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

Chinese Dragon in Space!

NGC 5189. Credit: ESO

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This new image from the ESO telescope in Chile shows what looks like a Chinese dragon in the sky. But really, it is NGC 5189 an S-shaped planetary nebula adorned with red and green cosmic fireworks. This dragon isn’t breathing fire – the colorful “smoke” is a signal that a star is dying.

At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate.

In particular, this planetary nebula exhibits a curious “S”-shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precession and this could result in the complex curves on the opposite sides of the star visible in this image.

This image has been taken with the New Technology Telescope at ESO’s La Silla Observatory in Chile, using the now decommissioned EMMI instrument. It is a combination of exposures taken through different narrowband filters, each designed to catch only the light coming from the glow of a given chemical element, namely hydrogen, oxygen and nitrogen.

Source: ESO

Mir’s Fiery Re-entry, March 23, 2001

The storied history of the Mir space station includes collisions, a fire, and political change. But it also consists of unprecedented long-duration spaceflights and scientific studies – and without it, the International Space Station may never have been built. Nine ten years ago, the journey of the 15-year-old Russian space station ended. On March 23, 2001, Mir re-entered the Earth’s atmosphere near Nadi, Fiji, and fell into the South Pacific. The planned and controlled re-entry began when the engines of a cargo ship docked to Mir were fired causing the station’s orbit to brake, starting Mir’s descent. The video here shows both real and computer generated images of the breakup of the 143-ton station as it descended to Earth.
Continue reading “Mir’s Fiery Re-entry, March 23, 2001”

Review: Hubble 3-D IMAX

Hubble 3-D IMAX movie poster.

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I have seen the new Hubble 3-D IMAX movie twice now, and both times I was overcome with tears by the end of the film. It wasn’t that the story of Hubble itself was overwhelming; no, that story I already knew by heart. It wasn’t that the account of the servicing mission to save Hubble was especially dramatic; actually, I think watching the five EVAs live on NASA TV in May 2009 was more heart-pounding. And it wasn’t that the cinematography was overly stunning or that there were non-stop 3-D effects.

What this film does is portray the immensity and gloriousness of our universe, and that we are currently, serendipitously, living during an amazing era of discovery, one that humanity has never known before. Some of these discoveries we are only able to make because of this marvelous telescope and the people who laid their lives on the line to fix it and make it better. It also shows — almost subtly – that we are inexorably connected to the Universe around us, joined like the intertwining web of 3-D galaxies shown near the movie’s final scenes. We are witnessing – and are a part of – history.

The movie chronicles the 20-year life of Hubble, and focuses on the STS-125 servicing mission, the final mission to Hubble. There ARE wonderful 3-D views of Hubble itself, anchored to shuttle Atlantis’ payload bay, where the telescope appears to come out into the audience and into your lap. This includes stunning views of planet Earth spinning overhead. “This is a gift we astronauts have been given,” astronaut Mike Massimino says of the vistas that can only be seen from space.

And viewers get to experience not one, but two shuttle launches captured in the so-close-up-you-can-feel-it shots which can only be experienced in IMAX. But much of the footage from on-orbit detailing the EVAs and action inside the shuttle were shot with the regular, albeit high-tech cameras that normally NASA flies on missions, including the small “lipstick” cameras on the helmets of the spacewalkers, and some was able to be rendered in grainy, but effective 3-D. The only genuine IMAX 3-D camera on board the mission was bolted to the shuttle’s cargo bay and it carried only 5,400 feet of film – which translates into just 8 minutes of IMAX 3-D footage. Here’s an article about a 3 D Solar System

Endearing are the behind-the-scenes looks at the STS-125 mission. Astronauts joking with each other on orbit – Commander Scott Altman sticking gum under the shuttle’s “dashboard,” Massimino describing how suiting up for an EVA is like putting on a snowsuit as a child. “You need your Mom,” he says.

In both showings I attended, the scene that got the most audible reaction from the audience was Drew Feustal making a chicken salad tortilla wrap. But, hey, we all have to eat, and for those who have never seen food preparation or astronauts eating in space before, it holds a certain level of fundamental fascination.

Additionally we get to hear what is going through the minds of the astronauts on launch day. Mike Good recalls how his grandfather opened up the Universe by showing him views through a telescope. Megan McArthur glows with excitement. John Grunsfeld meticulously goes through in his mind all the tasks that lie before him and the crew.

