Category: Mars

Image credit: NASA/JPL

With Spirit safely on the surface of Mars, engineers at NASA are starting to get a sense of the environment around it. So far, it looks like the rover couldn’t have landed in a better spot. The platform holding the rover is only tilted a few degrees, and there are no large rocks blocking the ramps. The terrain has lots of rocks to examine, but they’re well spaced out, which should let Spirit travel at a fairly high speed across the ground. Spirit will remain on the landing platform for another nine days or so before it ventures out onto search the area for evidence of past water.

NASA’s Spirit Rover is starting to examine its new surroundings, revealing a vast flatland well suited to the robot’s unprecedented mobility and scientific toolkit.

“Spirit has told us that it is healthy,” Jennifer Trosper of NASA’s Jet Propulsion Laboratory, Pasadena, Calif., said today. Trosper is Spirit mission manager for operations on Mars’ surface. The rover remains perched on its lander platform, and the next nine days or more will be spent preparing for egress, or rolling off, onto the martian surface.

With only two degrees of tilt, with the deck toward the front an average of only about 37 centimeters (15 inches) off the ground, and with apparently no large rocks blocking the way, the lander is in good position for egress. “The egress path we’re working toward is straight ahead,” Trosper said.

The rover’s initial images excited scientists about the prospects of exploring the region after the roll-off.

“My hat is off to the navigation team because they did a fantastic job of getting us right where we wanted to be,” said Dr. Steve Squyres of Cornell University, Ithaca, N.Y., principal investigator for the science payload. By correlating images taken by Spirit with earlier images from spacecraft orbiting Mars, the mission team has determined that the rover appears to be in a region marked with numerous swaths where dust devils have removed brighter dust and left darker gravel behind.

“This is our new neighborhood,” Squyres said. “We hit the sweet spot. We wanted someplace where the wind had cleared off the rocks for us. We’ve landed in a place that’s so thick with dust devil tracks that a lot of the dust has been blown away.”

The terrain looks different from any of the sites examined by NASA’s three previous successful landers — the two Vikings in 1976 and Mars Pathfinder in 1997.

“What we’re seeing is a section of surface that is remarkably devoid of big boulders, at least in our immediate vicinity, and that’s good news because big boulders are something we would have trouble driving over,” Squyres said. “We see a rock population that is different from anything we’ve seen elsewhere on Mars, and it comes out very much in our favor.”

Spirit arrived at Mars Jan. 3 (EST and PST; Jan. 4 Universal Time) after a seven month journey. Its task is to spend the next three months exploring for clues in rocks and soil about whether the past environment at this part of Mars was ever watery and suitable to sustain life.

Spirit’s twin Mars Exploration Rover, Opportunity, will reach its landing site on the opposite side of Mars on Jan. 25 (EST and Universal Time; Jan. 24 PST) to begin a similar examination of a site on the opposite side of the planet from Gusev Crater.

JPL, a division of the California Institute of Technology, manages the Mars Exploration Rover project for NASA’s Office of Space Science, Washington. Additional information about the project is available from JPL at: http://marsrovers.jpl.nasa.gov and from Cornell University at: http://athena.cornell.edu.

Original Source: NASA/JPL News Release

Image credit: NASA/JPL

NASA controllers confirmed that the Spirit rover successfully landed on Mars today. The spacecraft passed through the atmosphere, deployed its parachute, fired its retrorockets, and then bounced along the Martian surface protected by airbags – its landing time was January 4 at 0435 UTC (11:35 pm EST January 3). Pictures from the Martian surface are expected soon. Spirit will spend at least 90 days traveling around the surface of Mars, searching for evidence of past water with several scientific instruments. The next rover, Opportunity, is expected to land on January 24.

A traveling robotic geologist from NASA has landed on Mars and returned stunning images of the area around its landing site in Gusev Crater.

Mars Exploration Rover Spirit successfully sent a radio signal after the spacecraft had bounced and rolled for several minutes following its initial impact at 11:35 p.m. EST (8:35 p.m. Pacific Standard Time) on January 3.

“This is a big night for NASA,” said NASA Administrator Sean O’Keefe. “We’re back. I am very, very proud of this team, and we’re on Mars.”

Members of the mission’s flight team at NASA’s Jet Propulsion Laboratory, Pasadena, Calif., cheered and clapped when they learned that NASA’s Deep Space Network had received a post-landing signal from Spirit. The cheering resumed about three hours later when the rover transmitted its first images to Earth, relaying them through NASA’s Mars Odyssey orbiter.

