The Awesome Complexity of Hypersonic Flight

Stanford professor Parviz Moin shows a simulation of temperature fluctuations from a scramjet exhaust.


Researchers at Stanford University are working on solutions to the inherent difficulties of hypersonic flight — speeds of over Mach 5, or 3,000 mph (4828 km/h) — and they’ve created one amazing computer model illustrating the dynamics of air temperature variations created at those intense speeds.

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According to a news article from Stanford University, “Real-world laboratories can only go so far in reproducing such conditions, and test vehicles are rendered extraordinarily vulnerable. Of the U.S. government’s three most recent tests, two ended in vehicle failure.”

The video above shows some of the research team’s animation model — one of if not the largest engineering calculation ever created, it ran on 163,000 processors simultaneously and took 4 days to complete! And it’s utterly mesmerizing… not to mention invaluable to researchers.

“It’s something you could never have created unless you put computer scientists, mathematicians, mechanical engineers and aerospace engineers together in the same room,” said Juan Alonso, associate  professor of aeronautics and astronautics at Stanford. “Do it, though, and you can produce some really magical results.”

In a (very tiny) nutshell, the behavior of air through an hypersonic engine — called a scramjet (for supersonic combustion ramjet) — changes at extremely high speeds. In order for aircraft to travel and maneuver reliably the scramjets have to be engineered to account for the way the air will respond.

“If you put too much fuel in the engine when you try to start it, you get a phenomenon called ‘thermal choking,’ where shock waves propagate back through the engine,” explained Parviz Moin, the Franklin P. and Caroline M. Johnson Professor in the School of Engineering. “Essentially, the engine doesn’t get enough oxygen and it dies. It’s like trying to light a match in a hurricane.”

“Understanding and being able to predict this phenomena has been one of the big challenges. It’s not one number or two numbers that come out of it at the end of the day… it is all of these structures that you see back there, the richness of it. It is understanding that allows you to control.”
– Parvis Moin, Stanford University professor

Thanks to this study, made possible by a 5-year $20 million grant from the U.S. Department of Energy, we may one day have aircraft that can travel up to 15 times the speed of sound. But the team’s groundbreaking computations aren’t just reserved for aeronautic aspirations.

“These same technologies can be used to quantify flow of air around wind farms, for example, or for complex global climate models,” said Alonso.

Read more on the Stanford University News here.

Video by Steve Fyffe and Linda Cicero. Source: Stanford University.

Watch Jupiter as a ‘Space Invader’

This great video created from images taken by the Solar and Heliospheric Observatory (SOHO) on May 13 and 14 show Jupiter as it comes close to the Sun (from our vantage point) in a solar conjunction. But what it really looks like is the old “Space Invaders” video game, with Jupiter marching across the screen. There’s even a couple of sungrazing comets “pewpew-ing” in like the laser cannon shots in the game, and a coronal mass ejection completes the scene as an explosion (which is actually more like “Asteroids.”) For more fun, the team who created this video at the Naval Research Laboratory’s Sungrazing Comets website takes the time to show all the different objects in the scene, which amazingly includes Callisto and Ganymede, two of Jupiter’s moons. All it needs is the funky video game background music.
Continue reading “Watch Jupiter as a ‘Space Invader’”

Can You Find a Hubble Hidden Treasure?

Visible in the constellation of Andromeda, NGC 891 is located approximately 30 million light-years away from Earth. Credit: ESA/Hubble & NASA

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Just look at the kind of stunning images that are buried in the archives from the Hubble Space Telescope! Here, Hubble turned its powerful wide field Advanced Camera for Surveys towards this spiral galaxy and took this close-up of its northern half. The entire galaxy, called NGC 891, stretches across 100,000 light-years and we see it exactly edge-on. Visible are filaments of dust and gas escaping the plane of the galaxy. A few foreground stars from the Milky Way shine brightly in the image, while distant elliptical galaxies can be seen in the lower right of the image.

This is just an example of the hidden gems in Hubble’s archives that have never been seen by the general public. There’s a new contest to find more — so how can you participate?

The HST has made over one million observations during its more than two decades in orbit. New images are published nearly every week, but hidden in Hubble’s huge data archives are some truly breathtaking images that have never been seen. They’re called Hubble’s Hidden Treasures, and between now and May 31, 2012, ESA invites you to help bring them to light. Just explore the Hubble Legacy Archive (HLA), and dig out a great dataset, adjust the contrast and colors using the simple online tools, and submit to the Hubble’s Hidden Treasures Contest Flickr group. For more information about the competition, visit the Hubble’s Hidden Treasures webpage.

The European Southern Observatory (ESO) also conducted a similar ‘treasure hunt’ with great results

This image was found by contestant Nick Rose.

