Plankton’s Glow Seen from Space

For the first time, scientists may now detect a phytoplankton bloom in its early stages by looking at its red “glow” under sunlight, due to the unique data from two NASA satellites. According to a study conducted in the Gulf of Mexico, this phenomenon can forewarn fishermen and swimmers about developing cases of red tides that occur within plumes of dark-colored runoff from river and wetlands, sometimes causing “black water” events.

Dark-colored river runoff includes nitrogen and phosphorus, which are used as fertilizers in agriculture. These nutrients cause blooms of marine algae called phytoplankton. During extremely large phytoplankton blooms where the algae is so concentrated the water may appear black, some phytoplankton die, sink to the ocean bottom and are eaten by bacteria. The bacteria consume the algae and deplete oxygen from the water that leads to fish kills.

Chuanmin Hu and Frank Muller-Karger, oceanographers at the College of Marine Science of University of South Florida, St. Petersburg, Fla., used fluorescence data from NASA’s Moderate Resolution Imaging Spectroradiometer (MODIS) instruments aboard both NASA’s Terra and Aqua satellites. MODIS detects the glow or phytoplankton fluorescence, from the plant’s chlorophyll. The human eye cannot detect the red fluorescence.

The ability to detect glowing areas of water helps researchers identify whether phytoplankton are present in large dark water patches that form off the coast of Florida. Without these data, it is impossible to differentiate phytoplankton blooms from plumes of dark river runoff that contain few individual phytoplankton cells.

Because colored dissolved organic matter that originates in rivers can absorb similar amounts of blue and green color signals as plants do, traditional satellites that simply measure ocean color cannot distinguish phytoplankton blooms within such patches.

Although satellites cannot directly measure nutrients in lakes, rivers, wetlands and oceans, remote sensing technology measure the quantities of plankton. Scientists can then calculate how much nutrient might be needed to grow those amounts of plankton.

Hu and others used this technique to study the nature and origin of a dark plume event in the fall of 2003 near Charlotte Harbor, off the south Florida coast. Moderate concentrations of one of Florida’s red tide species, were found from water samples.

“Our study traces the black water patches near the Florida Keys to some 200 kilometers (124 miles) away upstream,” said Hu. “These results suggest that the delicate Florida Keys ecosystem is connected to what happens on land and in two remote rivers, the Peace and Caloosahatchee, as they drain into the ocean. Extreme climate conditions, such as abnormally high rainfall in spring and summer 2003, may accelerate such connections,” he added.

These findings are based on scientific analyses of several things. Data used include satellite ocean color from MODIS and Sea-viewing Wide Field-of-view Sensor (SeaWiFS), and wind data from NASA’s QuikSCAT satellite. U.S. Geological Survey, National Oceanic and Atmospheric Administration (NOAA), Florida?s Fish and Wildlife Research Institute, and other organizations provided rain, river discharge, and field survey information.

By knowing which way the winds blow and the currents flow, Hu and colleagues can predict where black water may move.

Red tides occur every year off Florida and are known to cause fish kills, coral stress and mortality, and skin and respiratory problems in humans. Previous studies show that prolonged “black water” patches cause water quality degradation and may cause coral death. The use of remote sensing satellites provides effective means for monitoring and predicting such events.

The link between coastal runoff and black water events is an example of how land and ocean ecosystems are linked together. “Coastal and land managers over large areas need to work together, to alleviate more black water events from taking place in the future,” said Muller-Karger.

This study appeared in a recent issue of the American Geophysical Union’s Geophysical Research Letters. Coauthors of the article include Gabriel Vargo and Merrie Beth Neely from University of South Florida and Elizabeth Johns from NOAA’s Atlantic Oceanographic and Meteorological Laboratory.

NASA’s Science Directorate works to improve the lives of all humans through the exploration and study of Earth’s system, the solar system and the Universe.

Original Source: NASA News Release

What Impact Would Set the World on Fire?

