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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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Ideal SETI-target planets and K-type stars

April 25, 2013

by tte-77

The Kepler-62 system – home to two habitable zone worlds. The small shining object to the right of Kepler-62f is Kepler-62e. Image credit: NASA Ames/JPL-Caltech.

Its been far too long since I contributed to Sky-Watching on a regular basis. On that sudden note here’s the first post in a while and its exoplanet related.

In the search for extraterrestrial life, NASA’s Kepler team have announced the discovery of Kepler-62 – a multiple planet system composed of five Earth and super-Earth sized planets, two of which are habitable zone worlds, orbiting an orange dwarf or to be precise a K-type main-sequence star.

Ok, so this is cool news right, and a K-type star too.  I’m intrigued.  Has Kepler found ideal SETI-target planets?

K-type stars are of particular interest in the search for other life because they are about three to four times as abundant as sun-like stars, making planet searches easier. K-type stars are also stable on the main sequence for a very long time, around 15 to 30 billion years which is two to three times longer than our own sun  and this may create an opportunity for life to evolve on the terrestrial planets orbiting them.

An artistic view of the system seen from Kepler-62f. Image credit: Danielle Futselaar/SETI Institute

The outermost planet, named Kepler-62f (see image) is about 1.4 times Earth’s radius and has a period of 267 Earth days. If Kepler-62f is a rocky planet with a similar atmosphere to Earth, sitting in the stars habitable zone it could host liquid water on its surface. Kepler-62e, also in the habitable zone is 1.6 times the Earth’s radius with a period of 122 Earth days, it could also host liquid water on its surface.

The authenticity of this multiple planet system was confirmed by a statistical analysis based on previous discoveries of multiple planets by Kepler as the detection of these planets was indirect.  The Kepler astronomers observed gradual loss of the host star’s brightness due to the passage of a planet in the line of sight, and not the planets themselves.  Speaking about the detection process Jason Rowe, Research Scientist at the Carl Sagan Center of the SETI Institute and co-author of the work said “Such calculations are only possible because of the thousands of additional transiting extrasolar planets that Kepler has discovered”.

About the discoveries Jon Jenkins,  Senior Scientist at the Carl Sagan Center of the SETI Institute and co-author of the work said “These discoveries move us farther down the road to discovering planets similar to Earth. While we don’t know if Kepler-62e and f are rocky or whether they have liquid water pooling on their surfaces, their existence shows that the incidence of small worlds in the habitable zone of Sun-like stars is high.

Thus we can look forward to the discovery and detailed characterization of Earth’s cousins in the years and decades to come by future missions and telescopes.”

So there you go – exoplanets, K-type stars, some smart scientists from the SETI Institute, nice images and a post with a final thought…

If Kepler has found ideal SETI-target planets, sort the funding and bring on the future missions and telescopes.

Sources: SETI / spacedaily.com

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Explosion on Jupiter captured by amateur astronomer

September 14, 2012

by tte-77

On Monday 10 September in Wisconsin, USA amateur astronomer Dan Petersen saw something incredible while viewing Jupiter from his backyard – a bright white flash on the planet’s surface.

The unexpected explosion lasted for about two seconds and appeared to be about 100-miles wide, Petersen wrote on community blog CloudyNights.com. “My best guess is that it was a small undetected comet that is now history,” he added.

In Dallas, Texas, another amateur astronomer George Hall happened to capture the flash on video. Watch it below.

The possible crash adds to the theory that Jupiter acts as an impact shield for Earth, NBC News’ Alan Boyle explains:

Astronomers suspect that giant Jupiter’s gravitational pull serves as a cosmic shield, sweeping up incoming objects that would have a deadlier effect if they were to slam into our planet. Some scientists say that without Jupiter, life on Earth wouldn’t have had much of a chance.

Thanks Jupiter from all at Sky-Watching!

Source: businessinsider

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Holy GRAIL – Far side of the moon

February 2, 2012

by tte-77

On 1 February NASA released the first video from GRAIL, its newest moon mission. As part of the mission twin spacecraft Ebb and Flow are orbiting the moon, and Ebb has captured a video of the moon’s far side. Awesome!

The Gravity Recover and Interior Laboratory or GRAIL for short consists of two robotic probes – GRAIL-A and GRAIL-B (named Ebb and Flow by school children in January 2012). The probes are orbiting the moon in tandem, using variations in the radio signals between them to help study the moon’s gravity with the overall goal of the mission understanding more about the formation of our solar system.

GRAIL is the first robotic planetary mission to carry equipment for the sole purpose of education. One piece of equipment that both probes carry is a MoonKAM (Moon Knowledge Acquired by Middle school students), which will allow students (in the U.S) to study specific parts of the moon helping inspire them to consider careers in science and engineering.

Thumbs up to NASA on this one.

Find out more about GRAIL here.

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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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