Researchers Seeing Red on Ocean Health

The MODIS instrument on NASA’s Aqua satellite compiled this global view of the amount of fluorescent light emitted by phytoplankton in the ocean. Credit: Oregon State University

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With the help of an orbiting satellite, researchers have conducted the first global analysis of the health and productivity of ocean plants. Using the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite, scientists have for the first time measured remotely the amount of fluorescent red light emitted by ocean phytoplankton and assess how efficiently the microscopic plants are turning sunlight and nutrients into food through photosynthesis. Now that they have their first data, this method should allow scientists to effectively keep an eye on the health of our oceans. So what did they find out so far?

Over the past two decades, scientists have employed various satellite sensors to measure the amount and distribution of the green pigment chlorophyll, an indicator of the amount of plant life in the ocean. But with MODIS, “red-light fluorescence” has been observed over the open ocean.

“Chlorophyll gives us a picture of how much phytoplankton is present,” said Scott Doney, a marine chemist from the Woods Hole Oceanographic Institution and a co-author of the paper. “Fluorescence provides insight into how well they are functioning in the ecosystem.”

Phytoplankton -- such as this colony of chaetoceros socialis -- naturally give off fluorescent light as they dissipate excess solar energy that they cannot consume through photosynthesis. Credit: Maria Vernet, Scripps Institution of Oceanography
Phytoplankton -- such as this colony of chaetoceros socialis -- naturally give off fluorescent light as they dissipate excess solar energy that they cannot consume through photosynthesis. Credit: Maria Vernet, Scripps Institution of Oceanography

Red-light fluorescence reveals insights about the physiology of marine plants and the efficiency of photosynthesis, as different parts of the plant’s energy-harnessing machinery are activated based on the amount of light and nutrients available. For instance, the amount of fluorescence increases when phytoplankton are under stress from a lack of iron, a critical nutrient in seawater. When the water is iron-poor, phytoplankton emit more solar energy as fluorescence than when iron is sufficient.

The fluorescence data from MODIS gives scientists a tool that enables research to reveal where waters are iron-enriched or iron-limited, and to observe how changes in iron influence plankton. The iron needed for plant growth reaches the sea surface on winds blowing dust from deserts and other arid areas, and from upwelling currents near river plumes and islands.

The new analysis of MODIS data has allowed the research team to detect new regions of the ocean affected by iron deposition and depletion. The Indian Ocean was a particular surprise, as large portions of the ocean were seen to “light up” seasonally with changes in monsoon winds. In the summer, fall, and winter – particularly summer – significant southwesterly winds stir up ocean currents and bring more nutrients up from the depths for the phytoplankton. At the same time, the amount of iron-rich dust delivered by winds is reduced.

This data-based map shows iron dust deposition on the oceans in spring 2004. Areas with low dust deposition have high fluorescence yields. Credit: NASA's Scientific Visualization Studio
This data-based map shows iron dust deposition on the oceans in spring 2004. Areas with low dust deposition have high fluorescence yields. Credit: NASA's Scientific Visualization Studio

“On time-scales of weeks to months, we can use this data to track plankton responses to iron inputs from dust storms and the transport of iron-rich water from islands and continents,” said Doney. “Over years to decades, we can also detect long-term trends in climate change and other human perturbations to the ocean.”

Climate change could mean stronger winds pick up more dust and blow it to sea, or less intense winds leaving waters dust-free. Some regions will become drier and others wetter, changing the regions where dusty soils accumulate and get swept up into the air. Phytoplankton will reflect and react to these global changes.

Single-celled phytoplankton fuel nearly all ocean ecosystems, serving as the most basic food source for marine animals from zooplankton to fish to shellfish. In fact, phytoplankton account for half of all photosynthetic activity on Earth. The health of these marine plants affects commercial fisheries, the amount of carbon dioxide the ocean can absorb, and how the ocean responds to climate change.