Image credit: Josh O?Conner and wildlandfire.com
Scientists conclude that, 65 million years ago, a 10-kilometer-wide asteroid or comet slammed into what is now the Yucat?n peninsula, excavating the Chicxulub impact crater and setting into motion a chain of catastrophic events thought to precipitate the extinction of the dinosaurs and 75 percent of animal and plant life that existed in the late Cretaceous period.

“The impact of an asteroid or comet several kilometers across heaps environmental insult after insult on the world,” said Dr. Daniel Durda, a senior research scientist at Southwest Research Institute? (SwRI?). “One aspect of the devastation wrought by large impacts is the potential for global wildfires ignited by material ejected from the crater reentering the atmosphere in the hours after the impact.”

Large impacts can blast thousands of cubic kilometers of vaporized impactor and target sediments into the atmosphere and above, expanding into space and enveloping the entire planet. These high-energy, vapor-rich materials reenter the atmosphere and heat up air temperatures to the point that vegetation on the ground below can spontaneously burst into flame.

“In 2002, we investigated the Chicxulub impact event to examine the extent and distribution of fires it caused,” said Durda. This cosmic collision carved out a crater some 40 kilometers (25 miles) deep and 180 kilometers (112 miles) across at the boundary between two geologic periods, the Cretaceous, when the dinosaurs ruled the planet, and the Tertiary, when mammals took supremacy.

“We noted that fires appeared to be global, covering multiple continents, but did not cover the entire Earth,” Durda continued. “That suggested to us that the Chicxulub impact was probably near the threshold size event necessary for igniting global fires, and prompted us to ask ‘What scale of impact is necessary for igniting widespread fires?'”

In a new study, Durda and Dr. David Kring, an associate professor at the University of Arizona Lunar and Planetary Laboratory, published a theory for the ignition threshold for impact-generated fires in the August 20, 2004, issue of the Journal of Geophysical Research. Their research indicates that impacts resulting in craters at least 85 kilometers wide can produce continental-scale fires, while impact craters more than 135 kilometers wide are needed to cause global-scale fires.

To calculate the threshold size impact required for global ignition of various types of vegetation, Durda and Kring used two separate, but linked, numerical codes to calculate the global distribution of debris reentering the atmosphere and the kinetic energy deposited in the atmosphere by the material. The distribution of fires depends on projectile trajectories, the position of the impact relative to the geographic distribution of forested continents and the mass of crater and projectile debris ejected into the atmosphere.

They also examined the threshold temperatures and durations required to spontaneously ignite green wood, to ignite wood in the presence of an ignition source (such as lightning, which would be prevalent in the dust-laden energetic skies following an impact event) and to ignite rotting wood, leaves and other common forest litter.

“The Chicxulub impact event may have been the only known impact event to have caused wildfires around the globe,” Kring noted. “The Manicouagan (Canada) and Popigai (Russia) impact events, however, may have caused continental-scale fires. The Manicouagan impact occurred in the late Triassic, and the Popigai impact event occurred in the late Eocene, but neither has been firmly linked yet to the mass extinction events that occurred at those times.”

Kring is currently at the International Geological Congress in Florence, Italy, giving a keynote address on the Chicxulub impact event and its relationship to the mass extinctions at the Cretaceous-Tertiary boundary period. Durda is available for comment at the SwRI offices in Boulder, Colo.

Original Source: SWRI News Release

Mars Express View of Eos Chasma

This image, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, shows the southern part of Valles Marineris, called Eos Chasma.

The images was taken during orbit 533 in June 2004, and is centred at Mars longitude 322? East and latitude 11? South. The image resolution is approximately 80 metres per pixel.

Between surrounding plains and the smooth valley floor, a height difference of about 5000 metres has been measured.

The plain to the south, above Eos Chasma, is covered by several impact craters with diameters of around 20 kilometres and drainage channels.

