QUEST Community Science Blog

Mockup of Phoenix (top) and ‘Robinson Crusoe on Mars’
(bottom)—both set in Death Valley National Park…
Credit: NASA (top), Paramount Pictures (bottom)It’s that time of the Martian year again: when a flying saucer from Earth appears in the skies of Mars. Imagine if there actually were Martians up there: what’s science fiction here on Earth would pass for reality on the Red Planet—and a routine occurrence at that!

This time the flavor of the day is the Phoenix Lander, courtesy of NASA, scheduled to land on May 25th at about 4:38 PM PDT. We’ll be watching live NASA coverage of the landing at Chabot Space & Science Center that afternoon, if you’d care to join us…

Following somewhat in the footsteps of the Viking landers of the 1970s, Phoenix’s primary mission is to look for evidence of life, or at least the chemical conditions that might be suitable for life to exist. The two Viking landers carried small chemical laboratories that analyzed soil samples scooped up from the surface, as does Phoenix.

While its mission parallels that of Viking, one big difference from Phoenix is its destination: the Northern Polar Ice Cap of Mars. The Vikings landed much farther south in the mid latitudes. Phoenix is targeting the ices of Mars’ arctic region.

Growing up, one of my favorite sci-fi films was Robinson Crusoe on Mars. Made in 1964, the same year that Mariner 4, the first space probe to Mars, was launched, RCOM made a descent stab at imagining what it was like. So what if the main character walked around in apparent t-shirt weather and with sufficient atmospheric pressure to keep his blood from boilin–he still wore a respirator that doled out oxygen from an ever-dwindling supply tank, a nod to Mars’ thin atmosphere.

A couple of other things our astronaut Robinson Crusoe found on that fictional Mars that we are now looking for on the real one: liquid water and life…Our hero found small caches of water (with the help of a monkey) in grottos between the rocks, and, lo and behold, living in that water was a vine-like life form with edible fruit or tubers. He even took a foot-trek, along with his guy Friday, to the polar ice cap…

(I also loved the film because some of its “Martian terrain” scenes were shot in my favorite spot on Earth, Death Valley…)

Though evidence of past liquid water action seems to be all about the planet, Phoenix certainly won’t find any brooks or pools or grottos of spring water, owing at least in part to the frigid arctic region it will set feet on–an arctic zone on a world where the warmest temperatures in the tropics might reach levels of the coldest climates on Earth. What’s important about landing on Mars’ ice cap is that Phoenix is almost certain to dig up some water–albeit frozen.

And it is the chemical compounds either locked up in that ice or preserved by its proximity that Phoenix is interested in. (Similarly, climatologists on Earth study ice cores from Antarctica to analyze the trapped and preserved gases of Earth’s atmosphere of past millennia.)

We wish Phoenix a happy landing, and look forward to the first images and discoveries from the Martian North Pole. And I’m fairly confident the epic polar adventure ahead won’t resemble in the least another “great” film of 1964: Santa Claus Conquers the Martians….

Benjamin Burress is a staff astronomer at The Chabot Space & Science Center in Oakland, CA.

Infrared image of a zebra from the London Zoo.
Credit: Steve Lowe

Right now I am very excited about the possibility of working on a new small telescope in southern Utah. This telescope was funded by a private donation and will be run by the University of Utah. We even found a mountain top in the middle of nowhere that this telescope will call home.

Why this particular mountain? There are essentially three reasons:

It’s dark
It’s clear
It doesn’t make the stars twinkle

The first two reasons are so obvious that I am almost embarrassed. The last reason is not quite so intuitive. What makes a star twinkle and why do we care? This goes back to a post I made a few months ago.

The basic idea here is that the churning atmosphere blurs your astronomical image. Local geography and weather patterns can either mitigate or exaggerate this effect. It is difficult to predict and many measurements need to be done to determine what is actually happening. Cameras were placed all around southern Utah on various mountain tops to observe the North Star over the course of the year. The mountain top that produced the highest resolution image of the star won the competition. That was Frisco Peak.

