Posted on by Tammy Plotner

Venus Express Discovers Venusian Ozone Layer

Venus Express has two solar cell panels per wing comprising alternating rows of standard triple junction solar cells as well as highly reflective mirrors to reduce the operating temperatures. There is twice as much sunlight in Venus's orbit as there is in Earth's orbit, plus additional thermal input from the Venusian surface and atmosphere – 75% of sunlight being reflected up from it. In certain cases, this results in Venus Express receiving an equivalent of the thermal input from 3.5 Suns. Credit: ESA

Every day brings on new discoveries and now ESA’s Venus Express spacecraft has delivered another… the red-hot planet has an ozone layer. Located high in the Venusian atmosphere, this planetary property will help us further understand how such features compare to Earth and Mars – along with refining our search for extra-terrestrial life.

This wonderful discovery was made while Venus Express was busy watching stars at the periphery. When seen through the planet’s atmosphere, the SPICAV instrument was able to distinguish gas types spectroscopically. By picking apart the wavelengths, ozone was detected through its absorption of ultraviolet light. It forms when sunlight breaks down the carbon dioxide molecules and releases oxygen. From there, they are distributed by planetary winds where the oxygen atoms will either combine into two-atom oxygen molecules, or form three-atom ozone.

“This detection gives us an important constraint on understanding the chemistry of Venus’ atmosphere,” says Franck Montmessin, who led the research.

This is an animation of Venus Express performing stellar occultation at Venus. Venus Express is the first mission ever to apply the technique of stellar occultation at Venus. The technique consists of looking at a star through the atmospheric limb. By analysing the way the starlight is absorbed by the atmosphere, one can deduce the characteristics of the atmosphere itself. Credits: ESA (Animation by AOES Medialab)

To date, ozone has been the sole property of Earth and Mars – but this type of discovery method could aid astronomers in searching for life on other worlds. Why is it important? Because ozone absorbs most of the Sun’s harmful ultra-violet rays… and because it is believed to be a by-product of life itself. When combined with carbon dioxide, this could create a signature as a strong signal for life. But don’t get too excited at the prospects, yet. The amount of ozone detected is also critical to refining models. It will need to be at least 20% of Earth’s value to even be considered.

“We can use these new observations to test and refine the scenarios for the detection of life on other worlds,” says Dr Montmessin.

While we know that chances are almost non-existent that Venus has life, it still brings it one step closer to planets like Mars and Earth.

“This ozone detection tells us a lot about the circulation and the chemistry of Venus’ atmosphere,” says Hakan Svedhem, ESA Project Scientist for the Venus Express mission. “Beyond that, it is yet more evidence of the fundamental similarity between the rocky planets, and shows the importance of studying Venus to understand them all.”

Original Story Source: ESA Space Science News.

Posted on by Tammy Plotner

Looking Into The Eye Of A Monster – Active Galaxy Markarian 509

Active galaxy Markarian 509 as seen by the Hubble Space Telescope's WFPC2. Credits: NASA, ESA, J. Kriss (STScI) and J. de Plaa (SRON)

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“The world is a vampire, sent to drain… Secret destroyers, hold you up to the flames…” Ah, yes. It’s the biggest vampire of all – the supermassive black hole. In this instance, it’s not any average, garden-variety black hole, but one that’s 300 million times the mass of the Sun and growing. Bullet with butterfly wings? No. This is more a case of butterfly wings with bullets.

An international team of astronomers using five different telescopes set their sites on 460 million light-year distant Markarian 509 to check out the action surrounding its huge black hole. The imaging team included ESA’s XMM-Newton, Integral, NASA/ESA Hubble Space Telescope, NASA’s Chandra and Swift satellites, and the ground-based telescopes WHT and PARITEL. For a hundred days they monitored Markarian 509. Why? Because it is known to have brightness variations which could mean turbulent inflow. In turn, the inner radiation then drives an outflow of gas – faster than a speeding bullet.

“XMM-Newton really led these observations because it has such a wide X-ray coverage, as well as an optical monitoring camera,” says Jelle Kaastra, SRON Netherlands Institute for Space Research, who coordinated an international team of 26 astronomers from 21 institutes on four continents to make these observations.