To the east on this plain, isolated regions with cracked surfaces become more prominent. The direction of flow of the drainage channels in this area of the plain is ambiguous, as the channels to the north-east drain towards the south-east, and those in the south-west normally flow to the north-west.

The northern part of Eos Chasma?s valley floor is a rough area with angular hills reaching almost 1000 metres. In contrast, the southern part reveals a smooth topography with distinct flow structures.

In some areas of the southern slope, at least two terrace levels can be observed. Some haze in the valley hints at the presence of aerosols (airborne microscopic dust or liquid droplets).

Original Source: ESA News Release

Wallpaper: Hurricane Frances

This photo of Hurricane Frances was taken by Astronaut Mike Fincke aboard the International Space Station as he flew 230 statute miles above the storm at about 9 a.m. CDT Friday, Aug. 27, 2004. At the time, Frances was located 820 miles east of the Lesser Antilles in the Atlantic Ocean, moving west-northwest at 10 miles per hour, with maximum sustained winds of 105 miles per hour. Fincke, the NASA ISS Science Officer and Flight Engineer, and Expedition 9 Commander Gennady Padalka are in the fifth month of a six-month flight aboard the Station.

Original Source: NASA News Release

Satellites Track Inland Water Levels From Space

A few NASA satellites designed to study heights of Earth’s ocean surfaces are now also coming in handy for tracking water levels of inland lakes and reservoirs.

When analysts at the United States Department of Agriculture (USDA) Foreign Agriculture Service (FAS) learned that NASA satellites could be used for measuring lake water heights, they saw a chance to get vital information for managing irrigation and forecasting crop production in out-of-the way places.

Since early this year, NASA has supplied the USDA with near-real time data on lake and reservoir heights from around the world. The USDA has posted this information on a web site that allows users with a computer and Internet to access it for their varied uses. Analysts who forecast crop production, scientists, in-country water and irrigation managers, those involved in fishing industries, and the general public have all been making use of the site.

NASA and the French space agency Le Centre National d?Etudes Spatiales (CNES) teamed up to design, build and launch the TOPEX/Poseidon and the Jason-1 satellites. These satellites were designed to study many aspects of the ocean. The TOPEX/Poseidon satellite, for example, orbits at a height of 1336 kilometers (830 miles) above Earth, and can measure the height of the ocean surface directly underneath the satellite with an accuracy of 4-5 centimeters (better than 2 inches). Jason-1 and TOPEX/Poseidon cover the global oceans every 10 days. With these capabilities, this technology is surprisingly valuable for looking at larger areas of inland water.

“The satellites were designed with oceanographic objectives in mind, so the fact that they can be used for lakes and rivers are an added bonus,” said Charon Birkett, a University of Maryland researcher based at NASA’s Goddard Space Flight Center in Greenbelt, Md. It was Birkett’s work with satellites and inland water sources that caught the USDA’s interest.

Water level data for many lakes can be hard to get. Lakes may be located within inhospitable regions. Terrain may make it hard to install water level gauges, or some countries may not have the money for proper equipment. Even if there is equipment, someone must be available to regularly record the measurements. For an international agency like the USDA FAS, information on water levels in remote lakes in Africa or Asia, for example, may only be possible if a researcher happens to be passing by the area.

“Now we have this dataset which gives you a global picture of irrigation capabilities,” said Brad Doorn, Remote Sensing Technical Coordinator for the FAS. “It’s very much a night and day perspective as it relates to global irrigation potential.”

NASA/CNES satellites fly over 350 of the world’s largest lakes. The USDA decided to focus on about 150 of those that are important for agriculture. Of those, about 70 are currently online, with more being regularly added as Birkett and co-worker, Brian Beckley, from Raytheon’s Information Technology and Scientific Services (ITSS) team learn to extract information on the smaller lakes. Fifteen of the lakes that are currently online are in Africa.

