Russians Unveil Science Beauty in Florida

Russian built Mini Research Module MRM-1 set to launch aboard US Space Shuttle Atlantis in May 2010 undergoes final prelaunch processing in Florida. Credit: Ken Kremer

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Russian space managers unveiled a science beauty today (March 25) in Florida, namely the ‘Rassvet’ research room which serves as Russia’s newest contribution to the International Space Station. Although ‘Rassvet’ was built entirely in Russia, the module is hitching a ride aboard the American Space Shuttle Atlantis as the primary cargo for the STS 132 station assembly mission slated to blast off soon in May 2010. ‘Rassvet’ translates as ‘Dawn’.

I was quite fortunate to inspect ‘Rassvet’ up close today during a press briefing and photo op inside the clean room at the Astrotech Space Operations Facility in Port Canaveral, FL and also speak with the top Russian space officials from RSC Energia who are responsible for her construction. Astrotech is situated a few miles south of the shuttle launch pad at the Kennedy Space Center from which she’ll depart Earth.

NASA is launching ‘Rassvet’, formally known as the Mini Research Module-1, or MRM 1, as part of a complex barter agreement among the partner nations of the ISS to share the costs of assembling and operating the massive orbiting outpost.

MRM-1 will be attached to the Earth- facing (nadir) port of the russian Zarya control module at the ISS. See diagram below showing location of MRM-1 and other components on the Russian Orbital Segment of the ISS.

Side view of Russian built Mini Research Module MRM-1 set to launch aboard Shuttle Atlantis during STS 132 flight in May 2010. Russian Soyuz and Progress capsules will berth at the docking port at right. Sensitive surfaces on the docking mechanism are currently protected by red covers which will be removed before flight to space. Credit: Ken Kremer

“MRM 1 arrived in Florida on Dec 17, 2009 from Russia and will be utilized for scientific research, cargo stowage, and also to provide an additional docking port at the ISS,” said Mikhail Kashitsyn, the Deputy Technical Manager and Head of MRM 1 Prelaunch Processing for the Design Bureau division of RSC Energia. RSC Energia is the prime contractor to Roscosmos, the Russian Federal Space Agency, and is responsible for the design, development and processing of MRM 1.

Russian MRM 1 managers: Mikhail Kashitsyn, Deputy Technical Manager Head of MRM 1 Prelaunch Processing and Sergey Saveliev, Deputy Project Manager for MRM1. from the Design Bureau division of RSC Energia at Astrotech for press briefing on March 25, 2010. Credit: Ken Kremer

The additional docking port provided by MRM -1 will greatly aid ISS mission planners in accommodating the busy manifest of berthings of incoming Soyuz, Progress and ATV vehicles on the Russian side of the station and alleviate the need to repark the ships as new vessels arrive.

“We have been working at a steady pace to complete the final check out and assembly of MRM 1for installation into the shuttle orbiter. Let me welcome you all here to view MRM 1 which was designed by RSC Energia, one of the leading corporations in Russia”.
“All preparations will be completed in about 1 week. It’s wonderful we have this cooperation with our American colleagues and I want to express my thanks to the US and NASA for their help and mutual understanding,” added Mr. Kashitsyn.

“MRM 1 will be the largest piece of Russian space hardware ever to launch on an American rocket,” Kashitsyn told me. “The last large piece of Russian space equipment to launch from the US was the Mir docking module for the Mir space station”.
“Several thousand people worked on MRM 1 in Russia and it took about 2 years to build. About 100 are involved in the pre launch preparations here at Port Canaveral”.

“Furthermore, the interior of the module will also be loaded with 1.5 tons of NASA cargo and supplies for the ISS, including items such as food, lithium hydroxide canisters, computers and printers”, according to Kashitsyn.

“This will be the last payload for Atlantis,” said Robert Ashley, the NASA ISS manager responsible for the STS 132 payload processing. “This will be my last mission as a station mission manager. It’s bittersweet. There will be a lot of lasts for a lot of people on these final shuttle missions”.

100 Russian scientists and engineers have spent several months working at Astrotech and have nearly completed preparing the Russian built Mini Research Module MRM-1 for launch aboard Atlantis to the ISS . Credit: Ken Kremer

“MRM 1 will be shipped to the NASA Space Station Processing Facility at KSC on April 2. After about three days of final integration and pressurization tests, it will be loaded into a shipping container on April 5 for delivery to the shuttle launch pad,” Ashley said.

