Space and astronomy news
Hubble view of star formation region N11 from the NASA/ESA Hubble Space Telescope. Image credit: NASA/ESA Hubble. Zoom by John Williams/TerraZoom using Zoomify.
New computer wallpaper alert. Light from the Large Magellanic Cloud takes nearly 200,000 years to travel to Earth. And it’s worth the wait.
Behold LHA 120-N 11, or just simply N11, in this image from the NASA/ESA Hubble Space Telescope.
Continue reading “Region in LMC Ablaze with Light and Color”
The Orion spacecraft has gotten a new look for its first launch atop the inaugural flight of NASA’s Space Launch System (SLS) booster on the Exploration Mission-1 flight around the Moon in 2017 as seen in this new animation.
The vehicles service module will be built by the European Space Agency (ESA), as a result of a new bilateral agreement between NASA and ESA. Orion is designed to carry humans back to the Moon and to deep space destinations like Asteroids and Mars.
The service module will fuel and propel the capsule on its uncrewed journey to the Moon and back on EM-1 in 2017.
Read my follow-up report for details about the new NASA/ESA agreement. See my earlier story here, about preparations for the first Orion launch in September 2014 on the upcoming Exploration Flight Test-1 in 2014 atop a Delta IV Heavy. An unmanned Orion will fly on a two orbit test flight to an altitude of 3,600 miles above Earth’s surface, farther than a human spacecraft has gone in 40 years, and then plunge back to Earth to test the spacecrafts systems and heat shield.
NASA is also simultaneously fostering the development of commercial ‘space taxis’ to fly astronauts to the International Space Station (ISS) as part of a dual track approach to restore America’s human space launch capability. The 1st commercial crew vehicle might fly as early as 2015 – details here.
Image caption: Orion EFT-1 crew cabin construction ongoing at the Kennedy Space Center which is due to blastoff in September 2014 atop a Delta 4 Heavy rocket. Credit: Ken Kremer
Image caption: Orion EFT-1 crew cabin construction ongoing inside the Structural Assembly Jig at the Operations and Checkout Building (O & C) at the Kennedy Space Center (KSC). This is the inaugural space-bound Orion vehicle due to blastoff from Florida in September 2014 atop a Delta 4 Heavy rocket. Credit: Ken Kremer
NASA is thrusting forward and making steady progress toward launch of the first space-bound Orion crew capsule -designed to carry astronauts to deep space. The agency aims for a Florida blastoff of the uncrewed Exploration Flight Test-1 mission (EFT-1) in September 2014 – some 20 months from now – NASA officials told Universe Today.
I recently toured the Orion spacecraft up close during an exclusive follow-up visit to check the work in progress inside the cavernous manufacturing assembly facility in the Operations and Checkout Building (O & C) at the Kennedy Space Center (KSC). Vehicle assemblage is run under the auspices of prime contractor Lockheed Martin Space Systems Corporation.
A lot of hardware built by contractors and subcontractors from all across the U.S. is now arriving at KSC and being integrated with the EFT-1 crew module (CM), said Jules Schneider, Orion Project manager for Lockheed Martin at KSC, during an interview with Universe Today beside the spacecraft at KSC.
“Everyone is very excited to be working on the Orion. We have a lot of work to do. It’s a marathon not a sprint to build and test the vehicle,” Schneider explained to me.
My last inspection of the Orion was at the official KSC unveiling ceremony on 2 July 2012 (see story here). The welded, bare bones olive green colored Orion shell had just arrived at KSC from NASA’s Michoud facility in New Orleans. Since then, Lockheed and United Space Alliance (USA) technicians have made significant progress outfitting the craft.
Workers were busily installing avionics, wiring, instrumentation and electrical components as the crew module was clamped in place inside the Structural Assembly Jig during my follow-up tour. The Jig has multiple degrees of freedom to move the capsule and ease assembly work.
“Since July and to the end of 2012 our primary focus is finishing the structural assembly of the crew module,” said Schneider.