How Big Are Sunspots?

Sunspots from today and from 65 years ago, with planet sizes for comparison.

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The short answer? Really big. The long answer? Really, really big.

The image above shows sunspot regions in comparison with the sizes of Earth and Jupiter, demonstrating the sheer enormity of these solar features.

Sunspots are regions where the Sun’s internal magnetic fields rise up through its surface layers, preventing convection from taking place and creating cooler, optically darker areas. They often occur in pairs or clusters, with individual spots corresponding to the opposite polar ends of magnetic lines.

(Read “What Are Sunspots?”)

The image on the left was acquired by NASA’s Solar Dynamics Observatory on May 11, 2012, showing Active Region 11476. The one on the right comes courtesy of the Carnegie Institution of Washington, and shows the largest sunspot ever captured on film, AR 14886. It was nearly the diameter of Jupiter — 88,846 miles (142,984 km)!

“The largest sunspots tend to occur after solar maximum and the larger sunspots tend to last longer as well,” writes SDO project scientist Dean Pesnell on the SDO is GO blog. “As we move through solar maximum in the northern hemisphere and look to the south to pick up the slack there should be plenty of sunspots to watch rotate by SDO.”

Sunspots are associated with solar flares and CMEs, which can send solar storms our way and negatively affect satellite operation and impact communications and sensitive electronics here on Earth. As we approach the peak of the current solar maximum cycle, it’s important to keep an eye — or a Solar Dynamics Observatory! — on the increasing activity of our home star.

(Image credit: NASA/SDO and the Carnegie Institution)

SpaceX says All Systems GO for Historic May 19 Blast Off to ISS

SpaceX Dragon approaches the ISS on COTS 2 test flight slated for May 19 liftoff and docking of Day 4. Astronauts will grapple it with the robotic arm and berth it at the Earth facing port of the Harmony node. Illustration: NASA /SpaceX

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In less than 48 hours, SpaceX is primed to make history and launch the first ever commercial rocket and spacecraft to the International Space Station (ISS) early Saturday morning on May 19.

Following today’s Launch Readiness Review (LRR), SpaceX was just given the official “GO” from NASA to proceed with the blastoff of the Falcon 9 at 4:55 a.m. EDT (0855 GMT) from Space Launch Complex-40 on Cape Canaveral Air Force Station in Florida. This also marks the first night time liftoff of the Falcon 9 rocket.

“Just passed final launch review with NASA”, SpaceX CEO Elon Musk tweeted this evening. “All systems go for liftoff on Sat morn”.

The SpaceX developed Dragon cargo resupply spacecraft is bolted on top of the two stage Falcon 9 rocket and stands 157 feet tall for the mission dubbed “COTS 2”. The Falcon 9 booster generates 1 million pounds of thrust

The official Air Force weather forecast gives a 70% chance of acceptable conditions for launch. The primary concern for launch day is a violation of the Cumulus Cloud Rule. On the heels of a significant drought, stormy weather has rolled into the Florida Space Coast and thunder is striking the area at the moment.

In the event of a launch scrub, the next launch opportunity comes in three days on May 22.

The launch will be broadcast live on NASA TV and via SpaceX Webcast at http://spacex.com

This SpaceX Falcon 9 rocket inside the processing hanger at Pad 40 is due for liftoff on May 19, 2012 to the ISS. Credit: Ken Kremer/www.kenkremer.com

Technicians plan to roll the Falcon 9/Dragon duo out to the seaside launch pad tonight. The rocket will be moved on rail tracks about 600 feet from the processing hanger to the pad and vertically erected.

The purpose of Dragon is to carry supplies up to orbit and dock at the ISS and partially replace the capabilities of NASA’s now retired space shuttle. Dragon is a commercial spacecraft designed and developed by SpaceX.

SpaceX is under contract with NASA to conduct twelve resupply missions to the ISS to carry cargo back and forth for a cost of some $1.6 Billion.

The Dragon spacecraft is loaded with nearly 1200 pounds of non-critical cargo such as food and clothing on this flight. A collection of student experiments, commemorative patches, pins and emblems will also be on board Dragon’s upcoming test flight.

On Friday, Ken will be reporting from Space Launch Complex-40 on Cape Canaveral.

Ken Kremer

Ring of Fire! Annular Solar Eclipse on May 20

As the solar eclipse on May 20th progresses, its partial and annular phases will look very similar to this eclipse on May 10, 1994. Photo by Fred Espenak/SkyandTelescope.com.