“This is the first direct measurement of the health of the phytoplankton in the ocean,” said Michael Behrenfeld, a biologist who specializes in marine plants at the Oregon State University in Corvallis, Ore. “We have an important new tool for observing changes in phytoplankton every week, all over the planet.”

Source: NASA

Astrometry Finally Finds an Exoplanet

This artist's concept shows the smallest star known to host a planet. Image credit: NASA/JPL-Caltech

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Using the method of astrometry to find planets orbiting other stars has been around for 50 years, and until now it hasn’t bagged a single exoplanet. But finally, astronomers found a Jupiter-sized planet , called VB 10b, using this method. Astrometry is difficult and requires very precise measurements over long periods of time. So why did they keep trying for so long? “This method is optimal for finding solar-system configurations like ours that might harbor other Earths,” said astronomer Steven Pravdo of JPL. “We found a Jupiter-like planet at around the same relative place as our Jupiter, only around a much smaller star. It’s possible this star also has inner rocky planets. And since more than seven out of 10 stars are small like this one, this could mean planets are more common than we thought.”

The finding confirms that astrometry could be a powerful planet-hunting technique for both ground- and space-based telescopes. For example, a similar technique would be used by SIM Lite, a NASA concept for a space-based mission that is currently being explored.

The newfound exoplanet is about 20 light-years away in the constellation Aquila. It is a gas giant, with a mass six times that of Jupiter’s, and an orbit far enough away from its star to be labeled a “cold Jupiter” similar to our own. In reality, the planet’s own internal heat would give it an Earth-like temperature.

The planet’s star, called VB 10, is tiny. It is what’s known as an M-dwarf and is only one-twelfth the mass of our sun, just barely big enough to fuse atoms at its core and shine with starlight. For years, VB 10 was the smallest star known — now it has a new title: the smallest star known to host a planet. In fact, though the star is more massive than the newfound planet, the two bodies would have a similar girth.

Because the star is so small, its planetary system would be a miniature, scaled-down version of our own. For example, VB 10b, though considered a cold Jupiter, is located about as far from its star as Mercury is from the sun. Any rocky Earth-size planets that might happen to be in the neighborhood would lie even closer in.

“Some other exoplanets around larger M-dwarf stars are also similar to our Jupiter, making the stars fertile ground for future Earth searches,” said Stuart Shaklan, Pravdo’s co-author and the SIM Lite instrument scientist at JPL. “Astrometry is best suited to find cold Jupiters around all kinds of stars, and thus to find more planetary systems arranged like our home.”

Two to six times a year, for the past 12 years, Pravdo and Shaklan have bolted their Stellar Planet Survey instrument onto Palomar’s five-meter Hale telescope to search for planets. The instrument, which has a 16-megapixel charge-coupled device, or CCD, can detect very minute changes in the positions of stars. The VB 10b planet, for instance, causes its star to wobble a small fraction of a degree. Detecting this wobble is equivalent to measuring the width of a human hair from about three kilometers away.

Other ground-based planet-hunting techniques in wide use include radial velocity and the transit method. Like astrometry, radial velocity detects the wobble of a star, but it measures Doppler shifts in the star’s light caused by motion toward and away from us. The transit method looks for dips in a star’s brightness as orbiting planets pass by and block the light. NASA’s space-based Kepler mission, which began searching for planets on May 12, will use the transit method to look for Earth-like worlds around stars similar to the sun.

“This is an exciting discovery because it shows that planets can be found around extremely light-weight stars,” said Wesley Traub, the chief scientist for NASA’s Exoplanet Exploration Program at JPL. “This is a hint that nature likes to form planets, even around stars very different from the sun.”

