The Solar Dynamics Observatory Soars to Study the Sun

The Atlas V rocket carrying SDO roars off the launchpad. Credit: Nancy Atkinson

The Solar Dynamics Observatory launched successfully – and beautifully – Thursday morning from Cape Canaveral Launch Complex 41 to begin a 5-year mission that will provide streaming, high-definition views of our sun. It was the 100th launch of the Atlas/Centaur combo, and was a gorgeous sight as it roared and soared into the blue Florida sky. “It was great; a beautiful launch,” said Dean Pesnell, SDO Project Scientist, immediately after the launch. “The rocket rises so slowly off the pad — it is wonderful to see. This is third Atlas launch I’ve seen and this is the best one so far.”

Amazingly, viewers here at Kennedy Space Center saw the Atlas rocket fly close to a sundog just as the spacecraft reached Max-Q, creating a ripple effect around the spacecraft. “We saw this sundog come out and SDO flew right through it. Then the sun dog disappeared,” said Pesnell. “This may be the first time we’ve sent a probe through a sundog, and people will be studying this, so already we are learning things about our atmosphere from SDO.”

See this amazing video shot by a 13-year-old girl in attendance at the KSC VIP site that shows the sundog and shockwave. (as noted by Jon Hanford in the comments).

Today’s countdown was extremely smooth as the high winds that thwarted Wednesday’s launch attempt calmed as the opening of the launch window approached. After counting down to the planned T-4 minute hold, launch managers proceeded directly to launch at the beginning of the window at 10:23 a.m. EST.

Project Scientist Dean Pesnell describing the launch. Image: Nancy Atkinson

“I was a little worried about the clouds coming in,” said Tom Woods, Principal Investigator for the EVE instrument on SDO, the EUV Variability Experiment, which will be studying the extreme ultraviolet radiation of the Sun. “But we were very excited to see SDO launch today, as otherwise it would have been a 10-day delay until the next attempt. It was a wonderful launch!”

“It was so beautiful,” said Lika Guhathakurta, SDO program scientist immediately following the launch as we walked together back to the press building. “I can still feel the rumbling in my stomach!”

SDO science team celebrates after the launch: Dean Pesnell, Jennifer Rumburg, Chris St. Cyr, and Lika Guhathakurta. Image: Nancy Atkinson

Called the “Crown Jewel” of NASA’s fleet of solar observatories, SDO is a technologically advanced spacecraft that will take images of the sun every 0.75 seconds and daily send back about 1.5 terabytes of data to Earth — the equivalent of downloading 380 full-length movies every day.

SDO launch. Credit: Nancy Atkinson

“We’re going to be able to better understand the Sun as a star,” said Guathakurta, “but SDO will also give us a comprehensive view of how it interacts with the Earth and everything else in the solar system.

The sun’s dynamic processes affect everyone and everything on Earth. SDO will explore activity on the sun that can disable satellites, cause power grid failures, and disrupt GPS communications. SDO also will provide a better understanding of the role the sun plays in Earth’s atmospheric chemistry and climate.

Vapor trail from the Atlas rocket after the SDO launch. Image: Nancy Atkinson

A contrail from the launch appeared only in the region of Earth’s atmosphere where conditions were right for cloud formation. “There weren’t any clouds there, but we provided the very fine particles so that a contrail cloud appeared,” said Pesnell.

A later update confirmed that SDO separated from the Centaur and the spacecraft’s solar arrays deployed on time and correctly, and are now generating power.

Here’s the video of the launch from NASA TV:

Hubble Captures Double Aurorae Light Show on Saturn

Hubble's view of Saturn with a double view of its fluttering aurorae. Credit: NASA, ESA and Jonathan Nichols (University of Leicester)


In January and March 2009, researchers using Hubble took advantage of a rare opportunity to record Saturn when its rings are edge-on, resulting in a unique look featuring both of the giant planet’s poles. And Saturn cooperated by providing an incredible double light show with Saturn’s own northern and southern lights. Since Saturn is only in this position every 15 years or so, this favorable orientation has allowed a sustained study of the two beautiful and dynamic aurorae.