The MRM-1 payload comprises the module itself, an airlock chamber, an exterior portable work station and replacement elbow joints for the European Robotic Arm. The total mass exceeds 17,000 pounds.

Integrated Cargo Carrier during prelaunch preparations at Astrotech facility in clean room adjacent to MRM 1. Credit Ken Kremer
Also tucked in Atlantis payload bay will be the 8000 lb Integrated Logistics Carrier (ICC) carrying spare parts and Orbital Replacement Units (ORU’s) including six spare batteries, a boom assembly for the Ku-band antenna and spares for the Canadian Dextre robotic arm extension.

STS 132 is currently planned as the final flight of Atlantis. Unless the shuttle program is extended, Atlantis will be the first of NASA’s three shuttle orbiters to be retired from duty marking a significant milestone toward the end of the Space Shuttle Program. Many experts both in and out of NASA now say that the shuttles are being prematurely retired, mostly due to a lack of money.

Location of MRM-1 and other components on the Russian Orbital Segment of the ISS
Russia MRM 1 Research Module and Ken Kremer at Astrotech Space Operation Facility in Port Canaveral, Florida for press briefing

Earth Hour 2010

Where will you be when the lights go out? Earth Hour 2010 will take place on Saturday, March 27 at 8:30 pm local time. Even though it will spark a tirade of controversy just asking folks to turn off their lights for one hour, let’s see who would rather fight than turn off a switch. In 2009 hundreds of millions of people around the world showed their support and Earth Hour 2010 will continue to be a global call to action to every individual, every business and every community. A call to stand up, to show leadership and be responsible for our future. Do you have what it takes to make such a simple gesture?

Then let’s rock the house…

Earth Hour started in 2007 in Sydney, Australia when 2.2 million homes and businesses turned their lights off for one hour to make their stand against climate change. A year later Earth Hour had become such a global force that more than 50 million people in 35 countries showed their support by switch off for a simple 60 minutes. Icons stood in dark silence as Sydney Harbour Bridge, The CN Tower in Toronto, The Golden Gate Bridge in San Francisco, and Rome’s Colosseum, all did their part as symbols of hope for the future.

Can you still use your imagination? Can you? Then imagine Earth Hour from space…

This year China’s Forbidden City heads up a list of some of the world’s most iconic landmarks that have confirmed their participation in Earth Hour – including The Great Pyramids of Giza and the Sphinx. They will be joined by Italy’s Trevi Fountain in Rome and Leaning Tower of Pisa, Big Ben and Houses of Parliament in London, Edinburgh Castle in Scotland, India Gate and Red Fort in Delhi, Victoria Falls in Zimbabwe, Bosphorous Bridge in Istanbul, Hohensalzburg Castle in Salzburg, and Independence Angel in Mexico City. They join a comprehensive list of the world’s great man-made marvels and natural wonders, including the Eiffel Tower, Brandenburg Gate, Hiroshima Peace Memorial, Empire State Building, London Eye, Table Mountain, Christ the Redeemer statue, Sydney Opera House and the world’s tallest building, Burj Khalifa, which will plunge into darkness for Earth Hour

Before you say “Why bother?” or “My contribution won’t make a difference.”, then think on this… Earth Hour has truly managed to raise our awareness of climate change issues. But there’s more to it than switching off your lights for one hour once a year. It’s all about giving people a voice on the future of our planet and working together. Even if you’d rather fight than flick the switch… you are participating. Whether you are an individual, a business, a school or a city, you can show your support for Earth Hour by turning off your lights at 8.30 pm on March 27 wherever you are on the planet. No one is saying you can’t use your computer or watch television. Bake a pizza and eat it by candlelight with your family! All it takes is the guts to show you understand and care enough to take action.

Do you have what it takes to flip the switch?

Where In The Universe #97

Here’s this week’s image for the Where In The Universe Challenge, to test your visual knowledge of the cosmos You know what to do: take a look at this image and see if you can determine where in the universe this image is from; give yourself extra points if you can name the instrument responsible for the image. We’ll provide the image today, but won’t reveal the answer until later. This gives you a chance to mull over the image and provide your answer/guess in the comment section. Please, no links or extensive explanations of what you think this is — give everyone the chance to guess.