The telescope that will be placed on Frisco Peak was built by a very specialized company. This is quite rare–more typical are either large custom-made telescopes or small amateur telescopes. This telescope falls in the middle. It is bought off the shelf but is far superior to the commercially made amateur telescopes.

We are now discussing plans for this telescope, like the type of cameras that should be used. There is a strong interest in building an infrared camera. This allows us to see through large clouds of dust and allows us to see very distant galaxies.

Like most people, I am much more experienced with cameras in the visible spectrum. I work on CCDs in Berkeley and have barely used anything in the infrared. CCDs are made of silicon which is sensitive to light that can be seen with the naked eye (plus a little more red than what can be seen).

However, there is a lot of information in the sky that is too red to be seen with the naked eye and too red to be detected with a silicon detector. New materials are required for detectors in this wavelength range. One of the major new materials for infrared detectors is a blend of mercury, cadmium and telluride, usually called Mer-Cad-Tell in the astro community. The wavelength range of the detector can be tuned by changing the amount of mercury in the blend.

Clearly, a lot of the legwork has been done for this new telescope. We have the funding, we have a vendor, and we have a location. Now all that’s left is to prioritize our science goals and to figure out how to get our hands on some mer-cad-tell.

Kyle S. Dawson is engaged in post-doctorate studies of distant supernovae and development of a proposed space-based telescope at Lawrence Berkeley National Laboratory.

Nobody likes moving. The packing, taping, lifting, shipping… it can be major hassle. But nobody’s experience compares to what’s going on at the California Academy of Sciences. They’re moving to their new 400,000 square-foot building in Golden Gate Park after three years in downtown San Francisco. But they’ve got a lot more to move than most people. Try 38,000 live animals and 20 million scientific specimens.

From fossils and gemstones to bird eggs and a stuffed Kodiak bear, it takes a lot of creativity to pack their collection. Everything seems to have special requirements. Their fish collection is made up of 200,000 jars - all filled with alcohol. And since it’s a flammable liquid, they’ll need a licensed hazmat driver to take it across town.

The live animals take extra care, of course. In this story, we followed the move of three black tip reef sharks. They hadn’t been fed in a few days (so they wouldn’t make any, um, deposits in their holding tank) and they weren’t easy for the staff to catch, but they made it safely to their new exhibit. Even the largest of the three, F3 as she’s known, made it ok, despite being a little groggy at first from too much oxygen.

As curator Bart Shepherd put it, their new Philippine Coral Reef Exhibit is a giant science experiment. The water for the 200,000 gallon tank comes straight from the Pacific Ocean through a four mile pipe. But most impressively, the Academy has been growing coral just for the exhibit. Just managing the water chemistry alone has been a major project, but now several dozen colonies of coral are happily planted in their new home.

Make sure to check out the audio slide show for this story to see how the new building is shaping up. And check out a few of the posts from QUEST science blogger Cat Aboudara, who is an Academy staff member, for more details on what it takes (here, here and here).

Watch the “Moving Day” audio slide show online, as well as find additional links and resources.

Lauren Sommer is an Associate Media Producer for QUEST.

A “penguin suit” doesn’t just refer to a tuxedo anymore.

Why does Pierre, the Academy’s 25-year-old penguin
need a wetsuit?Thanks to an innovative treatment at the California Academy of Sciences. Pierre, the Academy’s 25-year-old penguin was recently fitted with a wetsuit! Pierre’s feathers were thinning and not growing back. Because penguins rely on their feathers for warmth, Pierre was often shivering and uncomfortable without the protection of his feathers. When medical tests concluded there was no medical reason for the feather loss and more conventional treatments proved unsuccessful, senior aquatic biologist & penguin handler, Pam Schaller came up with a more creative approach to keep Pierre warm.