The records begin with archived data from TOPEX/Poseidon, launched in 1992. They continued with data from the Jason-1 satellite, launched in December 2001. The two stayed in the same orbit for about 7 months, before the TOPEX/Poseidon satellite’s orbit was changed. These months of cross-over data were crucial for validating each of the satellites and for making sure the data records from Jason-1 were compatible with the TOPEX/Poseidon archive.

The information provided by the satellites, and made public through the web site, is a blessing to those who manage water for irrigation. Irrigated areas generally have less rainfall, and therefore crops in these drier regions are dependent on stores of water, like lakes, reservoirs and rivers.

The FAS analyzes crop production around the world. They regularly use computer models that simulate agricultural production based on inputs that include weather information. In this way they can examine global crop conditions and production. But in irrigated areas that are not rain fed, these methods are limited. For irrigated areas, you have to be able to determine how much water is actually stored, after seasonal precipitation passes.

“Satellite records of lake and reservoir water levels give you a good indication of whether there is going to be a systematic or major problem in water supply,” said Doorn. “If water is low, there may be problems for agricultural production.” This type of information is especially important for food aid partners, who must budget ahead for how much and where food aid is distributed.

Lake Tharthar in Central Iraq provides irrigation water to areas downstream. It is also linked to the Tigris and Euphrates Rivers. A drought that carried over many years severely cut grain output between 1999 and 2001. But since then, rainfall has increased, allowing grain production to recover and even surpass pre-drought levels. Knowledge of water levels in a region like this is crucial for the people who divvy out water for irrigation, and for those who plan aid.

The satellites have noticed some striking changes in lake levels around the world. In Iran, Lake Urmia has steadily decreased over the last 5 years. Also, between 1999 and 2001, Lake Hamoun in Iran near the Afghanistan border all but dried up and disappeared. By May 2003, water had returned to the lake. In that same time period, Lake Michigan levels have also declined.

On the other hand, when there is plenty of water, irrigation managers and farmers can assess the potential for more agriculture. When Caspian Sea levels rose in 1994, spill-over created a reservoir where little water existed before. As a result, the Kara Bogaz reservoir that borders the Caspian Sea was once largely desert and is now a large inland water body. Lake Nasser in Egypt also exists in a desert area where water supplies have increased.

As can be seen, the new technology allows researchers to get water level records regularly, globally, and in places where it is very hard to maintain or even acquire measurements. At the same time, there are also some limitations to the technology. For example, lake elevations can only be obtained during the lifetime of the satellite mission. Also, a satellite must pass directly over a lake for the radar to record water heights. But since the primary mission of these satellites is for studying the oceans, the fixed satellite orbit is determined by the community of oceanographers. That means people studying inland water have less input into the lakes that are monitored. In addition, some water bodies are simply too small for the instruments to pick up. These factors limit the number of observable lakes. “Sometimes, the lake that you want information about is the one you can’t get,” said Doorn.

Despite the current limitations, users like the FAS are thrilled to have access to the technology. Their web site provides new measurements to the public about a week to ten days after the satellite passes over.

“When USDA approached us, we told them the satellite record is not as accurate as a gauge sitting in a lake, but we can get good information within one to two weeks for many lakes in data-poor regions such as Africa and Asia,” said Birkett.

“It’s been a great USDA and NASA cooperative effort,” said Doorn. “It’s exactly what we needed and the type of cooperation provided has made it a real win-win situation.”

The project has been a collaborative effort between the NASA GSFC, USDA FAS, the University of Maryland, and Raytheon ITSS. The project was funded by the USDA/FAS.

Original Source: NASA News Release

3D Screensaver of Mars

I know you all like pretty pictures on your desktop, so here’s something that’ll help fill your bottomless need for photos. The European Space Agency releases screensavers from time to time filled with photos taken by their spacecraft. This one’s a little different, though, it’s a screensaver that displays 3D images. In order to properly see the perspective in the photo, you need a pair of those 3D glasses… you know the paper ones with a red and blue lens that you can get at 3D movies or with some books.