UPDATE: Answer has now been posted below.

This image shows a portion of the W5 star-forming region, located 6,500 light-years away in the constellation Cassiopeia. It is a composite of infrared data from Spitzer’s infrared array camera and multiband imaging photometer. It shows the nasty effects of living near a group of massive stars: radiation and winds from the massive stars (white spot in center) are blasting planet-making material away from stars like our sun. The planetary material can be seen as comet-like tails behind three stars near the center of the picture. The tails are pointing away from the massive stellar furnaces that are blowing them outward.

The image was taken in 2008, and is one of the best examples of multiple sun-like stars being stripped of their planet-making dust by massive stars.

Check back next week for another WITU challenge!

MRO Sees Opportunity on the Edge of Concepcion Crater (and more!)

Opportunity at the Edge of Concepción Crater (ESP_016644_1780) Opportunity at the Edge of Concepción Crater. Credit: NASA/JPL/University of Arizona

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It has been a while since I’ve posted a batch of new images from the Mars Reconnaissance Orbiter HiRISE camera, and what a treat when I saw what had just been released! This image shows the Mars Exploration Rover Opportunity perched on the edge of Concepción Crater in Meridiani Planum, Mars. This image was taken by HiRISE on February 13, 2010, on sol 2153 of Opportunity’s mission on Mars. If you look closely, you can see rover tracks in the ripples to the north and northwest of the rover! Wow! See below for a wonderful colorized close-up version by Stu Atkinson that shows the tracks very clearly. Scientists use these high-resolution images (about 25 cm/pixel) to help navigate the rover. In addition, rover exploration of areas covered by such high-resolution images provides “ground truth” for the orbital data. Oppy has moved along from Concepcion and is now heading towards a set of twin craters. You can check out Stu’s blog Road to Endeavour to see what Opportunity is seeing these days. One milestone (meterstone?) Oppy recently reached was hitting 20 km on her odometer and she seems to continue to be in great operating condition. Go Opportunity! Click here to be able to download larger versions of the image.

Tracks by the Opportunity rover, as seen by HiRISE, color version by Stu Atkinson. Credit: NASA/JPL/U of AZ

Signs of Aeolian and Periglacial Activity at Vastitas Borealis Credit: NASA/JPL/University of Arizona

This image is interesting because of all the interesting different aspects you can find if you look closely. The surface must be relatively young because there are no recent impact craters. There are numerous dust devil tracks crisscrossing across the image. Plus, there are polygon features in the soil – the same features seen around the Phoenix lander area which are produced by repeated expansion and contraction of the soil-ice mixture due to seasonal temperature changes. This is the Vastitas Borealis region on Mars’ northern plains.

Another interesting feature is the circle of boulders that appears on the right side. Is there an impact crater buried under shifting Martian sand? A visit by a rover or human could tell us for sure.

The image covers approximately 400 x 250 meters (350 x 225 yards).

Layers and Dark Debris in Melas Chasma (PSP_002419_1675) Layers and Dark Debris in Melas Chasma Credit: NASA/JPL/University of Arizona

This is an impressive looking region in Melas Chasma. Scientists say the layers are sedimentary in origin, but there are many processes that could have deposited them, such as volcanic airfall from explosive eruptions, or dust-size particles settling out of the atmosphere due to cyclic changes, and deposition in standing bodies of water.

See more great images at the HiRISE website.

Astronomers Find 90% More Universe!

The GOODS South Field. ESO/M. Hayes

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Astronomers have long known that many surveys of distant galaxies miss 90% of their targets, but they didn’t know why. Now, astronomers have determined that a large fraction of galaxies whose light took 10 billion years to reach us have gone undiscovered. This was found with an extremely deep survey using two of the four giant 8.2-meter telescopes that make up ESO’s Very Large Telescope (VLT) and a unique custom-built filter. The survey also helped uncover some of the faintest galaxies ever found at this early stage of the Universe.