Since it takes Saturn almost thirty years to orbit the Sun, the opportunity to image both of its poles occurs only twice in that period. Hubble has been snapping pictures of the planet at different angles since the beginning of the mission in 1990, but 2009 brought a unique chance for Hubble to image Saturn with the rings edge-on and both poles in view. At the same time Saturn was approaching its equinox so both poles were equally illuminated by the Sun’s rays.

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These recent observations go well beyond just a still image and have allowed researchers to monitor the behavior of both Saturn’s poles in the same shot over a sustained period of time. The movie they created from the data, collected over several days during January and March 2009, has aided astronomers studying both Saturn’s northern and southern aurorae. Given the rarity of such an event, this new footage will likely be the last and best equinox movie that Hubble captures of our planetary neighbor.

Despite its remoteness, the Sun’s influence is still felt by Saturn. The Sun constantly emits particles that reach all the planets of the Solar System as the solar wind. When this electrically charged stream gets close to a planet with a magnetic field, like Saturn or the Earth, the field traps the particles, bouncing them back and forth between its two poles. A natural consequence of the shape of the planet’s magnetic field, a series of invisible “traffic lanes” exist between the two poles along which the electrically charged particles are confined as they oscillate between the poles. The magnetic field is stronger at the poles and the particles tend to concentrate there, where they interact with atoms in the upper layers of the atmosphere, creating aurorae, the familiar glow that the inhabitants of the Earth’s polar regions know as the northern and southern lights.

At first glance the light show of Saturn’s aurorae appears symmetric at the two poles. However, analysing the new data in greater detail, astronomers have discovered some subtle differences between the northern and southern aurorae, which reveal important information about Saturn’s magnetic field. The northern auroral oval is slightly smaller and more intense than the southern one, implying that Saturn’s magnetic field is not equally distributed across the planet; it is slightly uneven and stronger in the north than the south. As a result, the electrically charged particles in the north are accelerated to higher energies as they are fired toward the atmosphere than those in the south. This confirms a previous result obtained by the space probe Cassini, in orbit around the ringed planet since 2004.

Source:
ESA

Falcon 9 Flight Hardware Arrives at Cape Canaveral

The Falcon 9 vehicle undergoes final integration in the hangar at the SpaceX launch site in Cape Canaveral, Florida. The vehicle's nine Merlin 1C engines are at far left, and second stage is at far right. Credit: SpaceX

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SpaceX announced Thursday that all flight hardware for the first launch of the Falcon 9 rocket has arrived at the SpaceX launch site, at Space Launch Complex 40 (SLC-40), in Cape Canaveral, Florida, which I was able to see earlier this week. The final delivery included the Falcon 9 second stage, which recently completed testing at SpaceX’s test facility in McGregor, Texas. SpaceX has now initiated full vehicle integration of the 47 meter (154 feet) tall, 3.6 meter (12 feet) diameter rocket. In an upcoming launch, possibly as early as March, SpaceX will test their the cargo- and crew-carrying ability, using a Dragon spacecraft qualification unit. Since SpaceX is poised to figure prominently in the future of human spaceflight, the upcoming test flight is crucial, both for SpaceX and NASA.

“We expect to launch in one to three months after completing full vehicle integration,” said Brian Mosdell, Director of Florida Launch Operations for SpaceX. “Our primary objective is a successful first launch and we are taking whatever time necessary to work through the data to our satisfaction before moving forward.”

