esa Archives

January 30, 2013December 23, 2015 by Jason Major

Lighting Up Andromeda’s Coldest Rings

Cold rings of dust are illuminated in this image taken by Herschel’s Spectral and Photometric Imaging Receiver (SPIRE) instrument. Credit: ESA/NASA/JPL-Caltech/B. Schulz (NHSC)

Looking wispy and delicate from 2.5 million light-years away, cold rings of dust are seen swirling around the Andromeda galaxy in this new image from the Herschel Space Observatory, giving us yet another fascinating view of our galaxy’s largest neighbor.

The colors in the image correspond to increasingly warmer temperatures and concentrations of dust — blue rings are warmer, while pinks and reds are colder lanes of dust only slightly above absolute zero. Dark at shorter wavelengths, these dust rings are revealed by Herschel’s amazing sensitivity to the coldest regions of the Universe.

The image above shows data only from Herschel’s SPIRE (Spectral and Photometric Imaging Receiver) instrument; below is a mosaic made from SPIRE as well as the Photodetecting Array Camera and Spectrometer (PACS) instrument:

“Cool Andromeda” Credit: ESA/Herschel/PACS & SPIRE Consortium, O. Krause, HSC, H. Linz

Estimated to be 200,000 light-years across — almost double the width of the Milky Way — Andromeda (M31) is home to nearly a trillion stars, compared to the 200–400 billion that are in our galaxy. And within these cold, dark rings of dust even more stars are being born… Andromeda’s star-making days are far from over.

Herschel’s mission will soon be coming to an end as the telescope runs out of the liquid helium coolant required to keep its temperatures low enough to detect such distant heat signatures. This is expected to occur sometime in February or March.

Herschel is a European Space Agency cornerstone mission with science instruments provided by consortia of European institutes, and with important participation by NASA. Launched May 14, 2009, the telescope orbits the second Lagrange point of the Earth-Sun system (L2), located 1.5 million km (932,000 miles) from Earth. Read more from the Herschel mission here.

January 21, 2013December 23, 2015 by Jason Major

Take a Rollercoaster Ride Around Venus

If you’ve ever wanted to see what it’s like to buzz Venus like only a spacecraft can, here’s your chance: this is a video animation of images taken by ESA’s Venus Express as it makes a pole-to-pole orbit of our neighboring world.

Captured in ultraviolet wavelengths, the images were acquired by the spacecraft’s Venus Monitoring Camera last January over a period of 18 hours. It’s truly a “day in the life” of Venus Express!

From ESA’s description of the video:

We join the spacecraft from a staggering 66,000 km above the south pole, staring down into the swirling south polar vortex. From this bird’s-eye view, half of the planet is in darkness, the ‘terminator’ marking the dividing line between the day and night sides of the planet.

Intricate features on smaller and smaller scales are revealed as Venus Express dives to just 250 km above the north pole and clouds flood the field of view, before regaining a global perspective as it climbs away from the north pole.

The observed pattern of bright and dark markings is caused by variations in an unknown absorbing chemical at the Venus cloud tops.

False-color image of cloud features on Venus. Captured by Venus Express from a distance of 30,000 km (18,640 miles) on December 8, 2011. (ESA/MPS/DLR/IDA)

Source: European Space Agency

January 18, 2013December 23, 2015 by Nancy Atkinson

Gorgeous Images: Ancient River on Mars?

Perspective view of Reull Vallis. ESA’s Mars Express imaged the striking upper part of the Reull Vallis region of Mars with its high-resolution stereo camera last year. Reull Vallis, the river-like structure in these images, is believed to have formed when running water flowed in the distant martian past, cutting a steep-sided channel through the Promethei Terra Highlands before running on towards the floor of the vast Hellas basin. Credit and Copyright: ESA/DLR/FU Berlin (G. Neukum)

The Mars Express has long been taking pictures of what appears to be an ancient riverbed on Mars. In fact, Reull Vallis was one of the first objects on the Red Planet that Mars Express ever imaged back in 2004 when the spacecraft arrived in orbit. The latest images show the sinuous river-like feature that stretches for nearly 1,500 km across the Martian landscape. This winding depression is 6-10 km wide, and its depth varies from 100-600 meters. In comparison, the Amazon River on Earth is about 6,500 km long and 11 km wide in places.

So, is this really an ancient river?

High-Resolution Stereo Camera image of Reul Vallis taken on May 14, 2012 by ESA’s Mars Express. Credit: ESA/DLR/FU Berlin (G. Neukum)

Planetary scientists seem to be fairly unanimous that, from orbit, this appears to be a riverbed. There is a system of tributaries and side channels that all appear to flow into the huge Hellas Basin.

There are various theories as to how it may have formed, however. Some scientists say that this feature may have been created quickly in a sudden deluge or runoff event, as the entire system look like stream beds cut by sudden runoff in desert regions on the Earth.

Reull Vallis in context. Credit: NASA MGS MOLA Science Team.

Others suggest this system consists of parts that were formed during several phases rather than being a single continuous channel, and likely had independent formation phases and different sources of water. For example, numerous crescent-shaped features could be older craters distorted by water flow.

There is also evidence of deposits of volatiles in the walls of the channel that could be ice.

In the wider context image above, the tributary intersecting the main channel appears to be part of a forking of the main valley into two distinct branches further upstream before merging back into a single main valley.

The right (northern) part of the main image is dominated by the Promethei Terra Highlands with their high and soft-rounded mountains shown in these images, rising around 2500 m above the surrounding flat plains.

The perspective view below shows one of these mountains with nearby sediment-filled impact craters:

This computer-generated perspective view shows part of the Promethei Terra highlands adjacent to Reull Vallis. Credit: ESA/DLR/FU Berlin (G. Neukum)

What about lava flow? Could this be a giant lava flow or tube that has collapsed? Astronomers say that lava and glacial erosion would have produced very different channels.

And so it appears Reull Vallis provides evidence of past water on Mars. And if so, it means that the planet’s climate has changed dramatically since these features were formed between 3.5 billion and 1.8 billion years ago.

One of the first images taken by Mars Express in 2004 of Reull Vallis. Credit: Credit: ESA/DLR/FU Berlin (G. Neukum)

Sources: ESA Science paper from 1997 by Scott Mest and David Crown, University of Pittsburgh, Paper by Kostama, et al, 2007, ESA 2004.

January 17, 2013January 4, 2016 by John Williams

Region in LMC Ablaze with Light and Color

Nearly 200 000 light-years from Earth, the Large Magellanic Cloud, a satellite galaxy of the Milky Way, floats in space, in a long and slow dance around our galaxy. As the Milky Way’s gravity gently tugs on its neighbour’s gas clouds, they collapse to form new stars. In turn, these light up the gas clouds in a kaleidoscope of colours, visible in this image from the NASA/ESA Hubble Space Telescope.

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”

January 17, 2013December 23, 2015 by Ken Kremer

New Look and New Animation for Orion’s 2017 Flight to the Moon and Back

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.

Ken Kremer

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

December 23, 2012December 23, 2015 by Ken Kremer

Orion assemblage on track for 2014 Launch

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 !

Ken Kremer

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

December 20, 2012December 23, 2015 by Jason Major

The Most Remote Workplace on Earth

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)

“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.

December 18, 2012December 23, 2015 by Nancy Atkinson

The Year in Space, From NASA and ESA

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.

December 6, 2012December 23, 2015 by John Williams

Pink Galactic Smackdown Results in Cosmic Bulls-eye

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

December 3, 2012December 23, 2015 by Jason Major

Are Venus’ Volcanoes Still Active?

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.