Pam was very familiar with the warmth of wetsuits. She then mused why couldn’t a wetsuit be designed for a penguin? She approached Academy veterinarian, Freeland Dunker with her left field idea. At first, he was dubious but after talking with Pam, he agreed it was worth a try as long as the wetsuit was fitted to insure it did more good than harm. In other words, as long as the wetsuit was fitted not to impede movement or cause rashes, it was worth a shot. Pam knew the best person to design a custom wetsuit would be Celeste Argel, the Early Childhood Specialist at the Academy, who is an excellent and creative seamstress. Celeste was asked to collaborate with Pam to develop and fit a wetsuit just Pierre’s size.

But how do you go about designing a penguin wetsuit? The answer seems to be trial and error. Celeste sat down with me and went over the details about the unusual experience. The process from idea to creation required a great deal of patience and re-fitting.

Celeste, Pam and Pierre met several times in order to customize dimensions. The first fitting consisted of Pam restraining Pierre in order for Celeste to take measurements. From the start, Celeste marveled at the strength of Pierre. “From far away,” she commented, “penguins just look so cute and cuddly but being up close gave me an appreciation for just how strong penguins really are.” With measurements in hand, Celeste drafted up a pattern for the wetsuit and created the first prototype from white cotton bed linens.

On the second fitting, Celeste was faced with a new challenge - getting Pierre’s flippers through the armhole. Pam wanted to keep the armholes as small as possible to maximize warmth. In doing so, Pierre’s flippers had to be bent at the joint and folded in upon themselves in order to thread them though the armholes. While Pam again restrained Pierre, Celeste applied pressure at the joint to fold his wings. “It was amazing and scary to fold up Pierre’s flipper. I wanted to make sure I wasn’t hurting him but to fold his flipper required a bit of pressure at the joint,” Celeste related. With the prototype on, Celeste was able to use a marker and note where the suit had to be taken in or taken out to make Pierre more comfortable. And then again, it was back to the drawing board.

A few more fittings took place to streamline the suit and to ensure that Pierre’s flippers had full mobility. Then Velcro was added to the back of the suit. Pierre was let loose in the penguin enclosure to see how he moved. Both Celeste and Pam sat down to watch his movements and observed where the fabric was bunching. Pierre seemed to be adjusting to his suit quite well but the other penguins, new to a mostly white Pierre, started poking and prodding to investigate the newly adorned bird. Because of the interest from the other birds, the session in the suit only lasted a few minutes. Celeste changed the color of the prototype to a dark brown to see if the other penguins would respond differently and they did. They accepted Pierre with a dark physique. More sessions in the new prototype followed and when Pierre jumped into the water and swam around with the suit on, Celeste and Pam knew it was time for the neoprene fitting.

Celeste conducted research to see how neoprene would act differently than cotton. From her research, she concluded that the whole suit would have to be taken in at least an inch because of the give of the material. However, Celeste didn’t have a machine to sew neoprene effectively so Pam asked Oceanic Worldwide, who supplied wetsuits to the human staff at the Academy, to manufacture a neoprene suit. Pam delivered the working prototype and the patterns to Oceanic who agreed to donate their time and materials. “We were really excited to do it,” said Teo Tertel, company marketing specialist. “We heard most of these penguins only live to 20, and our little buddy there was already 25. Anything we could do to help them, we were all for it.”

When the suit from Worldwide was delivered, it still wasn’t quite ready. The neoprene suit fit differently than expected and had to be re-fitted all over again. However neoprene can be glued instead of sewn so it was a matter of trying the suit on Pierre, marking where it didn’t fit snugly and adjusting. “I would walk behind him and look at where there were any gaps, and cut and refit and cut and refit until it looked like it was extremely streamlined,” Pam remarked on the final alterations. There were hiccups with a penguin being in a wetsuit for the first time and being curious about the Velcro and tabs. So nothing was left unaltered for Pierre’s comfort and mobility.