And the vampire reared its ugly head. Instead of the previously documented 25% changes, it jumped to 60%. The hot corona surrounding the black hole was spattering out cold gas “bullets” at speeds in excess of one million miles per hour. These projectiles are torn away from the dusty torus, but the real surprise is that they are coming from an area just 15 light years away from the center. This is a lot further than most astronomers speculate could happen.

“There has been a debate in astronomy for some time about the origin of the outflowing gas,” says Kaastra.

But there’s more than just bullets here. These new observations at multiple wavelengths are showing the coolest gas in the line of sight toward Markarian 509 has 14 different velocity components – all from different locations at the galaxy’s heart. What’s more, there’s indications the black hole accretion disc may have a shield of gas harboring temperatures ranging in the millions of degrees – the motivating force behind x-rays and gamma rays.

An artist's impression of the central engine of an active galaxy. A black hole is surrounded by matter waiting to fall in. Fearsome radiation from near the black hole drives an outflow of gas. Credits: NASA and M. Weiss (Chandra X-ray Center)

“The only way to explain this is by having gas hotter than that in the disc, a so-called ‘corona’, hovering above the disc,” Jelle Kaastra says. “This corona absorbs and reprocesses the ultraviolet light from the disc, energising it and converting it into X-ray light. It must have a temperature of a few million degrees. Using five space telescopes, which enabled us to observe the area in unprecedented detail, we actually discovered a very hot ‘corona’ of gas hovering above the disc. This discovery allows us to make sense of some of the observations of active galaxies that have been hard to explain so far.”

To make things even more entertaining, the study has also found the signature of interstellar gas which may have been the result of a one-time galaxy collision. Although the evidence may be hundreds of thousands of light years away from Mrk 509, it may have initially triggered this activity.

“The results underline how important long-term observations and monitoring campaigns are to gain a deeper understanding of variable astrophysical objects. XMM-Newton made all the necessary organisational changes to enable such observations, and now the effort is paying off,” says Norbert Schartel, ESA XMM-Newton Project Scientist.

Ah, Markarian 509… “Despite all my rage… I am still just a rat in cage.”

Original Story Source: ESA News. For Further Reading: Multiwavelength Campaign on Mrk 509 VI. HST/COS Observations of the Far-ultraviolet Spectrum.

Posted on by Jason Rhian

ESA’s ExoMars Mission in Jeopardy

NASA has stated that it cannot provide one of the Atlas rockets required to launch the ExoMars mission that it has partnered with ESA on. Image Credit: ESA

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The European Space Agency’s “ExoMars” mission is under threat of cancellation. NASA and ESA heads will meet on Monday, Oct. 3 to decide how much more can be cut from the rapidly slimming mission. This meeting comes on the heels of NASA’s latest round of cuts – which means that the U.S. space agency cannot provide ESA with the Atlas V rocket that was slated to launch part of the mission.

ESA still might be able to keep ExoMars going if it can acquire a Proton rocket under the trade system that the agency is working to negotiate with Russia. Barring that? ExoMars will more-than-likely be cancelled. ESA had been hoping to send a diverse science package to the red planet. ExoMars is currently comprised of a communications relay system, descent and landing modules and a rover that is similar in design to the Mars Exploration Rovers Spirit and Opportunity which have been operating on Mars for the past seven years.

The ExoMars Trace Gas Orbiter was originally set to launch in 2016, now its future is uncertain. Image Credit: ESA

NASA Administrator Charles Bolden and ESA Director-General Jean-Jacques Dordain are scheduled to meet in Cape Town, South Africa, during the International Astronautical Congress. During this meeting they are set to discuss one of two options that are left for their joint Mars expedition. The first is a single 2018 launch that will include a NASA-ESA rover and communications package. The second will be to try and maintain, despite the issues with the launch vehicle, the planned 2016 launch.

If a rocket can somehow be procured and the current schedule maintained, ExoMars would be a two launch affair with the Atlas V launching one of the mission’s components and another launch vehicle transporting the remainder. If the mission is saved, but scaled back further, only a single launch would take place in 2018. The Proton rocket scenario appears to be a last-ditch effort to salvage the program at this time. The final deciding factor as to whether-or-not ESA can save the program, to some degree, in its current configuration – depends on ESA obtaining a rocket to replace the Atlas V which NASA says it can no longer provide.