“We’ve got many steps to go before this mission is over, but we’ve retired a lot of risk with this landing,” said JPL’s Pete Theisinger, project manager for the Mars Exploration Rover Project.

Deputy project manager for the rovers, JPL’s Richard Cook, said, “We’re certainly looking forward to Opportunity landing three weeks from now.” Opportunity is Spirit’s twin rover, headed for the opposite side of Mars.

Dr. Charles Elachi, JPL director, said, “To achieve this mission, we have assembled the best team of young women and men this country can put together. Essential work was done by other NASA centers and by our industrial and academic partners.

Spirit stopped rolling with its base petal down, though that favorable position could change as airbags deflate, said JPL’s Rob Manning, development manager for the rover’s descent through Mars’ atmosphere and landing on the surface.

NASA chose Spirit’s landing site, within Gusev Crater, based on evidence from Mars orbiters that this crater may have held a lake long ago. A long, deep valley, apparently carved by ancient flows of water, leads into Gusev. The crater itself is basin the size of Connecticut created by an asteroid or comet impact early in Mars’ history. Spirit’s task is to spend the next three months exploring for clues in rocks and soil about whether the past environment at this part of Mars was ever watery and suitable to sustain life.

Spirit traveled 487 million kilometers (302.6 million) miles to reach Mars after its launch from Cape Canaveral Air Force Station, Fla., on June 10, 2003. Its twin, Mars Exploration Rover Opportunity, was launched July 7, 2003, and is on course for a landing on the opposite side of Mars on Jan. 25 (Universal Time and EST; 9:05 p.m. on Jan. 24, PST).

The flight team expects to spend more than a week directing Spirit through a series of steps in unfolding, standing up and other preparations necessary before the rover rolls off of its lander platform to get its wheels onto the ground. Meanwhile, Spirit’s cameras and a mineral-identifying infrared instrument will begin examining the surrounding terrain. That information will help engineers and scientists decide which direction to send the rover first.

JPL, a division of the California Institute of Technology, manages the Mars Exploration Rover project for NASA’s Office of Space Science, Washington. Additional information about the project is available from JPL at:

http://marsrovers.jpl.nasa.gov , www.nasa.gov and from Cornell University, Ithaca, N.Y., at http://athena.cornell.edu.

Original Source: NASA/JPL News Release

When Pathfinder arrived at Mars back in 1997, I kept a tiny video window open on my desktop to watch every moment of the mission – all thanks to the Internet. It was pretty choppy at times, so hopefully NASA has more bandwidth this time.

Spirit is expected to arrive in Gusev Crater on Mars on January 4 at 0435 UTC (11:35 pm EST, 8:35 pm PST January 3). Live coverage on NASA television begins about two hours before landing and will continue all through Sunday and into Monday. You can access the NASA television page here. The main NASA TV link will probably overwhelmed, so I highly recommend you try out some of the alternative links. We’ll try and keep track of links to video streams in the forum which are able to handle the bandwidth.

Come on Spirit!

Fraser Cain
Publisher
Universe Today

Image credit: Beagle 2

The search for Beagle 2 continues. Operators announced on December 31 that the British lander had failed to report in for the eighth time. At this point, the lander will have switched to a new mode where it tries to communicate twice a day. Although unlikely, it’s possible that Beagle 2’s onboard timer was reset during the landing, which would mean it was trying to communicate out of sync with Mars Odyssey and Earth-based radio telescopes. Mars Express will start searching on January 5, which operators believe will bring their best chances of finding it.

News on the outcome of today’s communication attempt via Mars Odyssey was delayed for several hours because NASA’s Deep Space Network is also being used for the Mars Exploration Rover and Stardust missions, which will be reaching their climax in the next few days.

As from last night, Beagle 2 should have switched to an emergency mode known as ‘ communication search mode 1′ (CSM 1). When the lander switches to CSM 1, it attempts to communicate twice every Martian day (sol), during the best daytime and best night-time pass by an available orbiter.

Meanwhile, ESA’s Mars Express orbiter was successfully inserted into a polar orbit around the Red Planet yesterday morning. This manoeuvre means that Mars Express will be ideally placed to communicate with Beagle 2 when it passes over the landing site in Isidis Planitia in a few days’ time.