Astronomers frequently use the strong, characteristic “fingerprint” of light emitted by hydrogen known as the Lyman-alpha line, to probe the amount of stars formed in the very distant Universe Yet there have long been suspicions that many distant galaxies go unnoticed in these surveys. A new VLT survey demonstrates for the first time that this is exactly what is happening. Most of the Lyman-alpha light is trapped within the galaxy that emits it, and 90% of galaxies do not show up in Lyman-alpha surveys.

“Astronomers always knew they were missing some fraction of the galaxies in Lyman-alpha surveys,” explains Matthew Hayes, the lead author of the paper, published this week in Nature, “but for the first time we now have a measurement. The number of missed galaxies is substantial.”

To figure out how much of the total luminosity was missed, Hayes and his team used the FORS camera at the VLT and a custom-built narrowband filter to measure this Lyman-alpha light, following the methodology of standard Lyman-alpha surveys. Then, using the new HAWK-I camera, attached to another VLT Unit Telescope, they surveyed the same area of space for light emitted at a different wavelength, also by glowing hydrogen, and known as the H-alpha line. They specifically looked at galaxies whose light has been traveling for 10 billion years (redshift 2.2), in a well-studied area of the sky, known as the GOODS-South field.

“This is the first time we have observed a patch of the sky so deeply in light coming from hydrogen at these two very specific wavelengths, and this proved crucial,” said team member Goran Ostlin. The survey was extremely deep, and uncovered some of the faintest galaxies known at this early epoch in the life of the Universe. The astronomers could thereby conclude that traditional surveys done using Lyman-alpha only see a tiny part of the total light that is produced, since most of the Lyman-alpha photons are destroyed by interaction with the interstellar clouds of gas and dust. This effect is dramatically more significant for Lyman-alpha than for H-alpha light. As a result, many galaxies, a proportion as high as 90%, go unseen by these surveys. “If there are ten galaxies seen, there could be a hundred there,” Hayes said.

Different observational methods, targeting the light emitted at different wavelengths, will always lead to a view of the Universe that is only partially complete. The results of this survey issue a stark warning for cosmologists, as the strong Lyman-alpha signature becomes increasingly relied upon in examining the very first galaxies to form in the history of the Universe. “Now that we know how much light we’ve been missing, we can start to create far more accurate representations of the cosmos, understanding better how quickly stars have formed at different times in the life of the Universe,” said co-author Miguel Mas-Hesse.

The breakthrough was made possible thanks to the unique camera used. HAWK-I, which saw first light in 2007, is a state-of-the-art instrument. “There are only a few other cameras with a wider field of view than HAWK-I, and they are on telescopes less than half the size of the VLT. So only VLT/HAWK-I, really, is capable of efficiently finding galaxies this faint at these distances,” said team member Daniel Schaerer.

Read the team’s paper.

Source: ESO

UK Launches New Space Agency

Britain has created a new national space agency, with plans to build a multimillion-dollar space innovation center. Until now UK space policy has been split between government departments. “The new agency will be a focal point in order to coordinate in a much more streamlined and efficient manner, working both on national projects and alongside ESA for the wider industry as well” said the UK’s first astronaut Major Tim Peake, who was selected in 2009 to represent England in space.

The U.K. Space Agency (UKSA) will begin operation – and have a new website available — by April 1, 2010.
“The action we’re taking today shows that we’re really serious about space,” said Lord Paul Drayson, U.K. Minister for Science and Innovation. “The U.K. Space Agency will give the sector the muscle it needs to fulfill its ambition.”

Drayson and Peake both said that the British space industry has remained strong despite recession troubles elsewhere and could grow into a $60 billion-a-year industry and create more than 100,000 jobs over the next 20 years.

“Our industry is really a hidden success story,” said Peake speaking on the BBC, “even during economic downturn, the space sector has been one of the few industry that has shown steady growth. We are in the forefront of the robotics technology and manufacturing small satellites and telecommunications as well.”

Peake said the UK space industry currently add $6.5 billion pounds to the economy and employs 68,000 people.

No new money will be added to the UK space budget, and the 200 million pounds allocated for UKSA is a consolidation of existing funding.

Peake said this doesn’t mean that the UK will leave the ESA alliance. “It is not a case of forging our way on our own. Every country that is in ESA also has their own agency and space policy. The ESA allows us to get involved in projects that no single country could afford to.”

