Archive for the ‘ESA’ Category

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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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3D printers could construct Moonbase

February 1, 2013

by yaska77

London based architects Foster and Partners have revealed designs for a building on the Moon that could be constructed from the material already on its surface.

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Foster+Partners have joined with ESA to test the feasibility of 3D printing using lunar soil (click to enlarge) – Credit: Foster+Partners/ESA

Working with the European Space Agency, the plan involves launching a capsule which includes an inflatable structure to deploy near the Moon’s southern pole. This structure will then be covered with an outer shell built by 3D printers.

The robot operated printers would use soil from the Moon, known as regolith, to build the layered cover.

Designed to initially house four people, the firm said there was plenty of scope for wider expansion.

Multi-dome_base_being_constructed_fullwidth

Once assembled, the inflated domes are covered with a layer of 3D-printed lunar regolith by robots to help protect the occupants (click to enlarge) – Credit: Foster+Partners/ESA

Buildings on Earth by the architect firm include Wembley Stadium and Hong Kong International airport.

We may just get that moonbase yet, children of the 70′s and 80′s :)

Sources:

Foster and Partners
European Space Agency

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Hubble’s eXtreme view of the Universe

September 26, 2012

by yaska77

When it comes to looking into and imaging the past, the Hubble Space Telescope continues to produce shots of breathtaking wonder.

Called the eXtreme Deep Field, or XDF, the image below was assembled by combining 10 years of NASA Hubble Space Telescope photographs taken of a patch of sky at the center of the original Hubble Ultra Deep Field.

Astronomers have assembled a new, improved portrait of mankind’s deepest-ever view of the universe (click to enlarge) – Credit: NASA; ESA; G. Illingworth, D. Magee, and P. Oesch, University of California, Santa Cruz; R. Bouwens, Leiden University; and the HUDF09 Team

The Hubble Ultra Deep Field is an image of a small area of space in the constellation Fornax (latin for Furnace) located in the southern sky, far away from the glare of the Milky Way, and was created using Hubble Space Telescope data from 2003 and 2004.

By collecting faint light over many hours of observation (around 500 hours) it revealed thousands of galaxies, both nearby and very distant, making it the deepest image of the universe ever taken.

A finger held at arm’s length would appear to be about twice the width of the moon in this image (click to enlarge) – Credit: NASA/ESA and Z. Levay, STScI; Moon Image Credit: T. Rector/I. Dell’Antonio/NOAO/AURA/NSF

The new full-color XDF image contains about 5,500 galaxies even within its smaller field of view. The faintest galaxies are one ten-billionth the brightness of what the human eye can see.

The history of galaxies – from soon after the first galaxies were born to the great galaxies of today, like our Milky Way – is laid out in this one amazing image.

Garth Illingworth of the University of California at Santa Cruz (principal investigator of the Hubble Ultra Deep Field program) said, “The XDF is the deepest image of the sky ever obtained and reveals the faintest and most distant galaxies ever seen. XDF allows us to explore further back in time than ever before”.

It should certainly keep astronomers busy for a while, at least until the James Webb Space Telescope launches! With it’s specialised infrared instruments it is expected to find even fainter galaxies that existed when the universe was just a few hundred million years old.

You can read more details on the NASA Hubble Website here.  Galactic!

Source: NASA

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Hubble spies a beautiful butterfly

November 15, 2011

by yaska77

The bright clusters and nebulae of our night sky are often named after insects or flowers, and NGC 6302 is no exception!

What a massive wingspan! The Butterfly Nebula (NGC 6302) as imaged from Hubble in 2009 (click to enlarge) - Credit: NASA/ESA & Hubble SM4 ERO Team

With an estimated surface temperature of around 250,000°C, the central star of this particular planetary nebula is exceptionally hot, though its bright ultraviolet light is hidden from view by a dense ring of dust.

This amazingly detailed close-up image of the dying star’s nebula was captured by the Hubble Space Telescope soon after its upgrade in 2009.

This “Butterfly Nebula” lies about 4,000 light-years away in the constellation of Scorpius (the Scorpion).

Utterly beautiful and totally awesome :)

Source: NASA Astronomy Picture of the Day (13th November)

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Galaxy pile-up in Pandora’s Cluster

June 23, 2011

by yaska77

Scientists studying Abell 2744, nicknamed Pandora’s Cluster, have used both ground based and space telescopes to determine the giant galaxy cluster was formed by a simultaneous pile-up of at least four seperate smaller galaxy clusters.

Observations taken using the Hubble Space Telescope, the European Southern Observatory’s Very Large Telescope (VLT), the Japanese Subaru telescope, and NASA’s Chandra X-ray Observatory suggest this giant crash took place over 350 million years.

Click to enlarge in new tab - Credit: NASA/ESA/J. Merten (Institute for Theoretical Astrophysics, Heidelberg/Astronomical Observatory of Bologna) and D. Coe (STScI)

The galaxies in the cluster make up less than 5% of its mass, with about 20% being gas that is so hot it only appears in X-rays (coloured red in the image above). The distribution of invisble dark matter makes up the remaining 75%, appearing in the image as blue areas.

Dark matter does not emit, absorb, or reflect light, but can be detectable through its gravitational attraction. To help locate this elusive substance a phenomenon known as gravitational lensing was used. This is the bending of light from distant galaxies as they pass through the gravitational field created by the cluster.

This method provided a series of distortions in the images from the Hubble and VLT observations. After careful analysis of these distortions the team involved was able to accurately map where the dark matter is.

Chandra mapped the distribution of hot gas in the cluster.

The information gathered suggests the galactic pile-up separated the hot gas (which interacts upon collision) and the dark matter (which does not) so that they now lie apart from each other, and from the visible galaxies.

More information direct from NASA here

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