NASA had originally stated that it would provide two Atlas V rockets for the mission, the space agency has taken at least one of these off off the table recently. Photo Credit: ULA

ESA has estimated that either way, the mission will cost them the same 850 million euros ($1.36 billion) that it has already garnered from the nations that comprise the European Union. This is largely due to the fact that ESA has already spent the money to procure the materials and services needed for the orbiter component of the mission.
The primary issue that has continued to threaten mission is the poor state of the economy – both in the U.S. and Europe.

ExoMars started out as a rover and a separate ground station, and was originally set to launch in 2011 on a Soyuz Fregat rocket. In 2009 ESA signed into the Mars Joint Exploration Initiative with NASA. This agreement with NASA both pushed back the launch of the mission considerably and started ExoMars down the path to where it currently finds itself.

ExoMars has been changed repeatedly since its inception and now it is facing possible cancellation. Image Credits: ESA

Posted on by Jason Rhian

ATK and Astrium’s Liberty Launcher Added to NASA’s Commercial Crewed Roster

The Liberty launch vehicle, produce by ATK and Astrium, has been added to the fleet of commercial rockets and spacecraft that are being developed for NASA. Image Credit" ATK

[/caption]CAPE CANAVERAL, Fla – Liberty has wings. That is to say that the launch vehicle proposed by Alliant Techsystems or ATK as they are more commonly known has been given the green light by NASA – albeit unfunded – as part of a Space Act Agreement. The announcement was made at the Kennedy Space Center press site’s auditorium in Florida Tuesday at 3 p.m. EDT. With ATK’s addition – the fleet of potential spacecraft and launch vehicles could mean that the space agency will not only be able to return to human space flight operations sooner – but with a more diverse range of vehicles to do so as well.

The proposal to use the Liberty launch vehicle, which is comprised of a five-segment solid rocket booster (similar to the four-segment SRB utilized during the shuttle program) and an Ariane V upper stage could reduce the human space flight “gap” that NASA is currently experiencing. As the company that produces the Ariane V, Astrium, is a European firm this deal also works to fulfill the White House’s wishes that space endeavors be conducted on an international level. More importantly – ATK has stated that they could be ready to launch as early as 2015.

Liberty is a combination of so-called "legacy" hardware. The first stage is a modified shuttle Solid Rocket Booster and the upper stage comes from the Ariane V rocket. Image Credit: ATK

After the Ares I launcher was scrapped along with most of the rest of the Constellation Program by the Obama Administration ATK looked into ways to preserve the project. ATK was one of the first to see the commercial crewed writing on the wall and went to work revamping the project. With a far lower cost, international partner and a new paint job – Liberty was born.

The rationale behind why the Liberty announcement was made at KSC – was highlighted by ATK’s Vice-President for Test and Research Operations, Kent Rominger.

“We want to launch Liberty from Kennedy Space Center,” said Rominger. “Our concept of operations is based around KSC assets such as the Vehicle Assembly Building (VAB). Liberty will be processed much in the same manner as the space shuttle was – so KSC is central to Liberty’s operations.”

With the inclusion of Liberty – most elements of the Constellation Program are back in place. Liberty could potentially be the launch vehicle that sends astronauts to orbits, the Space Launch System which closely resembles the Ares V is currently in development, the Orion Multi-Purpose Crew Vehicle is still in place as is the Lunar Electric Rover (although it has been renamed the “Space Exploration Vehicle”). The only element that has yet to be resurrected is the over-arching ‘Vision for Space Exploration’ – which directed NASA to go to the “Moon, Mars and Beyond.”

If all works out with NASA’s Commercial Crew Program NASA could see a problem that faced the space agency in the wake of the Challenger and Columbia accidents – erased. After the loss of each of the orbiters NASA was unable to launch astronauts to orbit for a period of roughly two years. With Liberty and man-rated versions of United Launch Alliance’s Atlas and SpaceX’s Falcon 9 rocket – if one of these launch vehicles experienced an in-flight anomaly NASA could simply switch to another launcher while any problem with another rocket is being investigated. This of course depends on whether-or-not NASA receives the funding to accomplish this.