Source: JPL

We All Need to Chill Out About Flight Tests

Artist concept of the Ares 1-X launch. Credit: NASA

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At a session today from the International Space Development Conference going in Orlando, Florida, the CEO of the commercial space company XCOR Aerospace had a few suggestions for all the eager space enthusiasts out there concerning test flights. In so many words Jeff Greason said everyone needs to chill out about the results from initial test flights. Of course, he was talking about all the test flights taking place with commercial space endeavors, but with the Ares 1-X getting ready to head to the launch pad for its first flight test, scheduled for August, perhaps we all need heed Greason’s advice and let the experts do their jobs.

Greason said in the past when they first started testing their early designs, “no one knew where Mojave was, we could test all sorts of strange things, and people would not be Twittering and blogging about what we did every day. But now it’s going on under a glare of publicity.”

Jeff Greason.  Credit:  XCOR
Jeff Greason. Credit: XCOR

While he appreciates the interest everyone is showing in the nascent commercial spaceflight industry and how people are watching with great enthusiasm and consuming every scrap of news, he is not exactly thrilled with tone of some of the commentary on what is being said on commercial flight tests.

“It’s called flight test for a reason,” Greason said. “You find problems, you always do. Any airplane you’ve ever ridden on had problems turn up on flight test program. Some of the most successful aircraft programs in history had a ridiculous number of problems show up in the flight test program. There is no correlation whatsoever between whether you or not you have problem in the flight test program and how good the finished product is. But there is a huge correlation whether you fix the problems you find in flight tests. ”

Greason said it isn’t helpful for journalists and the public to jump on every glitch and issue that comes up in every mission and say the sky is falling. “Just wait until flight tests to finish and by then there should be an answer. I see lot of blog posts three minutes after a flight test, saying the sky is falling. Stuff happens. So, I have a plea for the knowledgeable people out there: When you’re neighbor says ‘The sky is falling,’ tell them, ‘No, it’s just flight tests.”

Greason said flight tests are designed to find the problems and allow the engineers to fix the problems. But they take time. “That’s why I or anyone else never commits to how long flight tests lasts. Flight tests take as long as it going to take. When you fix the problems, that’s the end of the flight test program.”

Greason said he knows everyone is enthused because they want to see the missions happen, but every vehicle is a “new beast with their own design issues.”

More information on how XCOR designs and tests their vehicles, see this article from TimeCompression.com.

More information about the upcoming tests of the Arex 1-X.

Kid’s Astronomy: Of Kings and Queens and Royal Things…

The month of May is a fine time for flowers and colors – and even getting married! There once was an old tradition where children took ribbons and ‘danced around the Maypole’ in circles, weaving patterns around a central focal point. Before the month is over, why not celebrate the flowers and the dance of the stars around the northern pole as well? Let’s take another look at a constellation that’s becoming very visible at this time of year as we visit “Kings and Queens and Royal Things”…

492px-cepheus_constellation_mapRight now, as evening begins, the constellation of Cepheus is directly below Polaris for the northern hemisphere. As the sky darkens, this collection of five moderately bright stars will slowly turn counter-clockwise around Polaris… moving first seeming eastward, only to rise high above the pole star during the late hours of the night and begin moving towards the west as the Sun rises. While you are looking for a place where you can see the northern horizon well, listen to the wind and you’ll hear the voice of of the night. It has a story for you…

cepheusurania“As legend tells it, there once was a king of ancient Aethiopia named Cepheus – whose Queen was the beautiful Cassiopeia. They had many children together and one of Cassiopeia’s favorite places was the royal garden. Now, Cepheus loved to please his wife, so in this garden he contructed her a temple with a pointed roof where she and the children could spend their days among the many flowers. Cassiopeia’s favorite bloom was the iris, and to this day you can still find the “Iris Nebula”, (NGC 7023) blooming nearby.”

iris_wood

714px-erakis_garnet_sidus“Over the years Cepheus and Cassiopeia had many children together and take their place among the stars. When their strong sons would go out hunting, Cassiopeia was said to have lighted a candle in the window the the garden temple to lead them home on a dark night. To this very day, its deep red glow can be seen as Mu Cephi, Herschel’s Garnet Star.”