In reading reactions from some of the UK bloggers, however, most convey skepticism about the new organization.

In New Scientist, Dr.Stu Clark wonders where the science is among the allocations for buildings and new technology. Plus he’s not sure if the plan for the UKSA is sustainable. “So it’s all very well having a 20-year plan, but the big question is whether UKSA can survive the next six months.”

At Astronomyblog, Stuart Lowe expressed disappointment. “For me, the launch has been a let down. We were led to believe that UKSA would be a NASA for the UK. The reality is far from it… I want to have an fantastic, inspiring, space agency. I want us to invest in it like we mean it. I want a NASA. I feel as though we’ve got a refurbished, second-hand agency that might collapse as soon as it leaves the launchpad and never make it past the General Election. Come on UK. You can do so much better.”

The e-Astronomer isn’t too fond of the UKSA logo: We got an exciting new logo. Actually I hated it. Looks like something somebody invented for a fictional fascist party in a cheap TV drama. Modern and thrusting and all that. But I guess its memorable.

Still others ask the big question: How is UKSA going to be pronounced? “Uk-sah” or “You-Kay-Ess-Ay?”

Sources: BBC, The Guardian, New Scientist, e-Astronomer, Parsec

ISS to get ‘Man Cave’ Complete with Robot Butler

Cosmonaut Yuri Gidzenko floats inside Leonardo during its first flight to the ISS. Leonardo will become a permanant module later in 2010. Credit: NASA

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There might be a new favorite hang-out for astronauts aboard the International Space Station later this year. The Multi Purpose Logistics Module (MPLM) known as Leonardo – which will be going to the ISS on the upcoming STS-131 mission carrying cargo and supplies — will be transformed after the mission into a Permanent Multipurpose Module (PMM), and brought up to stay on the station on STS-133 as a storeroom for supplies. But it might also become a haven to get away from it all.

“The thought is, the PMM might become sort of a ‘man cave’,” said Mike Kinslow, the Boeing payload manager out at Kennedy Space Center. “It won’t have all the background noise of fans, computers and other equipment running like in the laboratories, so it will be a quieter atmosphere that might appeal to the astronauts during their off-duty hours.”

No plans for a big screen TV Kinslow said, but there will be ports for computers, and since internet is now available on the ISS, Leonardo could be the location of choice to compose emails to loved ones back home, or do a little Twittering.

Another interesting piece of hardware scheduled to fly on the PMM is the Robonaut 2, NASA’s second generation of dexterous robots with a human-like torso that can work with tools and one day are envisioned to be able to do EVA work outside the ISS. But for now, R2 will be tested inside the station in zero-g. “It will be used on orbit for routine maintenance indoors only.” said Kinslow, “This is not an external unit.”

It has a “head” with a vision system, with hands that can do work, controlled by virtual-reality-like operation. Any chance R2 could be programmed to serve drinks or bring food into the man cave?

See our article on how General Motors is going to use R2 for manufacturing cars.

Turning Leonardo into a permanent module will take some work, said NASA Payload Manager Joe Delai. “Once it returns from this flight we will beef up the external shield and change things internally to become a permanent module. It will be about a four month process to get it ready.”

Leonard being attached to the ISS on a previous mission. Credit: NASA TV

The MPLMs were built in Italy, but are owned by the U.S. and provided in exchange for Italian access to U.S. research time on the Station. Four modules were built; three flew to the ISS. STS-131 will be Leonardo’s seventh trip to space.

Kinslow said shields for an MPLM are lighter weight because they are only meant to be on orbit for 2 weeks at a time. “Leonardo will be plated with a multilevel Kevlar blanket, the same type of exterior shielding other modules have, which is similar to armor plating, to protect against meteorite or debris impact. Internally, not a lot of changes will be made,” he said. “It already has a ventilation system like a normal module, but will need a computer system and a few other additions.”

Leonardo won’t be outfitted with a sleep station or crew quarters because it might be in a more vulnerable position for radiation or debris hits. “They don’t really want crew to get in and sleep because of the shielding,” Kinslow said. “It will be a storage module, and we’re discussing putting exercise equipment in there.”

The PMM will be berthed on the Node 1 nadir, or Earth-facing port. Leonardo measures about 6.5 meters (21 feet) long and 4.5 meters (15 feet) in diameter.