An updated list of future opportunities to communicate with Beagle 2, including pre-programmed sessions with Mars Express, is posted on the Beagle 2 Web site.

The next Beagle 2 press briefing is scheduled to take place at the Media Centre in Camden on Sunday 4 January. Details will be confirmed on the Web sites at a later date.

Original Source: PPARC News Release

Image credit: NASA/JPL

NASA’s Spirit rover made a slight correction to its trajectory on December 26, when it fired its thrusters for 3.4 seconds. The maneuver went flawlessly, and put the lander right on course to land in Mars’ Gusev Crater on January 4 at 0435 UTC (11:35 pm EST January 3). This was Spirit’s fourth trajectory correction maneuver since its launch on June 10, and two more might still happen in the final days if its flight is a little off-target. As with Beagle 2, the most dangerous part of the mission will happen when the rovers have to pass through Mars atmosphere and land safely on the planet.

NASA’s Spirit rover spacecraft fired its thrusters for 3.4 seconds on Friday, Dec. 26, to make a slight and possibly final correction in its flight path about one week before landing on Mars.

Radio tracking of the spacecraft during the 24 hours after the maneuver showed it to be right on course for its landing inside Mars’ Gusev Crater at 04:35 Jan. 4, 2004, Universal Time (8:35 p.m. Jan. 3, Pacific Standard Time.) Spirit’s twin, Opportunity, will reach Mars three weeks later.

“The maneuver went flawlessly,” said Dr. Mark Adler, Spirit mission manager at NASA’s Jet Propulsion Laboratory, Pasadena, Calif.

This was Spirit’s fourth trajectory correction maneuver since launch on June 10. Two more are on the schedule for the flight’s final three days, if needed. Adler said, “It seems unlikely we’ll have to do a fifth trajectory correction maneuver, but we’ll make the final call Thursday morning after we have a few more days of tracking data. Right now, it looks as though we hit the bull’s-eye.”

The adjustment was a quick nudge approximately perpendicular to the spacecraft’s spin axis, said JPL’s Chris Potts, deputy navigation team chief for the NASA Mars Exploration Rover project. “It moved the arrival time later by 2 seconds and moved the landing point on the surface northeast by about 54 kilometers” (33 miles), Potts said. The engine firing changed the velocity of the spacecraft by only 25 millimeters per second (about one-twentieth of one mile per hour).

For both NASA rovers approaching Mars, the most daunting challenges will be descending through Mars’ atmosphere, landing on the surface, and opening up properly from the enclosed and folded configuration in which the rovers arrive. Most previous Mars landing attempts, by various nations, have failed.

Each rover, if it arrives successfully, will then spend more than a week in a careful sequence of steps before rolling off its lander platform. The rovers’ mission is to examine their landing areas for geological evidence about past environmental conditions. In particular, they will seek evidence about the local history of liquid water, which is key information for assessing whether the sites ever could have been hospitable to life. Opportunity will land halfway around Mars from Spirit.

As of 13:00 Universal Time (6 a.m. PST) on New Year’s Day, Spirit will have traveled 481.9 million kilometers (299.4 million miles) since launch and have will have 5.1 million kilometers (3.2 million miles) left to go. Opportunity will have traveled 411 million kilometers (255 million miles) since its July 7 launch and will have 45 million kilometers (27.9 million miles) to go, with three remaining scheduled opportunities for trajectory correction maneuvers.

JPL, a division of the California Institute of Technology, manages the Mars Exploration Rover project for NASA’s Office of Space Science, Washington.

Additional information about the project is available from JPL at http://marsrovers.jpl.nasa.gov and from Cornell University, Ithaca, N.Y., at http://athena.cornell.edu.

Original Source: NASA/JPL News Release

Image credit: ESA

The European Space Agency’s Mars Express completed a major orbit maneuver, bringing the spacecraft from an equatorial orbit to a polar orbit around Mars. The spacecraft’s main engine was fired for four minutes. Now that it’s in a polar orbit around Mars, the spacecraft will be able to begin its scientific analysis of Mars, using its MARSIS radar to search up to several kilometres under the surface for reserves of water and ice. Mars Express will fly directly over the Beagle 2 landing site on January 7, 2004 and attempt to communicate with it.

This morning, at 09:00 CET, the first European mission to Mars registered another operational success. The Mars Express flight control team at ESOC prepared and executed another critical manoeuvre, bringing the spacecraft from an equatorial orbit into a polar orbit around Mars.