“Simultaneously the service module structural assembly is also ongoing. That includes all the mechanical assembly inside and out on the primary structure and all the secondary structure including the bracketry. We are putting in the windows and gussets, installing the forward bay structure leading to the crew tunnel, and the aft end CM to SM mechanism components. We are also installing secondary structures like mounting brackets for subsystem components like avionics boxes and thruster pods as parts roll in here.”
Image caption: Window and bracket installation on the Orion EFT-1 crew module at KSC. Credit: Ken Kremer
“A major part of what we are doing right now is we are installing a lot of harnessing and test instrumentation including alot of strain gauges, accelerometers, thermocouples and other gauges to give us data, since that’s what this flight is all about – this is a test article for a test flight.
“There is a huge amount of electrical harnesses that have to be hooked up and installed and soldered to the different instruments. There is a lot of unique wiring for ground testing, flight testing and the harnesses that will be installed later along with the plumbing. We are still in a very early stage of assembly and it involves alot of very fine work,” Schneider elaborated. Ground test instrumentation and strain gauges are installed internally and externally to measure stress on the capsule.
Construction of the Orion service module is also moving along well inside the SM Assembly Jig at an adjacent work station. The SM engines will be mass simulators, not functional for the test flight.
Image caption: Orion EFT-1 crew cabin and full scale mural showing Orion Crew Module atop Servivce Module inside the O & C Building at the Kennedy Space Center, Florida. Credit: Ken Kremer
The European Space Agency (ESA) has been assigned the task of building the fully functional SM to be launched in 2017 on NASA’s new SLS rocket on a test flight to the moon and back.
Although Orion’s construction is proceeding apace, there was a significant issue during recent proof pressure testing at the O & C when the vehicle sustained three cracks in the aft bulkhead of the lower half of the Orion pressure vessel.
“The cracks did not penetrate the pressure vessel skin, and the structure was holding pressure after the anomaly occurred,” Brandi Dean, a NASA Public Affairs Officer told me. “The failure occurred at 21.6 psi. Full proof is 23.7 psi.”
“A team composed of Lockheed Martin and NASA engineers have removed the components that sustained the cracks and are developing options for repair work. Portions of the cracked surface were removed and evaluated, letting the team eliminate problems such as material contamination, manufacturing issues and preexisting defects from the fault tree. The cracks are in three adjacent, radial ribs of this integrally machined, aluminum bulkhead,” Dean stated.
Image caption: NASA graphic of 3 cracks discovered during recent proof pressure testing. Credit: NASA
The repairs will be subjected to rigorous testing to confirm their efficacy as part of the previously scheduled EFT-1 test regimen.
A great deal of work is planned over the next few months including a parachute drop test just completed this week and more parachute tests in February 2013. The heat shield skin and its skeleton are being manufactured at a Lockheed facility in Denver, Colorado and shipped to KSC. They are due to be attached in January 2013 using a specialized tool.
“In March 2013, we’ll power up the crew module at Kennedy for the first time,” said Dean.
Orion will soar to space atop a mammoth Delta IV Heavy booster rocket from Launch Complex 37 at Cape Canaveral Air Force Station in Florida. Construction and assembly of the triple barreled Delta IV Heavy is the pacing item upon which the launch date hinges, NASA officials informed me.
Following the forced retirement of NASA’s space shuttles, the United Launch Alliance Delta IV Heavy is now the most powerful booster in the US arsenal and heretofore has been used to launch classified military satellites. Other than a specialized payload fairing built for Orion, the rocket will be virtually identical to the one that boosted a super secret U.S. National Reconnaissance Office (NRO) spy satellite to orbit on June 29, 2012 (see my launch story here).
Orion will fly in an unmanned configuration during the EFT-1 test flight and orbit the Earth two times – reaching an altitude of 3,600 miles which is 15 times farther than the International Space Station’s orbital position. The primary objective is to test the performance of Orion’s heat shield at the high speeds and searing temperatures generated during a return from deep space like those last experienced in the 1970’s by the Apollo moon landing astronauts.
The EFT-1 flight is not the end of the road for this Orion capsule.