The Liberty rocket has been designed to accomodate a wide-range of potential spacecraft. Image Credit: ATK
Posted on by Ray Sanders

HARPS Hauls in Over Fifty New Exoplanets

Artist’s impression of a Super-Earth planet orbiting a Sun-like star. Credit: ESO/M. Kornmesser

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Yesterday astronomers with the High Accuracy Radial velocity Planet Searcher or HARPS, announced a record-breaking discovery of more than fifty new exoplanets. This is the largest batch of confirmed extra solar planets ever announced at once. Another reason the discovery is noteworthy is that sixteen of the planets that were detected fall under the “super-Earth” classification, meaning the planets are thought to be rocky worlds less than ten times Earth’s mass.

The HARPS team, led by Michel Mayor from the University of Geneva, used the 3.6-metre telescope at ESO’s La Silla Observatory in Chile and claim their spectrograph instrument on the telescope is the most successful planet-finder to date. The team’s data suggests that about 40% of stars similar to our Sun have at least one planet less massive than Saturn.

The announcement of the big planetary haul was made at the Extreme Solar Systems II exoplanet conference taking place this week in Wyoming in the US.

How did Mayor and his team discover so many planets, and how are they certain of their findings?

The HARPS instrument uses a technique called “radial velocity”. Essentially, the instrument detects the slight movement of a star moving toward and away from observers on Earth. The changes in radial velocity shift the star’s light spectrum. When the star moves away from observers on Earth, the light is shifted to longer, redder wavelengths, called redshifting. When the star moves toward Earth, the opposite happens and the star’s light is blueshifted. Through various hardware and software upgrades over the years, HARPS is now so sensitive, it can detect radial velocities of about 1 meter per second and exoplanets less than twice the mass of Earth.

The radial velocity method of exoplanet detection that HARPS uses is different from say, the Kepler mission which uses the “transit” method to detect exoplanet candidates. The transit method, comparatively speaking, still uses the light from a distant star, but instead of measuring redshift or blue shift, Kepler instead looks for a dimming of the star’s light as exoplanets pass in front of their host star.

HARPS has been operating for the past eight years, using the radial velocity technique to discover over 150 new planets. HARPS has also detected a considerable portion of the known exoplanets less massive than Neptune (seventeen Earth masses). “The harvest of discoveries from HARPS has exceeded all expectations and includes an exceptionally rich population of super-Earths and Neptune-type planets hosted by stars very similar to our Sun. And even better — the new results show that the pace of discovery is accelerating,” said Mayor.

Image of the star HD 85512 using red and blue filters. The diffraction spikes are due to the telescope itself and are not caused by the star . Image Credit: ESO/Davide De Martin and Digitized Sky Survey 2.
One particular exoplanet Mayor and his team cited was HD85512b, estimated to be just over 3.5 times Earth’s mass. “The detection of HD 85512 b is far from the limit of HARPS and demonstrates the possibility of discovering other super-Earths in the habitable zones around stars similar to the Sun,” added Mayor. HD 85512b also happens to be situated on the edge of the “habitable zone” around its parent star – a zone where conditions could allow for water on the surface of a planet orbited in said zone.

Based on these latest findings, as well as previous HARPS discoveries, the team plans to install an exact copy of the HARPS instrumentation on the Telescopio Nazionale Galileo in the Canary Islands. The duplicate HARPS will allow scientists to survey stars in the northern sky.

“In the coming ten to twenty years we should have the first list of potentially habitable planets in the Sun’s neighborhood,” Mayor said. “Making such a list is essential before future experiments can search for possible spectroscopic signatures of life in the exoplanet atmospheres.”

The total tally of confirmed planets orbiting other stars stands at about 600, depending on who you ask. The Jet Propulsion Laboratory’s PlanetQuest website, shows 564 exoplanets while the Extrasolar Planets Encyclopedia, a database kept by astrobiologist Jean Schneider of the Paris-Meudon Observatory, lists 645 alien worlds. The discrepancy comes because PlanetQuest doesn’t add to their total until an exoplanet has been completely confirmed.

Source: ESO Press Release

Ray Sanders is a Sci-Fi geek, astronomer and space/science blogger. Visit his website Dear Astronomer and follow on Twitter (@DearAstronomer) or Google+ for more space musings.