STS-131 is currently scheduled for an April 5 launch, and STS-133 is shooting for a September 2010 launch.

Just a note on the ISS internet: T.J. Creamer, who is on board the station now told Universe Today that they aren’t able to have streaming video or download large files. “In terms of download speeds – you know, back in the old days, it kind of compares to 9.6 and the 14.4 kilobyte modems, so it’s not really fast enough to do large file exchange or videos, but it certainly lets us to do browsing and the fun reading we want to do, or get caught up on current events on that day. It’s a nice outreach for us, and of course you’ve heard about the Twittering which is a nice feature that we can partake in also.”

SDO On Station Transmitting First Data as Solar Science Payloads Open Today

Blast off on Feb 11 of mighty Atlas V rocket and SDO from Pad 41 at Cape Canaveral as viewed from the KSC press site. Credit: Ken Kremer

Video Caption: EVE rediscovered the Van Allen Radiation Belt. These EVE data highlight where the energetic protons are in the inner Van Allen radiation belt. The red dots indicate the highest concentration of protons (lower altitude), and the blue-violet dots represents very little detection of particles (higher altitude of GEO). Visualization by Chris Jeppesen.

Following several precise propulsion burns to circularize its orbit, NASA’s Solar Dynamics Observatory (SDO) has arrived “On Station” and multiple tasks critical to check out of the science instruments are in progress this week, according to Dean Pesnell. Pesnell is the SDO project scientist from NASA’s Goddard Spaceflight Center which built the spacecraft and manages the nearly $1 Billion mission for NASA.

“We reached our final orbit on March 16, 2010”, Pesnell told me in an interview. “The SDO spacecraft is working great and all systems are behaving as expected”. SDO was launched on Feb. 11, 2010 from Cape Canaveral Air Force Station aboard an Atlas V rocket.

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The revolutionary science mission has been dubbed the “crown jewel” of NASA’s Solar Exploration research fleet, joining the twin STEREO spacecraft and SOHO. SDO is equipped with three science instruments (HMI, AIA, and EVE) to explore the Sun and its complex interior mechanisms in unprecedented detail.

Although the doors to the solar science payload will be opened starting just today (March 24), SDO has already managed to transmit its “first data”, Pesnell explained. This bonus science data from Earth’s radiation belt was unexpected he said. The first solar light data will come after the science instruments are fully activated.

SDO Instruments
“One detector in EVE was responding to the protons in the inner Van Allen radiation belt. We spent several orbits going through that part of space and EVE was able to produce a map of the radiation belt,” said Pesnell.

“The amount of proton data was not expected as we were not supposed to spend as much time in the belts as we did. By spending a few extra days in the inner belt the MEGS-P radiometer was able to measure a more complete picture of the radiation belt. It may be the only measurement of the proton fluxes in the inner radiation belt during the extremely low solar activity of the current solar minimum,” added Pesnell.

Check out of the science payload is moving ahead swiftly as planned. “The SDO instruments are working through their initial steps to turning them completely on”, Pesnell explained. A key activity was to “bake out” the instruments to remove any remaining harmful contaminants that could threaten to degrade the quality of the science data.

“CCD decontamination heaters had been turned on for several weeks to allow the instruments to outgas any residual contamination”, according to Pesnell. “During the first 40 days of the mission the instruments kept their CCDs hot with heaters. This prevents water vapor from condensing onto the surfaces of the CCDs while forcing water vapor out of the interior of the instruments. Two instruments, HMI and EVE, have turned off their decontamination heaters while AIA will turn them off next week. Those heaters are being turned off to allow the CCD’s to cool to their normal operating temperatures of about minus 100 C”.

“HMI will open their payload door Wednesday and begin checking out the instrument. EVE is cooling their CCDs getting ready to open their doors on Thursday. AIA will open their doors on Saturday”.

Pesnell mentioned that the SDO team expects to show off the initial data at a telecom in mid-April. “The science data should start to flow in early May, fully calibrated data will show up later. We will discuss the data at the SPD/AAS meeting in Miami, FL at the end of May”.