“Following the EFT-1 flight, the Orion capsule will be refurbished and reflown for the high altitude abort test, according to the current plan which could change depending on many factors including the budget,” explained Schneider.
“NASA will keep trying to do ‘cool’ stuff”, Bill Gerstenmaier, the NASA Associate Administrator for Human Space Flight, told me.
Stay tuned – Everything regarding human and robotic spaceflight depends on NASA’s precarious budget outlook !
Image caption: Orion EFT-1 crew cabin assemblage inside the Structural Assembly Jig at the Operations and Checkout Building (O & C) at the Kennedy Space Center (KSC); Jules Schneider, Orion Project Manager for Lockheed Martin and Ken Kremer. Credit: Ken Kremer
ESA’s Proba-1 satellite imaged the French-Italian Concordia base on November 21, 2012 (ESA)
Located in one of the loneliest locations on Earth, the French-Italian Concordia station was captured on high-resolution camera by ESA’s Proba-1 microsatellite last month, showing the snow-covered base and 25 square kilometers of the virtually featureless expanse of Antarctic ice surrounding it.
A cluster of scientific research buildings situated 3233 meters above sea level in the Antarctic interior, Concordia is one of the only permanently-crewed stations on the southern continent. Around 12–15 researchers and engineers spend months — sometimes over a year — in isolation at Concordia, where during the winter months there are no deliveries, no chance of evacuation, temperatures below -80 ºC (-112 ºF) and the next closest station is 600 km (370 miles) away. It’s like working on another planet.
And that’s precisely why they’re there.
The researchers who live and work at Concordia are there because of the station’s incredible remoteness and harsh conditions. This allows them to study not only the pristine Antarctic ice beneath their feet but also how humans behave in such an environment, where a small team must learn to work together and merely venturing outside can be a hazardous task.
It’s the next closest thing to an actual outpost on Mars, or the Moon. Even the astronauts on the ISS aren’t as far removed from the rest of the world.
(Although the night sky views from Concordia can be comparably stunning.)
Concordia Base boasts some of the clearest, darkest — and coldest — skies on Earth (ESA/IPEV/PNRA – A. Salam)
Read more: Milky Way to Concordia Base… Come In, Concordia Base…
“Boredom and monotony are the enemy,” wrote ESA-sponsored medical researcher Dr. Alex Salam, regarding his 2009 13-month stay. “The darkness has a habit of sucking the motivation out of even the hardiest. But despite the effects the darkness can have on sleep, mood and cognitive performance, there is something inherently special about the Antarctic night. The heavens present a view that many stargazers can only ever dream of. You just have to try and catch a glimpse of the stars before your eyelashes freeze together!
“Seeing the station from a distance with the Milky Way towering far above it never failed to make me feel both awe inspired and simultaneously insignificant.”
And another recent long-term resident of Concordia, Dr. Alexander Kumar, who departed the base on November 15, shared this reflection as his year-long term was approaching its end:
“Concordia has, in removing me from civilisation where sometimes it is harder to step back, enabled me to see the bigger picture, provide a unique experience and reminded me of somethings, setting a course and direction for the future… I think once you come to Antarctica, drawn to it under a spell like a seaman to a mermaid, you never can break the link you form with this raw, rugged and ruthlessly beautiful and enticing continent.”
The Sun returns to the Antarctic plateau (ESA/IPEV/PNRA – A. Salam)
“It’s the closest thing I’ll ever have to living on another planet.”
– Dr. Alex Salam
Read more about Concordia on the newly-redesigned ESA site here.
In orbit for over 11 years, Proba-1’s unique images are used by hundreds of scientific teams worldwide. To date its main Compact High Resolution Imaging Spectrometer (CHRIS) has acquired over 20,000 environmental science images used by a total of 446 research groups in 60 countries.
Both NASA and ESA have released videos looking back at the year 2012 in space. With Curiosity on Mars, the Flight of the Dragon, Venus Transit, ATV’s trips to the ISS, the flight of Vega, and much more, it was quite a year.