Posted on by Jason Rhian

NASA Facing Astronaut Deficit

A National Research Council report states that NASA's ability to conduct normal human space flight operations could be hampered if it cannot maintain a robust astronaut corps. Photo Credit: Jason Rhian

[/caption]This past December the White House directed the National Academies to review how many astronauts that NASA actually needed to conduct its operations in the post-shuttle era. New findings in a new report are showing that rather than the space agency having too many astronauts – it will have too few to meet mission objectives. The National Research Council (NRC) has released a report showing that NASA is entering into a period where low numbers of qualified astronauts will affect the agency’s ability to conduct human space flight operations.

NASA once had a strong, stable astronaut corps but the agency has slowly but surely saw those numbers dwindle. In 1999 NASA had 150 astronauts today it has 61 – with more leaving the space agency every month. NASA needs to have a stable corps of space flyers for not only International Space Station operations but also to help develop the Orion Multi-Person Crew Vehicle (MPCV).

With the shuttle program over and the fleet of orbiters on their way to museums, many astronauts are opting to leave the space agency. Photo Credit: Jason Rhian

Moreover NASA needs its astronaut corps to remain stable so as to maintain its agreements with the Russian Federal Space Agency, European Space Agency, Japanese Aerospace Exploration Agency and Canadian Space agency. Fewer astronauts weakens NASA’s ability to fulfill operations that are required under these arrangements.

NASA is losing astronauts at approximately the rate of one every two months. If this exodus is allowed to continue the agency’s ability to conduct normal operations will be dramatically impaired. The NRC report highlights many of the nuances that space flight requires – most of which are missed when one considers space flight. Ground operations, emergency response, training and other elements that are involved with crewed space flight operations.

Astronaut Mark Kelly, who commanded the final flight of the space shuttle Endeavour has announced that he will leave NASA effective Oct. 1, the commander of STS-133, the final flight of Discovery, has already departed the space agency. Photo Credit: Jason Rhian

For many astronauts however the appeal of working for the space agency is fading. NASA no longer has clear-cut objectives as it once did. In 2004 plans were announced for NASA to go to the Moon, Mars and then other points in the solar system after the shuttle was retired. In 2010 NASA had the so-called ‘Vision for Space Exploration’ cancelled and the space agency was directed to assist commercial entities in developing technology to reach low-Earth-orbit. It is hoped that once these firms become viable NASA will be freed to fly to an asteroid and then Mars sometime in the 2030s.

NASA is experiencing what some might call a “brain drain” not only are astronauts departing the agency in large numbers – so too are other NASA officials. In recent months NASA’s Chief Technologist Bobby Braun, Safety Chief Bryan O’Connor and the Associate Administrator for Exploration Douglas Cooke (who has been with NASA for 38 years) have either left NASA or signaled their intent to do so.

Posted on by Jason Rhian

Book Review: A Dictionary of the Space Age

A Dictionary of the Space Age covers most aspects of space flight but is somewhat lacking in detail. Image Credit: John Hopkins University & Alan Walters/awaltersphoto.com

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Writing a dictionary is not the same as writing a novel. While it might seem difficult to mess up a dictionary, even one with terminology that is as complicated as that used within the space industry – getting it right can be challenging. For those that follow space flight having such a dictionary can be invaluable. While A Dictionary of the Space Age does meet the basic requirements easily it fails somewhat in terms of its comprehensiveness.

When normal folks, even space enthusiasts watch launches and other space-related events (EVAs, dockings, landings and such) there are so many acronyms and jargon thrown about – that it is extremely hard to follow. With A Dictionary of the Space Age on hand, one can simply thumb through and find out exactly what is being said, making it both easier to follow along and making the endeavor being witnessed far more inclusive. That is as long if you are only looking for the most general of terms. The book is far from complete – but given the complex nature of the topic – this might not have been possible.

Crewed, unmanned, military space efforts and satellites – all have key terms addressed within the pages of this book.

The book is published by The Johns Hopkins University Press and was compiled and written by aerospace expert Paul Dickson. One can purchase the book on the secondary market (Amazon.com) for around $12 (new for around $25). The dictionary also has a Kindle edition which is available for $37.76. Dickson’s previous works on space flight is Sputnik: The Shock of the Century.