With all the alterations finally done, a final set of patterns was delivered to Oceanic Worldwide and they again donated their time to manufacture the final wetsuit for Pierre. All the hard work paid off for all involved when Pierre became warm again. It was a huge bonus when he also started to gain weight and his feathers began to grow back. The goal of designing the wetsuit for Pierre was to keep him comfortable and warm and the custom suit worked much better than expected. Having Pierre happy and healthy without the further need of the wetsuit was a perfect outcome for a very unusual treatment.

Cat Aboudara is the Special Projects Manager at California Academy of Sciences and works in the public programs division. The Academy is a wonderful fit for her because of her curiosity about the natural world and her experience in working with native California wildlife.

What does our use of bottled water say about us? View our 2-minute TV short “Future History: Plastic Water Bottles” to take a look from the perspective of an anthropologist from the distant future, and the take our poll below:

Josh Rosen is Series Producer for QUEST on KQED Television.

In 1968, John Dobson started the San Francisco Sidewalk Astronomers with the help of two boys who loved astronomy but couldn’t join an amateur astronomy club in the city because they were too young. So the trio created their own club, carting two homemade telescopes onto Jackson and Broderick Streets and inviting curious passersby to take a look at the craters of the moon, the rings of Saturn, the banded clouds of Jupiter.

Forty years later, the San Francisco Sidewalk Astronomers is still going strong, boasting a web site replete with a monthly star chart, specific for San Francisco, a calendar of monthly amateur astronomy events, a helpful “cheat sheet” of astronomical facts and answers to questions that routinely come up if you set up a telescope on your neighborhood sidewalk, and where to go if you want to borrow, build or donate a telescope.

Another great resource for the budding SF amateur astronomer is the Randall Museum, which hosts star parties, lectures by amateur and professional astronomers and classes for making your own Dobsonian telescope from scratch. The free public lectures at the Randall Museum take place on the third Wednesday of each month, sponsored by the San Francisco Amateur Astronomers.

Since 1952, the San Francisco Amateur Astronomers have been an invaluable resource for stargazers to learn about the choicest observing sites throughout the Bay Area, monthly star parties and make contact with a community of like-minded folks. Be sure to also check out their astrophotography web page, where they have uploaded photos and even videos shot with their telescopes of galaxies, comets, moons, planets and nebulae.

If you can’t get enough of amateur astronomy clubs in the Bay Area, check out the Astronomical Society of the Pacific and the Astronomical Association of Northern California. The Astronomical Society of the Pacific, founded in the 19th century, has members from 70 countries and claims to be the largest astronomy society in the world. It also boasts educational outreach programs, such as Astronomy from the Ground Up, a National Science Foundation-funded program that helps informal science educators such as docents and volunteers by giving them the tools and training to more effectively communicate astronomy information to the public.

If you should need to buy equipment or talk with some very knowledgeable folks about the right telescope, accessories or CCD digital camera to begin your foray into astrophotography, check out Scope City, a retailer in San Francisco specializing in telescopes and binoculars.

Watch the “Amateur Astonomers” TV Story online, as well as find additional links and resources.


Sheraz Sadiq is an Associate Producer for QUEST on KQED Television.

Artist concept of a geyser erupting on Enceladus.
Credit: David Seal.Back when I was young…okay, a previous generation might have ended that sentence with, “…I’d walk forty miles through the snow to get to school…” But I’m not exaggerating when I say, when I was young we knew next to nothing about faraway places in the Solar System…such as the moons of Saturn.

A layer of the veil around Saturn’s moons was removed when Pioneer 11 and Voyagers 1 and 2 made flybys of Saturn in the ’70s and ’80s. The Saturnian moons, it appeared, were not the lumps of rock and dust that Earth’s own Moon is made of, but objects containing no small amount of water ice. Not terribly surprising, considering the low temperatures of the outer solar system where ice-rich comets roam.

Visions of frozen alien landscapes, replete with icicles and ice cliffs and ice fields and ice ice ice! were conjured in my imagination, and in artist depictions of majestic ringed Saturn seen from moons like Rhea or Dione or Enceladus.