cassiopeia_1_thTime passed and Cassiopeia gave birth to a daughter – Andromeda. So beautiful was the baby girl, that Cassiopeia would sit in her chair under a palm tree on the west side of the garden temple where she could show her daughter’s loveliness to the gods. Zeus thought Andromeda was beautiful as well, and so he bestowed upon her the “Little Cloud” we now know as the Andromeda Galaxy.

androa

However, Cassiopeia was far too proud of her daughter and she boasted once too often on her good looks – proclaiming her to be even more beautiful than Zeus’ wife, Hera. This did not sit well with the Queen of the gods, so she demanded that Andromeda be sacrificed to Cetus, the Sea Monster – or marry her monster son, Calibos.

In order to save her daughter, Cassiopeia called upon one of Zeus’ mortal sons, Perseus to save her… But first Perseus had to win his winged horse, Pegasus, and defeat the Medusa. In order to gain his opportunity, Perseus had to answer a riddle. What is joined together but has no end?”

doubleclusterThe answer was the double pearl ring worn by Calibos, and when Pereus retrieved the ring, the gods put it up in the sky where it remains as the fine double star cluster, NGC 869 and 884. Perseus then flew away on Pegasus to defeat the Medusa, and the gods placed her head in the sky. To this day, you can still see her eye – Algol – changing brightness rapidly and waiting to turn unwary watchers, and Sea Monsters into stone.”

So go out, before the Moon captures the sky in the nights to come and hides the faint stars. Are there any iris in bloom where you are? Can you find the Royal House of Cepheus? Watch as the night moves and see how it turns around the pole star, just like children dancing around a maypole. Did you know that for each night that passes, our sky progress by six minutes? For example, when you locate Cepheus, make note of the time you first spotted it and its position. Now, look again an hour later. This is where you will find Cepheus 10 days from now at the time you first located it! Check Cepheus’ position 3 hours later and this is where it will appear a month from now at your initial time.

Isn’t SkyWatching wonderful?!

Many thanks to Torsten Bronger for the Cepheus constellation map, Uranometria historical Cepheus image, the “Iris Nebula” courtesy of Kent Wood, the “Garnet Star” courtesy of Francesco Malafarina, Cassiopeia courtesy of the University of Florida, M31 courtesy of Bill Schoening, Vanessa Harvey/REU program/NOAO/AURA/NSF and the “Double Cluster” courtesy of N.A.Sharp/NOAO/AURA/NSF. We thank you!

Anne is a Jolly Good Fellow!

Anne Minard

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Congrats to our very own Anne Minard who has been named one of five Ted Scripps Fellows in Environmental Journalism! Anne will be moving to Colorado to attend a nine-month academic program for professional journalists at the University of Colorado – Boulder. The Fellowship immerses journalists in classes and research about environmental issues to help them gain a better understanding of this topic, allowing them to cover the environment more effectively and enrich the public’s knowledge of this crucial subject. Anne will undoubtedly be busy with this new endeavor, but she hopes to keep her toe in the water here at Universe Today and share what she is learning. Congratulations Anne!

Universe Today is Hiring… a Researcher

Universe Today has a new position open for a researcher, and we were wondering if anyone out there on the Internets is interested in applying.

We’re looking for a researcher who can help support the blogging team to find space and astronomy news stories and aggregate them together. This means tracking thousands of RSS feeds, watching twitter feeds until your eyes bleed, and lurking through many many discussion forums. You’ll cosy up to NASA press officers and university researchers, deriving hidden meaning from their slightest innuendo. And then, like a mighty hunter, you’ll return to Universe Today HQ with a bag filled with breaking space news to keep the bloggers busy.

Are you the right person for the job? Ask yourself:

  • Do you love space and astronomy?
  • Do you love to make lists? Do you have lists of your lists?
  • Do you have a burning need to know everything? Does it annoy you that somebody out there might know something that you don’t?
  • Do you have a strong opinion of what’s interesting, and what’s boring. What’s cool and what’s lame?
  • Are your friends tired of you telling them cool stuff you’ve found out? (we’ll never tire of it)
  • Do you already have a fully stuffed RSS reader pulling in stories from all directions like a hungry black hole?