Weighing in at 288 pages, the book briefly covers the primary terms used within the space community. In short, if you are interested in learning more about space flight – or wish to do so – this is a good book for you.

Posted on by Tammy Plotner

Exploring Geomagnetic Substorms

Schematic view of Cluster C3 and C1 satellite trajectories Copyright: ESA

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Every now and again, a sudden pulse of energy in Earth’s magnetosphere just cuts loose. As a result, we have a bright polar auroral display. While we’re beginning to understand more about magnetism and the Sun/Earth connection, there’s still a few rogues left in the gallery. Just what is a geomagnetic substorm and what does it do?

Although we’ve known about them for years, the exact process behind a geomagnetic substorm has been a mystery… one that’s being solved with data from missions like ESA’s Cluster spacecraft. Earth is continually being bathed in incoming sheets of electrons and protons – the product of an active Sun. These highly energized particles are simply a part of solar winds flowing from coronal holes and even powerful blasts from events like coronal mass ejections. For the most part, we’re shielded by the magnetosphere – but sometimes a wee bit escapes and collects in the magnetotail – stored like a battery charge. At a point, it’s released… and when it does, it re-arranges our magnetic field lines. The energy then conducts itself along these lines like a filament in a light bulb. When the watts hit the fan? Wow… We have polar aurora!

It’s not a new concept, but there’s never been a clear understanding of where these geomagnetic storms originate. Do they come from a sudden disruption of electric current about 64 000 km from the planet? Or are the created by a process called magnetic reconnection which occurs much further down the magnetotail, at a distance of around 125 000 – 200 000 km? If you remember our recent study of Alfven waves, then you know current consensus points towards the reconnection theory. But there’s only one problem. Alfven waves are slow movers, traveling at a reconnection speed of about 250 seconds. What we’re seeing is an event that occurs about 60 seconds after reconnection… and the birth of a new movement. The kinetic Alfven wave (KAW).

“We ran a very simple system, and simulated how the reconnection event released energy in the plasma sheet of charged particles,” said Shay. “We were looking for a faster mechanism for propagating the signal from the explosion than the Alfven waves that were already widely recognized.”

Unlike its predecessor which motivates both ions and electrons, the KAW only excites the electron, moving them through the plasma at twice the speed. Through simulations, it’s been proved the kinetic Alfven wave could be spawned by reconnection, move away from the explosion and activate aurora. The data was returned by the Fluxgate Magnetometer (FGM) and the Electric Fields and Waves (EFW) instrument and found by Jonathan Eastwood, a Research Fellow at The Blackett Laboratory, Imperial College London.

“I found 18 events which occurred at the time the four spacecraft were flying through the tail region,” said Dr. Eastwood. “The fast signal predicted by Michael Shay showed up in the Cluster data, supporting the theory that kinetic Alfven waves generated by reconnection were rapidly energizing the auroras.”

“It’s rather like what happens in a thunderstorm,” he added. “The fast-moving lightning flash arrives first, followed some time later by the slower sound waves of the thunderclap.”

Fancy that… Coming from a substorm!

Original Story Source: ESA Science and Technology News. For Further Reading: Super-Alfvenic Propagation of Substorm Reconnection Signatures and Poynting Flux.

Posted on by Tammy Plotner

Mars Express Delivers Views Of Martian Lake

Holden crater is 140 km across, filling the left side of the image, while to the right is the remaining part of Eberswalde crater, with a diameter of about 65 km. They are located in the southern highlands of Mars. North is to the right of the image. The image was acquired by Mars Express at approximately 25°S / 326°E during orbit 7208 on 15 August 2009. The images have a ground resolution of about 22 m per pixel. Credits: ESA/DLR/FU Berlin (G. Neukum)

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In the southern highlands of Mars, Eberswalde crater to be exact, ESA’s Mars Express exploration has pinpointed an area which once held a lake. Although it may have been some 4 billion years ago, the geologic remains – called a delta – are still evident in the new images. This region of dark sediments are a shadowed reminder that Mars once had water.