Four years ago, Saturn’s first permanent visitor from Earth–the Cassini spacecraft–arrived there, and since has been making extreme closeup examinations of Saturn, its rings, and its increasingly wondrous and beautiful moons. Cassini is almost literally ripping apart veil after veil of our ignorance of these little worlds.

Far from a contingent of enormous but simple snow cone balls, Cassini has shown us that some of Saturn’s moons are apparently alive with liquid motion. First, there were the surface “lakes” and “seas” on Titan, probably made of extremely cold liquid hydrocarbons like methane and ethane–the stuff that spouts out of the gas range in your kitchen. Lakes and seas and rolling waves of liquid natural gas are fine and dandy for an imagined shoreline scene–but take a dip in those “waters” and an actual water-based creature like you would freeze solid in seconds. Scenic, but not inviting for a swim…

But recent observations by Cassini have shown that Titan’s frigid unearthly lakes and Enceladus’ snowball exterior may just be additional veils that are now being lifted.

In March, Cassini flew within 30 miles of the surface of Enceladus and right through a plume of material venting into space from the moon’s interior—an enormous “geyser.” Earlier observations had sensed the presence of water in the plume, giving rise to speculation that liquid water in some form might exist beneath Enceladus’ surface—perhaps chambers of liquid heated by tidal stressing of the interior.

When Cassini flew through the plume, its chemical sensors “sniffed” more than just water in the stream, but a good deal of organic molecules as well…not unlike material found in comets, stuff left over from the formation of the Solar System that may have been the building blocks of life on Earth.

The other “water find” was that of a possible liquid ocean under the crust of Titan–similar perhaps to the deep liquid water ocean believed to exist under the surface of Jupiter’s moon Europa. Unexpected “drift” in the locations of landmarks on Titan’s surface is what suggests a liquid ocean–water with perhaps some ammonia–that the frozen crust may be floating on.

With all the liquid water and organic chemistry being revealed in the Saturn system (and elsewhere in the outer solar system), our imaginations can shift from the older standards of envisioning otherworldly landscapes of sculpted ice or even seascapes of liquid hydrocarbon lapping on shores of water ice sand, to something a little more, shall we say, “lively…”?

Benjamin Burress is a staff astronomer at The Chabot Space & Science Center in Oakland, CA.

Making Every Photon Count

Last week I went to a talk given by the leader of the Supernova Factory collaboration at LBNL. What is SN factory? This is an ambitious project to study supernovae like never before. I mentioned this project briefly in a previous post , now that they are so close to releasing their results I want to discuss it a bit more.

The main idea of this project is to study several hundred nearby supernovae using an instrument known as the Supernova Integral Field Spectrograph, or SNIFS. This type of instrument is essentially a blend between a traditional imaging camera and a spectrograph.

The resolution in an integral field spectrograph is defined in spaxels instead of the pixels that have become all too familiar with the advent of digital cameras. A spaxel is quite similar to a pixel, there aren’t nearly as many and each one carries at least a 1000 times as much information.

In your digital camera, the light passes through the lens and directly onto the CCD. Each pixel on the CCD counts the number of photons in the red, the blue, and the green. Typically, there are millions of pixels, each counting photons from a slightly different region of the subject of your photograph.

Now imagine that instead of just counting red, green, and blue, that each pixel counts the entire rainbow of light from your subject. Now you have a spaxel. In an intregral field unit, the light passes through an array of microlenses and prisms before landing on the detector. We would call each set of microlenses and prisms a spaxel. The resulting image carries information about every wavelength of light from every region of your target.

Spectrum of the first SN observed with SNIFSThe advantage to an integral field spectrograph like SNIFS is that you gain a lot more information than either an imager or spectrograph alone. With an integral field spectrograph you can basically identify and organize every photon that reaches the telescope.