The film quickly moves through the EVAs, highlighting anxious moments of the mission — stuck bolts, the handrail that Massimino had to rip off of Hubble, the tension of undertaking the meticulous repairs on a one-of-a-kind iconic telescope, all while wearing a bulky spacesuit. But within a 43 minute film, these situations are dealt with quickly, — and honestly, — the movie doesn’t give real justice to how tense some of these situations really were.

A vast canyon of dust and gas in the Orion Nebula from a 3-D computer model based on observations by NASA's Hubble Space Telescope. Credit: NASA, G. Bacon, L. Frattare, Z. Levay, and F. Summers (STScI/AURA)

But most mesmerizing in the film are 3-D visualizations of actual Hubble data. For this film, regular 2-D Hubble images were converted into 3-D environments, giving the audience the impression they are traveling through space and time.

Viewers get to experience an exhilarating ride through the Orion Nebula, swooping through a giant canyon of gas and dust, and witness star-forming regions that include dusty tadpole-shaped objects that are fledgling solar systems, likely a vision of how our own solar system once looked.

Later we travel to the distant Virgo Cluster and emerge on the other side of a black hole, and then travel back in time to witness early misshapen galaxies. Returning to more recent views that include new images from the Wide Field Camera 3 that was installed on STS-125, we see an ocean of stars in multiple wavelengths. Upon pulling away from the stars, we see 3-D galaxies interwoven like a web.

It’s these mind-numbing visions that produce a child-like sense of awe and wonder – and in my case, tears. The film is a testament to how Hubble has allowed us to see the wonders of our Universe.

I asked for reactions from the members of the audience following the premier showing of Hubble 3-D at the Kennedy Space Center IMAX, and while many commented on the amazing graphics, they also observed how small they felt in comparison to the rest of the Universe, but yet, incredibly an integral part of all that is.

The graphics were created by image processing specialists at Hubble’s Space Telescope Science Institute,– familiar names to those of us that follow Hubble : Frank Summers, Zolt Levay, Lisa Frattare, and Greg Bacon. They worked with the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign (more about them in a subsequent, upcoming article on Universe Today), and the Spitzer Science Center at the California Institute of Technology.

Hubble 3-D was directed by Toni Myers, who has been at the helm of all the space-themed IMAX movies, and narrated by Leonardo DiCaprio.

Go see the movie if you have the chance, and bring anyone who may not normally follow space exploration or astronomy. Their view of the Universe will never be the same.

For more info see the official Hubble 3-D IMAX website. Official trailer below.

First Flight of Virgin Galactic’s SpaceShipTwo

Virgin Galactic, the private aerospace company founded by billionaire Richard Branson, successfully tested the passenger space-plane SpaceShipTwo today. SpaceShipTwo (SS2), is also called the Virgin Space Ship Enterprise, or VSS Enterprise, an obvious tribute to another space vehicle of some note. SS2 was carried to 45,000 feet (13.7km) by its mothership, named WhiteKnightTwo (WK2), or ‘Eve’, after Branson’s mother. In this initial ‘captive carry’ test of the space plane, it remained attached to the mothership for the duration of the flight.

The SS2/WK2 combo took off from a runway at the Mojave Air and Space Port in California, and flew for approximately three hours over the deserts of the Antelope Valley. SS2 is a prototype passenger vehicle that is designed to take astronauts to suborbital flight. If the remaining tests go as planned, it will eventually take a crew of two pilots and up to six passengers to the edge of space, at just over 100km (62 miles).This may happen as early as the end of 2011.

SpaceShipTwo is an all-carbon composite plane that uses a hybrid rocket motor, and will be carried to 50,000 feet (15.2 km) by WhiteKnightTwo before being released. It will then fire the rocket to propel it above the Karman line.

Here’s a video of the takeoff and landing of SS2 today:

SS2 was unveiled to the public in December of last year, and this is the first in a series of tests to determine how safe and operational the craft is before it can begin to bring passengers into space. It will undergo another captive carry flight to 50,000 feet, and then will be brought into the air by WK2 and released in subsequent tests.

SpaceShipTwo was designed by Burt Rutan of Scaled Composites, who also led the design team for SpaceShipOne, which won the Ansari X-Prize of $10 million in 2004 for completing the first series of manned commercial spaceflights.