Van Allen Radiation Belts

SDO will collect a staggering 1.5 terabytes of data per day, equivalent to 380 full length movies per day on a 24/7 basis. “The data will be continuously beamed back to newly built receivers on Earth. We have no onboard recorders since nothing is available to handle such a huge data volume,” said Pesnell. “SDO will transmit 50 times more science data than any other mission in NASA history”.

Test data have already been transmitted via the spacecraft antenna to the receiving station on the ground in New Mexico, confirming that the vital communications systems are operating perfectly.

SDO’s measurements of the Sun’s interior, magnetic field and hot plasma of the solar corona will allow scientists to determine how violent solar events are created which then cause ‘space weather’ that ultimately affects every aspect of life here on Earth. The goal is create better predictions of ‘space weather’ in order to provide early warning to valuable satellites and astronauts operating in space, and to prevent disruption to navigation systems and failures in the power grid.

Rocket firing to raise SDO to its final orbit on March 16, 2010. click to enlarge
SDO was launched into a geosynchronous transfer orbit with an apogee altitude (farthest point from Earth) of 36,000 km (22,000 miles) and a perigee altitude (closest point to Earth) of 2500 km (1600 miles). Over the next 34 days the propulsion module was used to raise the perigee altitude to 36,000 km, with a few small burns to push both apogee and perigee to geosynchronous.

“SDO is in an inclined geosynchronous orbit at the longitude of New Mexico. The inclination of 28 degrees is the natural orbit when launched from Kennedy Space Center. Changing the inclination of an orbit requires a lot of fuel, so this orbit was less expensive than a geostationary orbit,” said Pesnell. This orbit will keep the observatory in constant view of the two newly constructed 18-meter dishes around the clock so that not a single bit of data should be lost.

Nancy Atkinson and Ken Kremer covered the Feb 11, 2010 SDO launch on site at KSC for Universe Today

Read SDO launch report by Nancy Atkinson here.

Read earlier SDO reports by Ken Kremer below, including from on site at the Atlas launch pad

NASA Sun Probe rolled to Pad; 10 hours to Blast off

NASA’s Solar Crown Jewel Bolted atop Atlas Rocket

NASA advanced Solar Observatory nearing February launch; will send IMAX like movies daily

Learn more at the NASA SDO Website

SDO soars to space from the Kennedy Space Center atop Atlas V rocket on Feb 11, 2010 as I observed from the KSC Press Site. Credit: Ken Kremer
Artist's concept of the Solar Dynamics Observatory in Orbit

Peggy Whitson: A Heroine of Science and Technology

Astronaut Peggy Whitson Photo: Cambria Harkey

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This post is part of Ada Lovelace Day, which is a worldwide effort to get as many people as possible to blog about a heroine of science or technology. Ada was a mathematician who lived in the 1800’s who created the first computer program. Yep — you read correctly — a computer in the 1800’s. It was actually a device called an analytical engine, which was an important step in the history of computers. You can read more about Ada and Ada Lovelace Day here.

The person I chose to write about is a goddess of both science AND technology. She is a biochemist and an astronaut. She was the first science officer on board the International Space Station and later become the first female commander of the ISS. She helped get some of the initial science programs going on the on the space station, and as commander oversaw a period of one of the biggest expansions for the station, coordinating the additions of European and Japanese laboratory modules. Her name is ….

Dr. Peggy Whitson

Perhaps I have always been drawn to Whitson because she grew up in a rural, agricultural environment, as I did. But I have always found Whitson to be endearing because of her easygoing and friendly personality. But yet, she must be almost a “slave-driver” and perfectionist when it comes to her work. During her expeditions on the ISS, Whitson earned a reputation for high achievement, which prompted mission planners to assign the crew extra work every day. NASA called it “The Peggy Factor.”

“We account for the fact that Peggy is going to do things more efficiently, and that she likes to work some on her time off, and so she’ll accomplish more,” said NASA deputy station project manager Kirk Shireman.

Whitson works with a science glove box on board the ISS. Credit: NASA

First some the details about Whitson: she graduated from Iowa Wesleyan College in 1981, and received her doctorate in biochemistry from Rice University in 1985. She worked as a Welch Postdoctoral Fellow before joining NASA in 1986.

From 1989 to 1993, Whitson was a research biochemist for NASA. During that time, she also served as an Adjunct Assistant Professor at the University of Texas and Rice University. In 1995, she became co-chair of a combined American and Russian working group, and a year later she was named an astronaut candidate.