Download the screensaver. – 1.4 MB

It’s actually a good idea for you to keep a pair of these glasses on hand by your computer. Mars Express, Spirit and Opportunity can take pictures in stereo, so you can see a 3D view of what the Red Planet really looks like. You should be able to find a pair of glasses at your local bookstore. And here’s a website that’s giving away free 3D glasses.

Have fun,

Fraser Cain
Publisher
Universe Today

Recent Launch Demonstrates NASA Radar System

Radar tracking data gathered during the Delta II launch of the MESSENGER spacecraft earlier this month has provided promising results that may benefit NASA’s Space Shuttle Program and Discovery’s Return to Flight.

A pair of radars installed at NASA’s Kennedy Space Center, Fla., at a site north of Haulover Canal tracked the launch phase of the Delta II, including separation of the nine solid rocket boosters and jettison of the first stage and the payload fairing, the “nose” of the rocket that protected the MESSENGER spacecraft during launch.

“This test was quite successful for us in proving a concept,” said NASA project manager Tony Griffith. “The use of high-resolution wide band and Doppler radars allows us to observe almost any possible debris during ascent and means we can observe the Space Shuttle without regard to limitations of visibility, cloud cover and darkness.”

More importantly, the tandem radars “saw” — in significant detail — ice shedding from the Delta first stage, ejection of the solid rocket booster nozzle throat plugs, and contents of their exhaust. These are normal Delta launch events. For the Space Shuttle Program, the test showed that the radars, working together, were effective in visualizing the vehicle elements in high resolution and the ability to attain speedy interpretation of the images for initial data analysis after a Shuttle launch.

The antennas have been on loan to NASA from the USNS Pathfinder, a U.S. Navy instrumentation ship. The 30-foot-diameter C-band wideband radar antenna and the smaller X-band Doppler radar worked together to image the Delta in flight. The Navy operated the radars for NASA during the MESSENGER launch. NASA was responsible for analyzing the imagery.

“This turned out to be a successful and mutually beneficial partnership with the Navy that we will pursue,” Griffith said.

Later this fall, a 50-foot-diameter C-band wide band radar will be installed on this site for a similar Return to Flight application and for use by the Navy. The radar is being relocated to KSC from the Roosevelt Roads Naval Station in Puerto Rico.

The radars used for the test are being returned to the USNS Pathfinder, though the C-band radar used in this test could return as a backup for Return to Flight, if available from the Navy. NASA is evaluating the procurement of two X-band Doppler radars for use on ships downrange, including one of the solid rocket booster retrieval ships.

Original Source: NASA News Release

Mars Odyssey Goes into Overtime

NASA’s Mars Odyssey orbiter begins working overtime today after completing a prime mission that discovered vast supplies of frozen water, ran a safety check for future astronauts, and mapped surface textures and minerals all over Mars, among other feats.

“Odyssey has accomplished all of its mission-success criteria,” said Dr. Philip Varghese, project manager for Odyssey at NASA’s Jet Propulsion Laboratory, Pasadena, Calif. The spacecraft has been examining Mars in detail since February 2002, more than a full Mars year of about 23 Earth months. NASA has approved an extended mission through September 2006.

“This extension gives us another martian year to build on what we have already learned,” said JPL’s Dr. Jeff Plaut, project scientist for Odyssey. “One goal is to look for climate change. During the prime mission we tracked dramatic seasonal changes, such as the comings and goings of polar ice, clouds and dust storms. Now, we have begun watching for year-to-year differences at the same time of year.”

The extension will also continue Odyssey’s support for other Mars missions. About 85 percent of images and other data from NASA’s twin Mars rovers, Spirit and Opportunity, have reached Earth via communications relay by Odyssey, which receives transmissions from both rovers every day. The orbiter helped analyze potential landing sites for the rovers and is doing the same for NASA’s Phoenix mission, scheduled to land on Mars in 2008. Plans call for Odyssey to aid NASA’s Mars Reconnaissance Orbiter, due to reach Mars in March 2006, by monitoring atmospheric conditions during months when the newly arrived orbiter uses calculated dips into the atmosphere to alter its orbit into the desired shape.