If you have $200,000 laying around and want to go into space, SS2 is your space plane. However, you’re going to have to get in line: over 300 people have already signed up for seats on the plane.

Source: Space.com, Virgin Galactic

Carnival of Space #146

This week’s Carnival of Space is hosted by our very own Mike Simonsen over at his very own website, Simostronomy!

Click here to read the Carnival of Space #145. Go give Mike a visit!

And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, let Fraser know if you can be a host, and he’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

Does The Sun Move?

The center of our Milky Way galaxy. Image credit: NASA.

[/caption]Does the Sun Move? What an interesting question. We mainly talk about everything in the solar system orbiting the Sun and celestial objects outside the solar system being in relation to the Sun. The answer to the question is : Yes. The Sun and the entire solar system orbits around the center of the Milky Way galaxy. The average velocity of the solar system is 828,000 km/hr. At that rate it will take about 230 million years to make one complete orbit around the galaxy.

You can check out these amazing books for more information about the Sun.

The Milky Way is a spiral galaxy. It is believed that it consists of a central bulge, 4 major arms, and several shorter arm segments. The Sun and the rest of our solar system is located near the Orion arm, between two major arms, Perseus and Sagittarius. The diameter of the Milky Way is about 100,000 light years and the Sun is located about 28,000 light-years from the Galactic Center. It has been suggested fairly recently that ours is actually a barred spiral galaxy. That means that instead of a bulge of gas and stars at the center, there is probably a bar of stars crossing the central bulge.

Everything in the known universe rotates on an axis and orbits something else in space. The Sun is no exception. Here is the NASA webpage about the sun’s movements through space. Astronomy Cast offers two good episodes: one is about the mysteries of the solar system and the other is about solar system movements.

IntelliScope

The Orion IntelliScope is a computerized object locator unit designed to compliment the Orion SkyQuest XT IntelliScope series of Dobsonian telescopes. It is essentially a handheld data base unit that plugs into a set of encoders mounted in the telescope base and axis – keeping track of the telescope’s position much like cursor and mouse work together on a computer screen. It consists of a two-line backlit LCD screen and illuminated keypad. The Intelliscope unit has an information base of 14,000 objects which include nebulae, galaxies, star clusters, double stars, planets and more.

It is the “more” that makes the Orion Intelliscope considerably different than a “GoTo”…

All computerized telescopes work on the same basic principle. They employ a set of positioning sensors located on the telescope’s ascension and declination axis – its up and down and right to left movement points. On a equatorial mount, these positions can be driven by a small set of servo motors which allows the telescope to automatically move itself to a selected position. These “GoTo” telescopes are a marvel of engineering, but with large aperture comes even a larger price. Traditionally, dobsonian style telescopes are favored by those who desire as much light gathering power as possible – made affordable by simplifying the telescope mount. As with all things, there is a trade-off. With affordable aperture, you lose the ability to “drive”.

The Orion Intelliscope solves the location equation by performing as digital setting circles. The specialized line of Orion SkyQuest XT IntelliScope Dobsonian Telescopes already have a set of high-resolution, 9,216-step digital encoders built into both axis. Simply plug the Computerized Object Locator into the base and you’re equipped to locate and view any of 14,000 celestial objects contained in its data base: : 837 stars (including double and variable stars), 7,840 NGC objects, 5,386 IC objects, 101 Messier objects, 8 major planets, and 99 user-entered objects. The Intelliscope unit features illuminated buttons and a backlit, two-line liquid crystal display (LCD). The intuitive menu buttons allow selection of objects by type (e.g., Planet, Nebula, Cluster, Galaxy) or catalog number (e.g., M57, NGC 253). Press the Tour button to select one of 12 tours of the best objects visible in any given month. Find something that you don’t know what it is? Then use the Intelliscope’s ID button to find out what object you’re viewing, if you’re not sure. The LCD screen provides information about the objects you see, including object type, common name (if any), magnitude, constellation, and a brief visual description.