I’m thinking that this’ll be a part-time job – 20 hours/week? And you’ll be able to work from the comfort of your own home – in any country. Oh, and it doesn’t pay very well. But it does pay.

So, if that’s you, send in an email to [email protected] and tell me your story.

Fly Over the Potential Landing Sites For Next Mars Rover (Video)


Hang on and take a bird’s eye look at the four different proposed landing sites for the Mars Science Lab! At a briefing yesterday, Dr. Richard Zurek presented a flyover video of the potential landing sites for the next Mars rover, set to launch in 2011. The video is now available, and Zurek narrates the excellent flyover footage of each site, created by images taken by the HiRISE camera on the Mars Reconnaissance Orbiter. Enjoy the video, and find out a little more on each of the proposed sites below.
Continue reading “Fly Over the Potential Landing Sites For Next Mars Rover (Video)”

50th Anniversary of Historic Space Monkey Flight

Able in her capsule. Image Credit:NASA

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The image to the left is not a primate astronaut from “Planet of the Apes.” It is, in fact, a real space monkey. Today marks the 50th anniversary of the first flight into space of a living being that survived the expedition. On May 28th, 1959, one rhesus monkey, named Able, and one squirrel monkey named Miss Baker became the first “astronauts” to survive a return flight into space.

Though they were not the first animals launched into space, Able and Baker helped pave the way for human spaceflight by showing that animals can indeed survive the rigorous launch and return of a spacecraft. Their vital signs were monitored during the mission, giving scientists a better understanding of what stresses spaceflight puts on a living body.

Launched aboard a Jupiter AM-18 rocket, Able and Baker flew to a height of 360 miles and traveled 1700 miles from their launch site at the Eastern Space Missile Center at Cape Canaveral, Florida. Their capsule landed in the ocean, and was retrieved by a U.S. Navy vessel commanded by Joseph Guion.

Guion told NASA, “As soon as I picked it up out of the water, it was flying all over the place. The ship was rolling and the nose cone swung back and forth. And I was just hoping that nobody would get hurt…We still didn’t know if the monkeys were alive ‘cause we didn’t have the telemetry. And so one technician ran up to the back end of it and plugged in and he says, ‘They’re alive!’ So everybody went ‘Yay!’ And that’s when I could finally say, ‘Ah!’ Relax.”

The entire flight lasted about 15 minutes, and during nine minutes of that the two tiny astronauts experienced weightlessness. After the recovery of their capsule, the monkeys were allowed to relax in an air-conditioned room aboard the vessel, then escorted to Washington, D.C. for a press conference.

To see a video of Able and Miss Baker getting ready for flight, check out this video on Youtube: Able and Baker blast off, from Universal News 1959.

Able died, unfortunately, a few short days after the flight. She needed an operation to remove an infected medical electrode, and had an adverse reaction to the anesthetic. Miss Baker, however, survived another 25 years, living at the U.S. Space and Rocket Center in Huntsville, Ala. During the rest of her life, she would receive over 100 letters a day from children who read about her adventures in textbooks and wanted to say ‘Hello’.

Miss Baker’s contribution was far from forgotten at the time of her death, and at her funeral in 1984 the attendance was well over 300 people. She still has a grave marker (pictured below) in front of the Alabama Rocket Center memorializing her part in the history of spaceflight.

Miss Baker's memorial. Image Credit:DCmemorials.com
Miss Baker's memorial. Image Credit:DCmemorials.com

Able and Baker were preceded by a long line of unsuccessful attempts by the U.S. to launch primates into space. The first attempt was Albert, who flew to 39 miles (63km) on June 11, 1948 aboard a V2 rocket, but died of suffocation during the flight. Albert II actually made it into space (above 62 miles/100km) on June 14th, 1949, but died upon the impact of his re-entry flight.

