not to bring to your attention.

Credit: NASA/MSFC/David Higginbotham

This section of the James Webb Space Telescope represents the first of 18 that make up the primary mirror for space observations.  It’s due to begin cryogenic testing at NASA’s Marshall Space Flight Center to make sure it will perform as expected in the extreme temperatures in space, before integration into the telescope’s permanent housing structure.

The James Webb Space Telescope is scheduled for launch in 2014.

Visit the JWST site here

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