All commands were transmitted to Mars Express via ESA’s new Deep Space Station in New Norcia, Australia. This morning, the main engine of Mars Express was fired for four minutes to turn the spacecraft into a new direction, at a distance of 188 000 kilometres from Mars and about 160 million kilometres from Earth. On 4 January 2004, this new polar orbit will be reduced even further.

Fascinating ESA science mission ahead
In a polar orbit, Mars Express can now start to prepare its scientific observation mission as planned, working much like an ‘Earth-observation satellite’ but around Mars. From the second half of January 2004, the orbiter’s instruments will be able to scan the atmosphere, the surface and parts of the subsurface structure of Mars with unmatched precision.

The MARSIS radar, for example, will be able to scan as far as four kilometres below the surface, looking for underground water or ice. The High Resolution Stereo Camera will take high-precision pictures of the planet and will begin a comprehensive 3D cartography of Mars. Also, several spectrometers will try to unveil the mysteries of Martian mineralogy and the atmosphere, as well as influences from the solar wind or seasonal changes.

Mars Express closes in on Beagle 2 landing area
The change of orbit by the Mars Express orbiter will allow increasingly closer looks at the Beagle 2 landing site, which measures 31 kilometres by 5 kilometres. In this narrowing polar orbit, the orbiter will fly directly over the landing site at an altitude of 315 kilometres on 7 January 2004, at 13:13 CET. The reduced distance, the ideal angle of overflight and originally foreseen communication interfaces between the ‘mother’ and ‘baby’ will increase the probability of catching signals from the ground.

Ongoing European co-operation and international support
The Mars Express flight control team of ESA in Darmstadt, Germany, is in regular contact with its colleagues of the Beagle 2 team and with NASA ground stations. In addition, ESA receives regular support or offers of support from the Jodrell Bank radio telescope in the UK, Westerborg telescope in the Netherlands, Effelsberg telescope in Germany and Stanford University’s telescope in the USA. ESA is grateful for this spirit of dynamic international co-operation on its first mission to Mars.

Original Source: ESA News Release

Image credit: Malin

Lord Sainsbury, the UK Minister of Science and Technology reinforced today that they haven’t given up hope on Beagle 2, and continue to be optimistic that the lander will be found. A “tiger team” of engineers and scientists are working through all the scenarios that could help to explain what’s wrong with Beagle 2 (other than it’s all smashed up on the Martian surface). One theory is that the lander might have fallen into a kilometre-sized crater which was in the landing zone; although, the chances of this happening are pretty remote.

The latest attempts to communicate with Beagle 2 via the Lovell Telescope at Jodrell Bank and the Mars Odyssey spacecraft have been unsuccessful. However, the Beagle 2 team has not given up hope and continues to be optimistic that efforts to contact the lander will eventually be successful.

This message was also reinforced by Lord Sainsbury, UK Minister for Science and Innovation, who this morning joined members of the Beagle 2 team to answer questions about the status of the project.

“While we’re disappointed that things have not gone according to plan, we are determined that the search should go on, both the search to make contact with Beagle 2 and also (the search) to answer the long term question about whether there is life on Mars,” said Lord Sainsbury.

“There’s clearly still a good opportunity to make contact with Beagle 2 with Mars Express when it comes into action, and that has to be the first priority at this point. I think everything is being done by the ‘tiger team’ in Leicester to make contact with Beagle 2 and I want to wish them every success in their efforts.”

“We are looking at a number of possible failure modes that we might do something about,” said Dr. Mark Sims, Beagle 2 mission manager from the University of Leicester.

“We are working under the assumption that Beagle 2 is on the surface of Mars and for some reason cannot communicate to us. In particular, we’re looking at two major issues. One is communications, and there are also related timing and software issues.

“We’ve got a few more Odyssey contacts, the last one being on 31 December. Then we have four contacts with Mars Express already pre-programmed into Beagle, assuming the software is running, on 6, 12, 13 and 17. The 6 and 12 are when Mars Express is manoeuvring into its final orbit, so they are not optimum for Beagle 2 communications. The 13th and 17th are very good opportunities for Mars Express.”

According to Dr. Sims, one of the scenarios the team was investigating – a timer and hardware reset – now seems unlikely, and can probably be ruled out. However, other possible slips of the onboard time may have been caused by software or problems of copying data between various parts of memory. Possibly, all of the stored command times have been lost.