Odyssey was launched April 7, 2001, and used the same dips into the atmosphere, known as aerobraking, to shape its orbit during the initial months after it reached Mars on Oct. 23, 2001. The spacecraft carries three research systems: a camera system made up of infrared and visible-light sensors; a spectrometer suite with a gamma ray spectrometer, a neutron spectrometer and a high-energy neutron detector; and a radiation environment detector.

Less than a month after the science mapping campaign began, the team announced a major discovery. The gamma ray and neutron instruments detected copious hydrogen just under Mars’ surface in the planet’s south polar region. Researchers interpret the hydrogen as frozen water — enough within about a meter (3 feet) of the surface, if the ice were melted, to fill Lake Michigan a couple times.

Here are a few of Odyssey’s other important accomplishments so far:

— As summer came to northern Mars and the north polar covering of frozen carbon dioxide shrank, Odyssey found abundant frozen water in the north, too.

— Infrared mapping showed that a mineral called olivine is widespread. This indicated the environment has been quite dry, because water exposure alters olivine into other minerals.

— Findings indicated the amount of frozen water in some relatively warm regions on Mars is too great to be in equilibrium with the atmosphere, suggesting that Mars may be going through a period of climate change. Features visible near small, young gullies in some Odyssey images may be slowly melting snowpacks left over from a martian ice age.

— The first experiment sent to Mars specifically in preparation for human missions found that radiation levels around Mars, from solar flares and cosmic rays, are two to three times higher than around Earth.

— Odyssey’s camera system obtained the most detailed complete global maps of Mars ever, with daytime and nighttime infrared images at a resolution of 100 meters (328 feet).

“We’ve accomplished everything we set out to do, and more,” said JPL’s Robert Mase, Odyssey mission manager. Although an unusually powerful solar flare in October 2003 knocked out the radiation environment instrument, Odyssey is otherwise in excellent health. The spacecraft has enough fuel onboard to keep operating through this decade and the next at current consumption rates. The mission extension, with a budget of $35 million, essentially doubles the science payoff from Odyssey for less than one-eighth of the mission’s original $297 million cost.

JPL, a division of the California Institute of Technology, Pasadena, manages Mars Odyssey for NASA’s Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, built and operates the spacecraft. Investigators at Arizona State University, Tempe; University of Arizona, Tucson; NASA’s Johnson Space Center, Houston; the Russian Aviation and Space Agency, Moscow; and Los Alamos National Laboratory, Los Alamos, N.M., built and operate Odyssey science instruments. For more information about Mars Odyssey on the Internet, visit: http://mars.jpl.nasa.gov/odyssey.

Original Source: NASA/JPL News Release

Beagle 2 Report Released

The UK-built Beagle 2 lander should have been on the surface of Mars, communicating with Earth for months now. But for some reason, shortly after it entered the Martian atmosphere, the small lander went silent, and it hasn’t been heard from since. Several inquiries have already been held, but now the mission operations team has released its own report to try and explain what could have gone wrong. The report provides a thorough list of ways the lander could have failed mechanically, but suggests that it was mostly likely that it failed during the entry, descent, and landing phase; probably because the atmosphere was less dense than the designers were expecting.

Smallest Extrasolar Planet Found

A European team of astronomers [1] has discovered the lightest known planet orbiting a star other than the sun (an “exoplanet”).

The new exoplanet orbits the bright star mu Arae located in the southern Altar constellation. It is the second planet discovered around this star and completes a full revolution in 9.5 days.

With a mass of only 14 times the mass of the Earth, the new planet lies at the threshold of the largest possible rocky planets, making it a possible super Earth-like object. Uranus, the smallest of the giant planets of the Solar System has a similar mass. However Uranus and the new exoplanet differ so much by their distance from the host star that their formation and structure are likely to be very different.