Flight hardware for the inaugural launch of Falcon 9 rocket undergoing final integration in the hangar at SpaceX's Cape Canaveral launch site in Florida. Components include: Dragon spacecraft qualification unit (left), second stage with Merlin Vacuum engine (center), first stage with nine Merlin 1C engines (right). Credit: SpaceX

Following full vehicle integration, SpaceX will conduct a static firing to demonstrate flight readiness and confirm operation of ground control systems in preparation for actual launch.
Space Launch Complex 40 (SLC-40), in Cape Canaveral. Credit: Nancy Atkinson

Though designed from the beginning to transport crew, SpaceX’s Falcon 9 launch vehicle and Dragon spacecraft will initially be used to transport cargo. Falcon 9 and Dragon were selected by NASA to resupply the International Space Station (ISS) once Shuttle retires. The $1.6B contract represents 12 flights for a minimum of 20 tons to and from the ISS with the first demonstration flights beginning in 2010.

Source: SpaceX

Where In The Universe #91

It’s time once again for another Where In The Universe Challenge. Test your visual knowledge of the cosmos by naming where in the Universe this image was taken and give yourself extra points if you can name the spacecraft responsible for this picture. Post your guesses in the comments section, and check back on later at this same post to find the answer. To make this challenge fun for everyone, please don’t include links or extensive explanations with your answer. Good luck!

UPDATE: The answer has been posted below:

This is a planetary nebula with some issues, as it is bipolar. M2-9 is a striking example of a ‘butterfly’ nebula. Another more revealing name might be the ‘Twin Jet Nebula,’ as it looks like a pair of exhaust steams from jet engines. The image was taken by the Hubble Space Telescope and you can get more info on it here from the ESA Hubble website.

Check back next week for another WITU challenge!

Pirouettes and Twitpics from Space

"Shuttle, approaching to ISS at dawn. Just imagine that this beast emerging from the complete darkness. KOOL!" Tweeted @Astro_Soichi, Soichi Noguchi

If you were watching NASA TV late Tuesday/early Wednesday you likely saw the beautiful backflip maneuver that space shuttle Endeavour performed before docking at 12:06 a.m. EST with the International Space Station. It was a striking sight to behold (see video above) as Commander George Zamka guided the orbiter through the nine-minute Rendezvous Pitch Maneuver, rotating the orbiter backwards so that space station astronauts could take high-resolution pictures of the shuttle’s heat-resistant tiles. Meanwhile, the ISS astronauts not taking the hi-res images were busy taking pictures of the approaching orbiter and posting them on Twitter.

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See more Twitpics from @Astro_Soichi

The detailed images of the Endeavour’s heat shield were analyzed on Wednesday and showed that everything looked “nominal” in NASA speak, and that no further examinations are required until after the shuttle undocks with the ISS. There are two other minor problematic items that NASA is monitoring for the shuttle.

Endeavour approaches ISS. A Soyuz docked to the station above the shuttle. Credit: NASA

A round ceramic spacer near one of the cockpit windows is sticking out. And a thermal tile repair that was made before the flight has failed, and the original crack is back, right over the cockpit.

Mission management team leader LeRoy Cain said Wednesday that neither problem appears to be serious. But he said everyone wants to be “very vigilant and take a closer look” in case spacewalking repairs are needed.

The shuttle astronauts had to wait about an hour longer than usual before entering the ISS. The vibrations that normally occur when the two spacecraft meet up and dock lasted longer than usual. Space shuttle flight director Kwatsi Alibaruho said this was caused by the massive and unsymmetrical bulk of the joined space station and shuttle, as well as the constant pull of Earth’s gravity on the “stack.” “It certainly not unexpected,” Alibaruho said.

The ISS and shuttle astronauts are now working together, getting ready for taking the Tranquility Node from the shuttle payload bay to attach it to the station. the first spacewalk of the mission. Today Endeavour’s crew transferred supplies from the shuttle’s middeck to the space station, including spacewalking equipment. Tonight, spacewalkers Bob Behnken and Nicholas Patrick will sleep in the Quest airlock as part of the overnight “campout” procedure that helps purge nitrogen from their bloodstreams, preventing decompression sickness once they move out into the vacuum of space.

See this interactive Flash feature from NASA which highlights the activities for each day of the shuttle mission.