How is this accomplished? Because the Orion IntelliScope Dobsonian telescope doesn’t employ drive motors, the user must manually move the telescope while watching the Intelliscope controller. A series of celestial coordinates will be displayed, prompting you to move the telescope in the desired direction – then simply watch the “countdown” until the telescope is in the proper position. While this seems easy, it does require some accurate user input to make it work correctly. Because the sky changes nightly, you must enter in the correct time and date. Our position on Earth also affects celestial positioning, so proper terrestrial coordinates must be selected from the database. Once this is entered in, the telescope tube must be leveled to make the “brain” understand the position – then at least two celestial points must be manually located, centered in the eyepiece and entered. This allows the Intelliscope unit to refine the telescope’s position – making its calculations more accurate. Haphazard entries will give you haphazard results!

The Orion Intelliscope Object Locator is a wonderful tool for both beginning and seasoned amateur astronomers. It will enable you to view many more celestial curiosities in an evening – and in a lifetime – than you ever dreamed possible. These telescope pointing systems are actually quite fun! Simply choose the aperture which suits your individual needs best, plug it in and away you go. But note… the IntelliScope Computerized Object Locator is not compatible with other encoder systems or other telescopes. Previous SkyQuest versions and SkyQuest XT Classic Dobsonian telescopes cannot be retrofitted for IntelliScope compatibility.

Amazing Mars Flyover Videos Keep Getting Better and Better

How do the folks from UnmannedSpaceflight do it?!! They keep surpassing themselves with every new flyover video! We’ve posted some Mars flyover videos before, created by UMSF founder Doug Ellison. Now, colleague Adrian Lark — who has been working on creating animations and enhanced images with data from the Mars missions for several years — has produced new features on the videos. This latest, which flies you around the scarp surrounding Olympus Mons has speed and height information as well as a context map included on the video. “The data I am using is generated from the HiRISE camera onboard the Mars Reconnaissance Orbiter,” Adrian told me. “The elevation data has a spatial resolution of 1 meter and the image data has a spatial resolution of 25 centimeters. There is no vertical exaggeration in any of the videos.”

Also, Adrian has experimented with You Tube’s stereoscopic 3-D player, providing a 3-D experience of flying through Candor Chasma. IMAX, watchout! You’ve got competition!

So hang on while you watch these incredible videos! See more below, and also Adrian shared with me a little about his software and how he creates these flyover videos.
Continue reading “Amazing Mars Flyover Videos Keep Getting Better and Better”

Speed of Gravity

Einstein and Relativity
Albert Einstein

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What is the speed of gravity? It’s 299,792,458 m/s. Seem familiar? Yep, it’s the speed of light (in a vacuum)!

How do we know that that’s the speed of gravity? Not by direct measurement, yet, but by the great success of Einstein’s theory of general relativity (GR).

In general, because it is so successful, and because the speed of gravity in GR is the same as the speed of light, we can say we know how fast gravity propagates.

In particular, observations of the Hulse-Taylor binary pulsar (and other binary pulsars) show the mutual orbit is decaying (the stars are slowly spiraling in, and will one day collide). The rate of decay is exactly as predicted by GR, and is due to the system radiating gravitational waves. The rate at which the system is losing energy tells us how fast that gravitational wave radiation is travelling … and it’s c, the speed of light, to within 1%!

Working out how gravity, as geometry in GR, makes planets in our solar system orbit the Sun is somewhat tricky, and misunderstanding of the details is what’s behind an erroneous claim you might come across on many websites (that the speed of gravity is many millions of times c, or even infinite).

A very long baseline radio interferometric observation of a quasar as it passed near Jupiter, in 2002, lead two researchers to claim to have directly measured the speed of gravity (they found it to be c, plus or minus about 20%). However, this claim is controversial, with several GR experts claiming the analysis contains subtle flaws, and that what was actually measured is the speed of light. The method Fomalont and Kopeikin used might allow a direct estimate of the speed of gravity to be made in future, in the view of their critics, with big improvements in precision.

More to explore: Speed of Gravity (NASA), What is the speed of gravity? (Cornell University), and Does Gravity Travel at the Speed of Light? (University of California Riverside).

Gravity Moves at the Speed of Light is an interesting Universe Today story on the speed of gravity; Warp Drives Probably Impossible After All is a very different take!

And check out the Astronomy Cast September 18th, 2008 Questions Show episode for more on the speed of gravity.

Sources:
Nobel Prize Press Release
Living Reviews in Relativity
UC-Riverside
NASA
Cornell Astronomy