Specifically designed to observe supernovae, SNIFS is being operated at the 88-inch telescope on Mauna Kea. Spaxels are quite expensive - this particular instrument has only 225. However, this is more than enough to observe the entirety of a galaxy, a supernova, and the background.

The members of the SN Factory have now observed over 100 SNe using this new camera. Last Thursday, I saw the data from the first 25 well-calibrated supernovae and was very impressed. The data showed the evolution of each supernova and the properties of the host galaxy in great detail. I’m sure the supernova community will be equally impressed when they first see these new results.

Kyle S. Dawson is engaged in post-doctorate studies of distant supernovae and development of a proposed space-based telescope at Lawrence Berkeley National Laboratory.

The camera has long been an invaluable tool of field researchers. For example, the initial identification of a new mammal species was initiated by a camera trap set up by Francesco Rovero of the Trento Museum of Natural Sciences in the Ndundulu Forest in Tanzania’s Udzungwa Mountains. Both Francesco Rovero and Galen Rathbun of the California Academy of Sciences followed this photographic proof toward the discovery of a new species of Giant Elephant Shrew - the grey-faced Sengi. Photographs allow researchers to view their surroundings in a more intimate way and extrapolate meaningful data. It can even lead to incredible discoveries.

The California Academy of Sciences is asking youth to get behind the camera to find discoveries in their backyard. On April 15, 2008, the Academy launched a photo contest for youth between the ages of 8 & 12 - “Through the Lens: California in your backyard”. Future photographers, researchers and scientists are right in our own backyard and the Academy is curious about what they are seeing in their surroundings. This contest will give youth a chance to have a researcher’s eye - to “get up close” and document what they observe.

The photographers with the “best eye” will have their work hung in a museum. The work of winning photographers will be exhibited as part of the Children’s Gallery at the Grand Re-opening of the California Academy of Sciences on September 27, 2008 and throughout the inaugural year. Winning photographers will also be awarded cash prizes.

It is up to the photographer how to convey the theme of this contest - “California in your backyard” and the Academy’s mission - to explore, explain and protect the natural world. All photographers entering the contest are encouraged to have lots of fun and be as creative as possible.

The deadline to submit photographs is May 26, 2008. Contest rules and submission instructions can be found at www.calacademy.org/contest. Aspiring and curious youth photographers are encouraged to submit work. It might be the catalyst to another great discovery!

Cat Aboudara is the Special Projects Manager at California Academy of Sciences and works in the public programs division. The Academy is a wonderful fit for her because of her curiosity about the natural world and her experience in working with native California wildlife.

Inside the National Ignition Facility. Lawrence Livermore National Lab is building the world’s largest laser. Actually, the National Ignition Facility won’t have only one laser beam. It will use 192 world-class lasers, all firing simultaneously. In a few billionths of a second about 500 trillion watts, which is nearly 1000 times the power generated in the entire US at any moment, will hit a target the size of a dime. The hope is that this will create enough heat and pressure to mimic the core of the sun and achieve a fusion ignition.

So in a nutshell, what is fusion? And how do lasers work? Why are you asking me? I was the kid who always struggled with math and would get hives on the eve of a high school science test.

Luckily, there are some darn good teachers out there and we were fortunate enough to feature one of them in our story. Richard Muller is a professor of physics at the University of California and has also become something of a web phenomenon. Thousands of “students” all over the world have viewed his lecture series titled “Physics for Future Presidents” on YouTube and Cal’s own website.

Muller designed this class to “stress conceptual understanding rather than math, with applications to current events.” As he told us, “imagine looking out on your classroom and picturing out there is the future president of the United States. What do you want that person to know?” What comes out is an explanation of the physics of energy, nuclear weapons, radioactivity, relativity and the universe– all explained in a way that the physics-challenged, like myself or maybe a future president, can understand.

Watch the “Super Laser at the National Ignition Facility” TV Story online, as well as find additional links and resources.

Chris Bauer is a Segment Producer for television on QUEST.