Primates were far from the first living things sent intentionally into space. That distinction belongs to a member of a different part of the animal kingdom: fruit flies. Fruit flies were sent into space, along with a sample of corn seeds, in 1947 to test the effects of radiation at high altitude.

So, to celebrate this historic event in spaceflight, it may be fitting to eat a banana for breakfast (or lunch, or dinner, or all three).

Source: NPR, NASA

China Looking Towards Manned Lunar Landing

Artist concept of a Chinese lunar mission. Credit: Xinhua

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A Chinese space scientist said that his country is considering the feasibility of a manned lunar landing mission sometime between 2025 and 2030. China is also planning a sample return mission to the Moon by 2017, said Ye Peijian, chief designer of the China’s Chang’e Project. “Through the development of lunar probes, we have made constant progress of the ability to explore the outer space,” Ye was quoted as saying by the China News Service.

Chang’e -1 launched successfully in 2007 and orbited the Moon for 16 months before conducting a controlled impact on the Moon’s surface earlier this year. The satellite mapped and created three-dimensional images of the lunar surface. Several performance tests were carried out while Chang’e-1 was in orbit to give engineers experience in orbit adjustment, and to test the spacecraft’s capability.

According to Ye, China will launch the second lunar probe Chang’e-2 in 2010 which will conduct research at a 100-kilometer-high moon orbit as the preparation for a soft landing by using variable thrusters with the Chang’e-3, which will include a lunar rover, currently in development.

The rover will work on the moon’s surface for three months, Ye said, adding scientists have decided to adopt isotope generator to provide energy for the rover when it is in lunar nights when temperatures drop to 200 Celsius degrees below zero.

The sample return mission will be able to gather two kilograms of lunar samples and launch a return capsule from the Moon back to Earth.

All of these incremental steps would lead to a human mission to the moon, likely to be similar to NASA’s Apollo missions. During the timeframe China is hoping to bring humans to the moon, the US is also hoping to return to the lunar surface with long duration missions with the new Constellation program.

Source: People’s Daily Online

Basalt

Lava fountain in Hawaii.

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Basalt is a hard, black volcanic rock with less than 52% silica. Because of this low silica content, basalt has a low viscosity (thickness), and so it can flow for long distances after erupting from a volcano. During an eruption, a basalt lava flow can easily move more than 20 km away from a vent. Basalt is the most common rock type in the Earth’s crust. In fact, most of the ocean floor is made up of basalt.

Basalt is made up of dark colored materials like pyroxene and olivine, but it also contains lighter minerals like feldspar and quartz. These crystals form because the lava cools slowly after erupting out of a volcano. Although a lava flow might look cool shortly after an eruption, it might take months or even years to cool all the way through. The crystals are bigger in the middle of a cooled lava flow because that part had longer to cool. If a lava flow cools quickly, like when it falls into a lake or ocean, it becomes a glass-like rock called obsidian. This is because the crystals in the rock don’t have time to form.

Shield volcanoes are made up entirely of basalt lava eruptions. A good example of this are the volcanoes Mauna Loa and Mauna Kea on the Big Island of Hawaii. Over hundreds of thousands of years, they have built up tall volcanoes that are extremely wide because of the fast flowing basalt lava.

Geologists have found large outpourings of lava covering hundreds of kilometers of land called flood basalt. The largest of these is known as the Siberian Traps in northern Russia. This is a region of 1.5 million square kilometers covered by basalt.

We have written many articles about volcanoes for Universe Today. Here’s an article about obsidian, and here’s an article about different types of lava.

Want more resources on the Earth? Here’s a link to NASA’s Human Spaceflight page, and here’s NASA’s Visible Earth.

We have also recorded an episode of Astronomy Cast about Earth, as part of our tour through the Solar System – Episode 51: Earth.