Bright pink nebulae encircle spiral galaxy NGC 922 in this image from the NASA/ESA Hubble Space Telescope. Credit: NASA/ESA. Zoom: John Williams/TerraZoom and Zoomify
Galaxies pack a wallop. A galactic bulls-eye ringed with pink nebulae is the only evidence of a rare galactic collision of NGC 922 that occurred millions of years ago. Clicking the button on the far right of the toolbar will allow awesomecosmicsauce to tantalize your eyes and work all of the pixels on your computer screen. Pressing the “ESC” will return you to the present universe.
Explore this awesome image from the NASA/ESA Hubble Space Telescope. While lovely, something is amiss in this image. NGC 922 used to be a spiral galaxy. As you zoom across the image, the spiral arms look distorted and disrupted. Hints of a galactic interaction are strewn across the galaxy from the large numbers of bright pink nebulae and blue stars to the spray of dim stars toward the top of the image. Ripples set up as the smaller galaxy passed through the gas and dust clouds of NGC 922 created new star formation. Ultraviolet radiation from these bright new stars cause hydrogen gas in the surrounding nebula to glow a characteristic pink. The tugs of gravity hurled thousands of stars outward.
Episode 60 of the Hubblecast explores NGC 922, a galaxy that has been hit square-on by another. Ripples of star-formation are still propagating out across thousands of light-years of space over 300 million years after the collision, making it a prime example of what astronomers call a collisional ring galaxy.
Scientists believe that millions of years ago a small galaxy, known as 2MASXI J0224301-244443, plunged through the heart of NGC 922. Sometimes, if a small galaxy hits a larger galaxy just right, a circle is formed. But more often than not, galaxies are not aligned perfectly. When a galaxy smacks another off center, one side of the ring is brighter than the other. NGC 922 is a prime example of what astronomers call collisional ring galaxies. Although only a few ring galaxies are seen in our cosmic neighborhood, of which the Cartwheel Galaxy is the most spectacular, ring galaxies appear to be commonplace as we peer further into the past.
As you explore the empty places of the image, look for faraway background galaxies. Several dim spiral galaxies dot the image both outside the galaxy and within the star-speckled interior.
NGC 922 is found about 330 million light-years from Earth toward the constellation Fornax. Sky mapper and French astronomer Nicolas Louis de Lacaille introduced Fornax, the Furnace, in 1756. Fornax is relatively devoid of stars allowing astronomers to peer deep into the universe. The constellation was the perfect target for the Hubble Ultra Deep Field image.
NASA/ESA Hubble Space Telescope image of NGC 922. Credit: NASA, ESA
Source: ESA Hubble
Artist’s impression of an active volcano on Venus (ESA/AOES)
Incredibly dense, visually opaque and loaded with caustic sulfuric acid, Venus’ atmosphere oppresses a scorched, rocky surface baking in planet-wide 425 ºC (800 ºF) temperatures. Although volcanoes have been mapped on our neighboring planet’s surface, some scientists believe the majority of them have remained inactive — at least since the last few hundreds of thousands of years. Now, thanks to NASA’s Pioneer Venus and ESA’s Venus Express orbiters, scientists have nearly 40 years of data on Venus’ atmosphere — and therein lies evidence of much more recent large-scale volcanic activity.
The last six years of observations by Venus Express have shown a marked rise and fall of the levels of sulfur dioxide (SO2) in Venus’ atmosphere, similar to what was seen by NASA’s Pioneer Venus mission from 1978 to 1992.
These spikes in SO2 concentrations could be the result of volcanoes on the planet’s surface, proving that the planet is indeed volcanically active — but then again, they could also be due to variations in Venus’ complex circulation patterns which are governed by its rapid “super-rotating” atmosphere.
“If you see a sulphur dioxide increase in the upper atmosphere, you know that something has brought it up recently, because individual molecules are destroyed there by sunlight after just a couple of days,” said Dr. Emmanuel Marcq of Laboratoire Atmosphères in France, lead author of the paper, “Evidence for Secular Variations of SO2 above Venus’ Clouds Top,” published in the Dec. 2 edition of Nature Geoscience.