Whitson flew her first space mission in 2002 as a flight engineer to the International Space Station as part of the Expedition 5 crew. While there, then NASA Administrator Sean O’Keefe gave her the title of first NASA Science Officer. Of course, she took some ribbing about being like “Spock,” the science officer on the original Star Trek, but she came to enjoy using the phrase “Live Long and Prosper.” During that mission she performed 21 experiments in human life science, microgravity sciences and commercial payloads.

During her second stint on the station, Expedition-16 in 2007-2008, she was named the commander.

I could go on about her accomplishments, but perhaps even better would be to let Whitson herself tell about her experiences in space. During her stays on the ISS, she wrote “letters home” to family and friends, answering questions and sharing details of her days in space.

Here’s what she had to say about doing science on the ISS:

I set up the first experiment inside the microgravity sciences glovebox this week. Tomorrow, I will do the powered checkouts of the glovebox and the next day start up the experiment. It is ssssoooo cool, getting to do science in space!!! This week we are also doing the urine collections for the renal stone investigation…and while I suspect this won’t be especially fun to collect the samples, I do think it’s one of the best experiments (I am biased, of course, since it is my experiment!).

In reading her letters, I found it interesting that she did amateur astronomy while on board the space station!:

One evening, I had dimmed the lights inside the module so that I could better watch the Earth/stars. I watched the sun set as we moved into the shadow of the Earth. I was pleasantly surprised a few min later to see a half-moon rise into view from behind the Earth. As the stars started popping into view, I was surprised again, as I saw a satellite pass by above us, looking so much like one of the other stars, but moving across the field of “constant” stars. I had never thought about the fact that I could, as one of those satellites, actually see another! And then I saw a second! Amazing.

Whitson during an EVA at the ISS. Credit: NASA

Whitson has conducted six spacewalks. Here’s how she described her first one:

My first look, as I poked my head out the hatch, was amazing! I previously compared the view of being in space to having lived in semidarkness for several years and having someone turn on the lights. Well, the view from my helmet, continuing the same analogy, would be like going outside on a sunny, clear day after having lived in semidarkness for years! If it gets better than this, I’m not sure my mind would be able to comprehend it!

And in this letter home, she waxes poetically about seeing Earth from space. She also talks about how people on Earth can watch for the ISS in the night sky, which is something that I love to do, and so it was interesting to read her perspective on that as well:

Although all the views of our planet are incredible and varied from our viewpoint up here on the Station, with the colors, textures, and lighting changing as we orbit…the most impressive view is the curve of the planet at the horizon. That curve is the special place where it is possible to see the layers of atmosphere extend beyond the surface to meet with the blackness of space beyond. Relative to the size of the Earth, it seems impossibly thin, less than a finger-width. The atmosphere carries all the shades of blue in that thin band, closest to the planet a glowing blue, like sunlit water over white sand, extending to the deepest blue-purple mixture that holds the blackness at bay.

As the night-side of the planet slips by beneath me, it carries on the fringes of darkness the colors of a sunset on the clouds below. The Station is still lit by the sun, despite the fact that we have already crossed the terminator between day and night below us. This is the timeframe when Station is most visible to folks on the ground, just before their dawn or after their dusk. A small bit of sunlight reflected off of our structure, illuminates us moving across their darkened sky. As the terminator approaches the horizon, the sun shows a blinding face that burns the atmosphere with molten reds and oranges before seemingly melting itself into the darkness, leaving a royal blue line that dissipates more slowly as the stars come out from hiding. Less than an hour passes before our path around the planet brings us back to the royal blue curve, signaling sunrise, as the process reverses itself. I am sure that after I return, I will again miss watching the curve of the Earth.

You can read more of Whitson’s letters home here.

Whitson’s ride home from space after Expedition 16 was more dramatic than expected. A malfunction made the Soyuz enter Earth’s atmosphere at a steeper angle than normal and the crew experienced “ballistic” descent at eight times the force of Earth-normal gravity. But, thankfully, everything turned out OK.

Whitson is currently chief of NASA’s astronaut office at Johnson Space Center.

Sources: Official NASA Astronaut bio, Orlando Sentinel