Hat Tip to Stu Atkinson on the Twitpics

Russia May Raise Price of Soyuz Seats

A Soyuz docked to the ISS. Credit: NASA

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Price gouging or simple laws of supply and demand? The Soyuz will soon be the only ride in town to the International Space Station, and reportedly, Russia is considering raising the price per seat. NASA and Roskosmos have an agreement for six rides to the ISS in 2012 and 2013, at a rate of about $51 million dollars per US astronaut. “We have an agreement until 2012 that Russia will be responsible for this,” Roskomos head Anatoly Perminov was quoted by the Interfax news agency. “But after that? Excuse me, but the prices should be absolutely different then!”

The end of the shuttle program means NASA has to buy rides on the Soyuz. The total deal of $306 million (224 million euros) seems to be a pretty good deal for Roskomos. But they say in order to provide seats for the NASA astronauts, they’ll have to quit their space tourism program, which charges only $35 million (28 million euros) per seat.

The $51 million includes training, equipment, medical checks, supplies, services for launch operations and support personnel to launch site, flight control operations, and rendezvous and docking services.

NASA says these services are “serving as a bridge between the Space Shuttle and the availability of a commercial vehicle. Until a commercial vehicle is available, continued access to Russian Crew launch, return, and rescue services is essential for planned ISS operations and utilization by all ISS partners.”

New VISTA of Orion

Orion from the VISTA infrared telescope. Credit: ESO

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Oh-oh-oh Orion! The new VISTA (Visible and Infrared Survey Telescope for Astronomy) infrared survey telescope has used its huge field of view to show the full splendor of the Orion Nebula. With its infrared eyes, it has peered deeply into dusty regions that are normally hidden to expose the curious behavior of the very active young stars buried there.

VISTA is the latest addition to ESO’s Paranal Observatory. It is the largest survey telescope in the world and is dedicated to mapping the sky at infrared wavelengths. The large (4.1-metre) mirror, wide field of view and very sensitive detectors make VISTA a unique instrument. This dramatic new image of the Orion Nebula illustrates VISTA’s remarkable powers.

The Orion Nebula is about 1,350 light-years from Earth. Although spectacular when seen through an ordinary telescope, what can be seen using visible light is only a small part of a cloud of gas in which stars are forming. Most of the action is deeply embedded in dust clouds and to see what is really happening astronomers need to use telescopes with detectors sensitive to the longer wavelength radiation that can penetrate the dust. VISTA has imaged the Orion Nebula at wavelengths about twice as long as can be detected by the human eye.

Four highlights of the new VISTA image of Orion. Credit: ESO

On the upper-left, the central region of VISTA’s view of the Orion Nebula is shown, centered on the four dazzling stars of the Trapezium. A rich cluster of young stars can be seen here that is invisible in normal, visible light images. In the lower-right panel the part of the nebula to the north of the center is shown. Here there are many young stars embedded in the dust clouds that are only apparent because their infrared glow can penetrate the dust and be detected by the VISTA camera. Many outflows, jets and other interactions from young stars are apparent, seen in the infrared glow from molecular hydrogen and showing up as red blobs. On the upper-right, a region to the west of center is shown. Here the fierce ultraviolet light from the Trapezium is sculpting the gas clouds into curious wavy shapes. A distant edge-on spiral galaxy is also seen shining right through the nebula. At the lower-left a region south of the center is shown. Each extract covers a region of sky about nine arcminutes across.

All these features are of great interest to astronomers studying the birth and youth of stars.

Source: ESO

We Moved the Universe Today

Just to let you know, I’ve moved Universe Today to a new server today. Everything seems to be working, but I’m sure there are still going to be problems (there are always problems). I’m hoping this should make the site a lot faster and more responsive. If you notice something misbehaving, please email me at [email protected].

Thanks!