Formed by an asteroid strike, Eberswalde crater has nearly eroded away with time. After it formed, it was partially obliterated by another impact which shaped 140 km diameter crater Holden. Although this second strike buried Eberswalde with ejecta, 115 square kilometers of delta area and feeder channels survived. These channels once were the arteries that pumped water along the surface to pool in the crater’s interior, forming a lake. As they carried water, they also carried sediments and – just as on Earth – left their mark. With time, the water dried up and even more sediments were carried along by the wind, exposing the area in vivid relief.

NASA’s Mars Global Surveyor spacecraft spied the delta in earlier missions, giving even further solidification that Mars was once a wet world. While Eberswalde crater and Holden crater were once a part of a list of possible landing sites for the Mars Science Laboratory, Gale crater was selected as the Curiosity’s landing site, given its high mineral and structural diversity related to water. But don’t count this wonderful, wet confession of a lake out forever. Thanks to high mineral diversity and suggestive structure, we’re sure to visit the delta of Eberswalde and Holden again, from orbit or with another landing mission.

Original Story Source: ESA News.

Posted on by Ray Sanders

First JWST Instrument Passes Tests

MIRI, ( Mid InfraRed Instrument ), during ambient temperature alignment testing in RAL Space's clean rooms. Image Credit: STFC/RAL Space

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One of many instruments that will fly aboard the James Webb Space Telescope (JWST) has just passed critical testing at ESA facilities in the UK. “MIRI”, the Mid-InfraRed Instrument, is being developed by the ESA as a vital part of the JWST mission. Researchers will use MIRI to study exoplanets, distant galaxies, comets and dust-shrouded star forming regions.  In order to work correctly and provide useful data, MIRI needs to consistently operate at temperatures of around 7 kelvin. (-266° C). How do engineers test these components to make sure they work properly in harsh conditions of space?

At the UK Science and Technology Facilities Council’s RAL Space in Oxfordshire, engineers performed tests to ensure the entire instrument assembly works as designed.  Inside the test chamber, special “targets” were used to help simulate scientific observations. The simulated observations will scientists develop the software necessary to calibrate MIRI after JWST’s launch. Based on the initial results of testing, the engineers believe MIRI is working properly and will perform all required science functions extremely well.

Peter Jakobsen, ESA JWST Project Scientist, said,  “Future users of JWST and MIRI are looking forward to learning more about the detailed performance of the instrument once the test results are analysed further in the coming months. The experience gained by the MIRI test team throughout this campaign has sown the seeds for a rich scientific harvest from the JWST mission.”

In the same ESA press release,  Gillian Wright, Principal Investigator and lead of the MIRI European Science Team added, “It is inspiring to see MIRI working extremely well at its operating temperature after so many years in development. The test campaign has been a resounding success and the whole MIRI team can be very proud of this magnificent achievement.”

Sean Keen making adjustments to MIRI during environmental testing in RAL Space's thermal vacuum chamber on August 16th. 2011.

This past July, the U.S House of Representatives’ appropriations committee on Commerce, Justice, and Science proposed a budget for fiscal year 2012 that would cancel JWST’s funding. In a testament to the dedication of the teams involved in JWST’s construction, work continues despite the uncertain fate of the JWST mission.

Aside from the MIRI instrument passing testing, over half of JWST’s mirrors have been polished and coated. Several of the mirror segments have passed rigorous testing, and at this time, nearly three-quarters of JWST’s hardware is being built or tested.

A screenshot of a JWST mirror segment in the laser testing facility at Ball Aerospace in Boulder, Colorado. Credit: John O'Connor, NASA Tech.

Above is a screenshot of a larger panoramic image from the NASA Tech website, showing one of the JWST mirror segments being tested in a laser testing facility at Ball Aerospace in Boulder, Colorado. You can see several panoramic views of the mirror testing at NASA Tech. These are big files, but are well worth the view! Just go to the main page and scroll down for the JWST panoramas.

If you’d like to learn more about the James Webb Space Telescope, visit: http://www.jwst.nasa.gov or: http://webbtelescope.org/webb_telescope

Resources on how you can contact your representative to express support for JWST can be found at: http://savethistelescope.blogspot.com.

You can also read a statement by the American Astronomical Society regarding JWST at: http://aas.org/node/4483 Source: ESA News Release