This discovery was made possible by the unprecedented accuracy of the HARPS spectrograph on ESO’s 3.6-m telescope at La Silla, which allows radial velocities to be measured with a precision better than 1 m/s. It is another clear demonstration of the European leadership in the field of exoplanet research.

A unique planet hunting machine
Since the first detection in 1995 of a planet around the star 51 Peg by Michel Mayor and Didier Queloz from the Geneva Observatory (Switzerland), astronomers have learned that our Solar System is not unique, as more than 120 giant planets orbiting other stars were discovered mostly by radial-velocity surveys (cf. ESO PR 13/00, ESO PR 07/01, and ESO PR 03/03).

This fundamental observational method is based on the detection of variations in the velocity of the central star, due to the changing direction of the gravitational pull from an (unseen) exoplanet as it orbits the star. The evaluation of the measured velocity variations allows to deduce the planet’s orbit, in particular the period and the distance from the star, as well as a minimum mass [2].

The continued quest for exoplanets requires better and better instrumentation. In this context, ESO undoubtedly took the leadership with the new HARPS spectrograph (High Accuracy Radial Velocity Planet Searcher) of the 3.6-m telescope at the ESO La Silla Observatory (see ESO PR 06/03). Offered in October 2003 to the research community in the ESO member countries, this unique instrument is optimized to detect planets in orbit around other stars (“exoplanets”) by means of accurate (radial) velocity measurements with an unequalled precision of 1 metre per second.

HARPS was built by a European Consortium [3] in collaboration with ESO. Already from the beginning of its operation, it has demonstrated its very high efficiency. By comparison with CORALIE, another well known planet-hunting optimized spectrograph installed on the Swiss-Euler 1.2-m telescope at La Silla (cf ESO PR 18/98, 12/99, 13/00), the typical observation times have been reduced by a factor one hundred and the accuracy of the measurements has been increased by a factor ten.

These improvements have opened new perspectives in the search for extra-solar planets and have set new standards in terms of instrumental precision.

The planetary system around mu Arae
The star mu Arae is about 50 light years away. This solar-like star is located in the southern constellation Ara (the Altar) and is bright enough (5th magnitude) to be observed with the unaided eye.

Mu Arae was already known to harbour a Jupiter-sized planet with a 650 days orbital period. Previous observations also hinted at the presence of another companion (a planet or a star) much further away.

The new measurements obtained by the astronomers on this object, combined with data from other teams confirm this picture. But as Fran?ois Bouchy, member of the team, states: “Not only did the new HARPS measurements confirm what we previously believed to know about this star but they also showed that an additional planet on short orbit was present. And this new planet appears to be the smallest yet discovered around a star other than the sun. This makes mu Arae a very exciting planetary system.”

During 8 nights in June 2004, mu Arae was repeatedly observed and its radial velocity measured by HARPS to obtain information on the interior of the star. This so-called astero-seismology technique (see ESO PR 15/01) studies the small acoustic waves which make the surface of the star periodically pulsate in and out. By knowing the internal structure of the star, the astronomers aimed at understanding the origin of the unusual amount of heavy elements observed in its stellar atmosphere. This unusual chemical composition could provide unique information to the planet formation history.

Says Nuno Santos, another member of the team: “To our surprise, the analysis of the new measurements revealed a radial velocity variation with a period of 9.5 days on top of the acoustic oscillation signal!”

This discovery has been made possible thanks to the large number of measurements obtained during the astero-seimology campaign.

From this date, the star, that was also part of the HARPS consortium survey programme, was regularly monitored with a careful observation strategy to reduce the “seismic noise” of the star.

These new data confirmed both the amplitude and the periodicity of the radial velocity variations found during the 8 nights in June. The astronomers were left with only one convincing explanation to this periodic signal: a second planet orbits mu Arae and accomplishes a full revolution in 9.5 days.