Fraser

SDO Launch Scrub; Try Again Tomorrow

SDO on the launchpad. Credit: Nancy Atkinson

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Note: Nancy Atkinson is at Kennedy Space Center to cover SDO and the STS-130 shuttle mission

Scrub! High winds kept the Solar Dynamics Observatory on the ground for today, but the launch team will try again Thursday (Feb. 11) at 10:26 a.m. EST (15:26 GMT). Weather is 60% go for tomorrow, and winds will be down to about 16 knots but cloud cover may be an issue. Today, winds consistently peaked well above the constraint speed of 20 knots – often well into the 30’s. The winds here at the press site were equally strong, and combined with cool weather, kept most people indoors until the launch team gave the go-ahead.

Winds were predicted to decrease later in the day, so the launch team pushed back the countdown as far into the launch window as possible. Originally slated for a 10:26 a.m. EST launch, they first moved it ahead 30 minutes to 10:56, and then to 11:26, leaving just the built-in hold at T-4 minutes in the countdown, — and more importantly, leaving only four minutes for a possible attempt. The count was able to pick up when the weather officer gave the go-ahead, but as soon as the countdown restarted, the count was automatically stopped because the wind loads had risen again.

The scrub was a disappointment for the SDO team, which has had repeated delays in their timeline leading up to launch. But now SDO and the Atlas V rocket can launch any day that the weather allows, so we’ll be back again tomorrow for another try!

You can follow my updates on Twitter (@Nancy_A) for live, real-time updates. I’ll also be reporting live Thursday morning on AstronomyFM, a 24-hour internet radio dedicated to astronomy and space exploration.

An XO For Valentine’s Day…

The planet XO-3b, and the star XO-3 positions - Credit : DSS survey

[/caption]Almost everyone the world over recognizes the letters X and O to represent a kiss and a hug, but this time the XO stands for Extrasolar Planet XO-3b. If you’d like an extra special “kiss and hug” for Valentine’s Day, then why not visit with Baraket Observatory on Februrary 13th as they present their live, on-line AstroCast of XO-3b transiting its parent star! This is definitely an event you won’t want to miss, so step inside for more information…

On February 13, 2010, Baraket Observatory will webcast (weather permitting) the transit of an extra solar planet named “XO-3b”. The event will be observed by using a highly sophisticated robotic telescope and a sensitive cooled CCD camera. The observatory will transfer live images of the transit as they’re being captured by the Bareket Internet EDU scope, while plotting its light curve through the site as the transit progress. This truly amazing process will give students and the general pubic a unique in side view to behind the observatory scenes, while presenting to the viewers how science is being done – all in real time. The event will be about 2 hours in duration, scheduled to take place at 19:00 UTC.

Live Astro-cast of the ExtraSolar Planet XO-3b Transit

Live Astro-cast of the ExtraSolar Planet XO-3b Transit (European Server)

The American Association of Variable Star Observers (AAVSO) is collaborating with Bareket Observatory on variable-object studies, of which transiting exoplanets are a key element. The AAVSO has calibrated nearby stars in each of the known transiting exoplanet systems to act as local standards against which you can compare the host star for variability. The AAVSO is also working with the XO project team to study other variable stars that they have discovered during their exoplanet survey. Exoplanet transits are hard to detect, since the dip is only one percent or so in brightness, but with care, any amateur observer with a CCD camera can watch the transit of a planet around another star. A transit means the extra solar planet acts very similar to Venus, in our own solar system, when it passed in front of our Sun (in a direct geometrical line between the sun and the Earth), featuring a “mini eclipse”. While Venus can be easily observed against the solar disc, the extended XO-3b planet only presented as a dim singular dot in the sky. While it’s total brightness only slightly vary during the extra solar planet transit, for a relatively short period of time. The drop in the brightness is proportional to the planet’s surface. Usually within a 1% for a gaseous giant (Such as Jupiter) and as low as 0.01% for an Earth–sized planet. Searching for extra solar planets by detecting their transit is well within the possibilities of many today’s Earth based observatories and now watching a transit electronically is like a dream come true!

Flowers and candy for Valentine’s Day? Sure, that’s nice… But if you want to win an astronomer’s heart, give ’em a big XO!

This project is a part of the Bareket observatory Live-@stro outreach programs.