“A volcanic eruption could act like a piston to blast sulphur dioxide up to these levels, but peculiarities in the circulation of the planet that we don’t yet fully understand could also mix the gas to reproduce the same result,” added co-author Dr Jean-Loup Bertaux, Principal Investigator for the instrument on Venus Express.
The rise and fall of sulphur dioxide in the upper atmosphere of Venus over the last 40 years, expressed in units of parts per billion by volume. Credits: Data: E. Marcq et al. (Venus Express); L. Esposito et al. (earlier data); background image: ESA/AOES
Because Venus’ dense atmosphere whips around the planet at speeds of 355 km/hour (220 mph), pinpointing an exact source for the SO2 emissions is extremely difficult. Volcanoes could be the culprit, but the SO2 could also be getting churned up from lower layers by variations in long-term circulation patterns.
Read: Venus Has a Surprisingly Chilly Layer
Venus has over a million times the concentration of sulfur dioxide than Earth, where nearly all SO2 is the result of volcanic activity. But on Venus it’s been able to build up, kept stable at lower altitudes where it’s well shielded from solar radiation.
Regardless of its source any SO2 detected in Venus’ upper atmosphere must be freshly delivered, as sunlight quickly breaks it apart. The puzzle now is to discover if it’s coming from currently-active volcanoes… or something else entirely.
“By following clues left by trace gases in the atmosphere, we are uncovering the way Venus works, which could point us to the smoking gun of active volcanism,” said Håkan Svedhem, ESA’s Project Scientist for Venus Express.
Read more on the ESA release here.
This weekend the International Space Station will turn itself to face the Sun, enabling ESA’s SOLAR instrument to capture an entire rotation of the solar surface. This is the first time the Station has changed attitude for scientific reasons alone.
This instrument has been on the ISS since 2008, and for the first time will record a full rotation of the Sun. It began this effort on November 19, 2012, and on December 1, the Station will spend two hours turning about 7 degrees so that observations can continue. It will hold this angle for ten days before returning to its original attitude.
“We want to record a complete rotation of the Sun and that takes around 25 days,” said Nadia This, operations engineer at the Belgian User Support and Operations Centre that controls SOLAR.
SOLAR needs to be in direct view of the Sun to take measurements but the Space Station’s normal orbit obscures the view for two weeks every month.
All the international partners had to agree on changing the ISS’s orientation.
However, moving a 450-ton orbital outpost the size of a city block isn’t a simple undertaking. Aside from calculating the correct orbit to keep SOLAR in view of the Sun, other factors need to be taken into account such as ensuring the solar panels that power the Station also face the Sun. Additionally, communication antennas need to be reoriented to stay in contact with Earth and other scientific experiments must be adjusted.
The SOLAR instrument located on the exterior of the Columbus module on the ISS. Credit: ESA
The SOLAR instrument was originally designed to last about 18 months, but has been going strong for 5 years. It is installed on the outside of the ESA’s Columbus module.
The SOLAR payload consists of three instruments to the solar spectral irradiance throughout virtually the whole electromagnetic spectrum.
The three complementary solar science instruments are:
SOVIM (SOlar Variable and Irradiance Monitor), which covers near-UV, visible and thermal regions of the spectrum.
SOLSPEC (SOLar SPECctral Irradiance measurements) covers the 180 nm – 3 000 nm range.
SOL-ACES (SOLar Auto-Calibrating Extreme UV/UV Spectrophotometers) measures the EUV/UV spectral regime.
Scientists say SOLAR’s observations are improving our understanding of the Sun and allowing scientists to create accurate computer models and predict its behavior.
Source: ESA
Artist concept of an ExoMars rover. Credit: ESA
After NASA was forced to back out of the joint ExoMars mission with the European Space Agency due to budget constraints, it looked like the exciting rover-orbiter mission might not happen. However, ESA went elsewhere looking for help, and has now announced a tentative cooperative arrangement with Russia’s space agency where Roscosmos will provide the two launch vehicles for multi-vehicle European-Russian ExoMars missions in 2016 and 2018.