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There’s a great reason to look up this weekend and hope for clear skies! On May 20-21 an annular eclipse of the Sun will be visible from a 300 kilometer-wide track that crosses eastern Asia, the northern Pacific Ocean and the western United States. An annular eclipse means the Moon will not cover the Sun completely, and so when the Moon is directly in front of the Sun, there will be a bright ring of visible light on the surrounding edges, creating a so-called ‘ring of fire.’ The eclipse begins at 20:56 UTC (16:56 EDT US time) on May 20, and ends at 02:49 UTC May 21 (22:49 on May 20 EDT).

Not in that swath? See the map below, but you may be able to see a partial eclipse if you are in Asia, the Pacific and the western two-thirds of North America.

A map of the area where the annular eclipse can be seen. The dark strip in the center indicates the best locations for viewing the eclipse. The eclipse is also visible in the areas that are shaded red, but less of the Sun's disk is obscured. The fainter the red shading the less of the Sun's disk is covered during the eclipse. Click on this image for an interactive map from TimeandDate.com

Still not in the path of the Sun during that time? There will be several webcasts, including one from SLOOH, and more from Hong Kong, the summit of Mt. Fuji in Japan, and Area 51 in Nevada USA (no alien spaceships will be seen in this webcast, guaranteed.)

An important note if you ARE in an area where you can see the eclipse. DO NOT look directly at the Sun, and especially do not look through a telescope or binoculars at the Sun with your eyes directly. That ‘ring of fire’ will indeed burn, burn, burn your retinas, and could cause serious and permanent eye damage. There are special eclipse glasses, or you can make your own eclipse viewers. Mr. Eclipse has a whole list with instructions for pinhole cameras, and other safe viewing methods. If you have a telescope, the folks from Galileoscope have instructions for how to build a Sun-funnel for safe viewing

We posted an article last week about special eclipse glasses you can purchase, but you might be running out of time to buy them.

If you take any images of the eclipse (again, know what you are doing and be careful!) please share them with us via our Flickr page, or send them in via email. We’ll have a grand eclipse gallery of images from around the world!

Some of the spacecraft will also be observing the eclipse and will provide images and movies, such as the JAXA/NASA Hinode mission. You will be able to see the images and videos here, and as an added bonus Hinode’s X-ray Telescope will be able to provide images of the peaks and valleys of the lunar surface.

Unfortunately, the orbits the Solar Dynamics Observatory (SDO), the Solar Terrestrial Relations Observatory (STEREO), and the Solar Heliospheric Observatory (SOHO) will not provide them with a view of the eclipse.

You can see more eclipse information from Sky and Telescope, NASA and TimeandDate.com

The next solar eclipse will be the total solar eclipse on November 13, 2012.

Here’s a video from NASA:

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JPL Wants To FINESSE Info From Exoplanets

FINESSE would observe exoplanets from a position in low-Earth orbit (NASA/JPL-Caltech)


Jet Propulsion Laboratory’s proposed FINESSE space telescope may not hunt for exoplanets, but it will find out what they’re made of.

Part of NASA’s Explorers program, FINESSE — which stands for (take a deep breath) Fast INfrared Exoplanet Spectroscopy Survey Explorer — would gather spectroscopic data from 200 known exoplanets over a two-year period, helping scientists to determine the composition of their atmospheres, surfaces, and even their weather.

While huge discoveries have been made by both ground- and space-based telescopes like Kepler and Corot over the past several years, identifying thousands of exoplanetary candidates, FINESSE will be the first mission dedicated to finding out what the atmospheres are like on worlds outside our solar system.

Using a sensitive spectrograph covering 0.7-5.0 microns, FINESSE will be able to identify molecular bands of water, methane, carbon monoxide, carbon dioxide, and other molecules. Its sensitivity and stability will even allow it to detect the differences between an exoplanet’s day and night side, allowing wind flow and weather to be determined.

Known as an Offner spectrometer, the design of the FINESSE detector is derived from the Moon Mineralogy Mapper instrument, which was designed at JPL and flew to the Moon aboard India’s Chandrayaan-1 spacecraft.

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Touted as “the next step” in exoplanetary exploration, FINESSE is proposed for launch in October 2016.

Learn more at JPL’s FINESSE site here.

“FINESSE is the next step in humankind’s journey of understanding our place in the cosmos.”

– Mark Swain, principal investigator for FINESSE

Watch How Life Recovers from Devastation

If a portion of Earth underwent a major cataclysm, how long would it take for life to recover? The 1980 eruption of Mount St. Helens is giving scientists an unprecedented opportunity to witness a recovery from devastation, as the eruption leveled the surrounding forest, blasted away hundreds of meters of the mountain’s summit, and claimed 57 human lives. Landsat satellites have tracked the what has happened on the mountain, and how the forest was reclaimed — all on its own. This video shows a timelapse of the recovery, with annual images from 1979-2011 from the Landsat satellites, which acquired the images seen here between 1979 and 2011.
Continue reading “Watch How Life Recovers from Devastation”