But this was not the only surprise: from the radial velocity amplitude, that is the size of the wobble induced by the gravitational pull of the planet on the star, the astronomers derived a mass for the planet of only 14 times the mass of the Earth! This is about the mass of Uranus, the smallest of the giant planets in the solar system.

The newly found exoplanet therefore sets a new record in the smallest planet discovered around a solar type star.

At the boundary
The mass of this planet places it at the boundary between the very large earth-like (rocky) planets and giant planets.

As current planetary formation models are still far from being able to account for all the amazing diversity observed amongst the extrasolar planets discovered, astronomers can only speculate on the true nature of the present object. In the current paradigm of giant planet formation, a core is formed first through the accretion of solid “planetesimals”. Once this core reaches a critical mass, gas accumulates in a “runaway” fashion and the mass of the planet increases rapidly. In the present case, this later phase is unlikely to have happened for otherwise the planet would have become much more massive. Furthermore, recent models having shown that migration shortens the formation time, it is unlikely that the present object has migrated over large distances and remained of such small mass.

This object is therefore likely to be a planet with a rocky (not an icy) core surrounded by a small (of the order of a tenth of the total mass) gaseous envelope and would therefore qualify as a “super-Earth”.

Further Prospects
The HARPS consortium, led by Michel Mayor (Geneva Observatory, Switzerland), has been granted 100 observing nights per year during a 5-year period at the ESO 3.6-m telescope to perform one of the most ambitious systematic searches for exoplanets so far implemented worldwide. To this aim, the consortium repeatedly measures velocities of hundreds of stars that may harbour planetary systems.

The detection of this new light planet after less than 1 year of operation demonstrates the outstanding potential of HARPS for detecting rocky planets on short orbits. Further analysis shows that performances achieved with HARPS make possible the detection of big “telluric” planets with only a few times the mass of the Earth. Such a capability is a major improvement compared to past planet surveys. Detection of such rocky objects strengthens the interest of future transit detections from space with missions like COROT, Eddington and KEPLER that shall be able to measure their radius.

More information
The research described in this Press release has been submitted for publication to the leading astrophysical journal “Astronomy and Astrophysics”. A preprint is available as a postscript file at http://www.oal.ul.pt/~nuno/.

Notes
[1]: The team is composed of Nuno Santos (Centro de Astronomia e Astrofisica da Universidade de Lisboa, Portugal), Fran?ois Bouchy and Jean-Pierre Sivan (Laboratoire d’astrophysique de Marseille, France), Michel Mayor, Francesco Pepe, Didier Queloz, St?phane Udry, and Christophe Lovis (Observatoire de l’Universit? de Gen?ve, Switzerland), Sylvie Vauclair, Michael Bazot (Toulouse, France), Gaspare Lo Curto and Dominique Naef (ESO), Xavier Delfosse (LAOG, Grenoble, France), Willy Benz and Christoph Mordasini (Physikalisches Institut der Universit?t Bern, Switzerland), and Jean-Louis Bertaux (Service d’A?ronomie de Verri?re-le-Buisson, Paris, France).

[2] A fundamental limitation of the radial-velocity method is the unknown of the inclination of the planetary orbit that only allows the determination of a lower mass limit for the planet. However, statistical considerations indicate that in most cases, the true mass will not be much higher than this value. The mass units for the exoplanets used in this text are 1 Jupiter mass = 22 Uranus masses = 318 Earth masses; 1 Uranus mass = 14.5 Earth masses.

[3] HARPS has been designed and built by an international consortium of research institutes, led by the Observatoire de Gen?ve (Switzerland) and including Observatoire de Haute-Provence (France), Physikalisches Institut der Universit?t Bern (Switzerland), the Service d’Aeronomie (CNRS, France), as well as ESO La Silla and ESO Garching.

Original Source: ESO News Release