Plans are for the mission to have an orbiter for launch in 2016, plus an ESA-built rover mission in 2018. Roscosmos will provide Proton rockets for the launches of the two missions, as well as providing an instrument for both the orbiter and the rover as well as overseeing the landing of the rover. The orbiter would study Mars’ atmosphere and surface and the six-wheeled vehicle would look for signs of past or present life.
The orbiter would also provide telecommunications for the rover.
Frederic Nordland, ESA’s director of international relations, said the agreement would be finalized before the end of the year and that its principal characteristics are already known and accepted by both sides. The announcement was made at a meeting in Naples, Italy this week of ESA’s space leaders from the 10 different nations that comprise the organization. The leaders are discussing future objectives and priorities for Europe in space, with the aim of shaping the development of Europe’s space capability.
During the meeting, Poland officially joined ESA, becoming the 20th member of the European space organization. It joins the other member states of Austria, Belgium, Britain, the Czech Republic, Denmark, Finland, France, Germany, Greece, Ireland, Italy, Luxembourg, The Netherlands, Norway, Portugal, Romania, Spain, Sweden and Switzerland.
ExoMars is now expected to cost ESA about 1.2 billion euros. So far, 850 million euros has been committed by the participating members, but officials remain confident the remaining funds can be raised.
ESA officials also said Russia’s Proton rocket might be used to launch Europe’s Juice mission to Jupiter in 2022, saving ESA’s science program some 170 million euros.
Sources: BBC, Space News
Caption: GOCE over ice. Credits: ESA – AOES Medialab
Since March 2009, the European Space Agency (ESA) mission, Gravity field and steady-state Ocean Circulation Explorer (GOCE) has been orbiting Earth. It carries highly sensitive instrumentation able to detect tiny variations in the pull of gravity across the surface of the planet, allowing it to map our planet’s gravity with unrivaled precision, producing the most accurate gravity map of Earth. With the planned mission completed, the fuel consumption has been much lower than anticipated, enabling ESA to extend GOCE’s life and put it into an even lower orbit, improving the quality of the gravity model.
The GOCE spacecraft was designed to fly low and has spent most of its mission roughly 500km below most other Earth-observing missions, at an altitude of 255km. ESA’s Earth Scientific Advisory Committee recommended lowering the orbit by 20km at a rate of about 300m per day, starting in August. After coming down by 8.6 km, the satellite’s performance and orbit were assessed. Now, GOCE is again being lowered while continuing its gravity mapping. It is expected to reach 235 km by February.
Decreasing the altitude increases the spatial resolution and the precision of the data. The expected increase in data quality is so high (possibly 35%) that scientists are calling it GOCE’s ‘second mission. Volker Liebig, ESA’s Director of Earth Observation Programmes has said “What the team of ESA engineers is now doing has not been done before and it poses a challenge. But it will also trigger new research in the field of gravity based on the high-resolution data we are expecting.”
Caption: The image on the left shows GOCE’s gravity measurements over northern Europe, acquired from its previous altitude. The image on the right depicts the expected measurements over the same area after the satellite has been lowered. Credits: ESA / GOCE+ Theme 2
The first ‘geoid’ based on GOCE’s gravity measurements was unveiled in June 2010. It is a crucial reference for conducting precise measurements of ocean circulation, sea-level change and ice dynamics. The mission has also been studying air density and wind in space, and its data was recently used to produce the first global high-resolution map of the boundary between Earth’s crust and mantle, called the Mohorovicic, or “Moho” discontinuity.
As the orbit drops, atmospheric drag increasingly pulls the satellite towards Earth, so GOCE has to use the tiny thrust of its ion engine to continuously compensate for any drag to stay aloft and maintain the stability it needs to measure Earth’s gravity. GOCE has enough xenon fuel for another 50 weeks of operations. When the fuel runs out the satellite will be pulled into the deep atmosphere where it will burn up
Find out more about the GOCE mission here