“None of these can yet be eliminated,” he said.

After the tenth contact attempt, Beagle 2 will move into communication search mode 1 (CSM 1), taking advantage of the ability of the software on board Beagle 2 to recognise when dawn and dusk occur on Mars by measuring the current feeding from the solar arrays.

“When we get into CSM 1 mode, Beagle 2 will start putting additional contacts on its time line, independent of the clock value,” said Mark Sims. “This will happen after 31 December.”

The team is also looking at sending blind commands to Beagle 2. This is helped by Beagle going into CSM 1 mode.

“The team has come up with a method of fooling the receiver into accepting commands without having to talk back to the orbiter,” said Dr. Sims. “We have an agreement with JPL to reconfigure Odyssey to provisionally attempt this on 31 December, the last programmed Odyssey pass.”

Malin Space Science Systems has also provided the Beagle 2 team with a picture of the landing site taken by the camera on Mars Global Surveyor 20 minutes after the spacecraft’s scheduled touchdown. It shows that the weather was quite good on the day Beagle landed, so it was unlikely to be a factor in the descent. The next opportunity to image the landing site with Mars Global Surveyor will not be until 5 January.

The image showing the centre of Beagle 2’s landing ellipse also shows a 1 km wide crater. There is just an outside possibility that the lander could have touched down inside this crater, resulting in problems caused by steep slopes, large number of rocks or disruption to communication from the lander. This image is now available on the Beagle 2 and PPARC Web sites (see link on the right hand side).

While the Lander Operations Control Centre in Leicester continues its efforts to communicate with the Beagle 2, Lord Sainsbury took the opportunity to inform the media that the UK government is keen to continue the innovative robotic exploration effort begun with the lander.

“Long term we need to be working with ESA to ensure that in some form there is a Beagle 3 which takes forwards this technology,” he said. “I very much hope that the Aurora programme, which is now being developed by ESA, will take forward this kind of robotic exploration.

“We’ve always recognised that Beagle 2 was a high risk project, and we must avoid the temptation in future to only do low risk projects.

“I’d like to use this opportunity to add my thanks to all those helping our efforts to make contact with Beagle 2. I think the amount of international collaboration one gets on these occasions is very, very impressive and very encouraging to the team.”

“We should not ignore the importance of Mars Express, which has three British-designed instruments on board and which looks set for success,” he added.

“Finally, can I use this opportunity to wish the Americans every success with its two Mars Exploration Rovers, Spirit and Opportunity.”

Original Source: PPARC News Release

Image credit: ESA

Unlike its missing passenger, Beagle 2, controllers from the European Space Agency know exactly where Mars Express is – exactly where they want it. The spacecraft is currently on a wide equatorial orbit which brings it as close as 400 km and then out to 188,000 km away from the planet. Engineers are preparing the spacecraft for a further burn of its main engine which will bring the spacecraft into a closer polar orbit around Mars. Once Mars Express modifies its orbit, it will be the best candidate to communicate with the missing Beagle 2; starting January 4, 2004.

The Mars Express orbiter, mothership of Europe’s first mission to the Red Planet, is in a stable and precise orbit around Mars.

The essential Mars Orbit Insertion (MOI) manoeuvre had been completed on 25 December at 3:47 CET. This brought the spacecraft as close as 400 kilometres to the surface of Mars.

Afterwards, the spacecraft went into a highly elliptical orbit, going as far as 188 000 kilometres away from the planet. The most essential part of the Mars Express mission is performing very well and we are expecting exciting science from January 2004 onwards.

Today, 27 December, the mission control team at ESOC prepared the next steps to turn Mars Express from a near-equatorial orbit into a polar orbit. Michael McKay, Mars Express Flight Director explained, “Our flight dynamics and flight operations teams thoroughly discuss, evaluate and prepare the commands to perform a series of manoeuvres starting with a major move on 30 December – where we will fire the main engine again for three minutes.

“These key manoeuvres will allow us to get even closer to Mars. They will not only allow us more frequent ‘overflights’ of the Beagle 2 landing area, but also ensure the beginning of the orbiter’s science mission. As Mars Express is the planned main communication partner of the Beagle 2, the chances of obtaining a signal strongly increase with these manoeuvres after 4 January 2004.”

Close European and international co-operation
The ESA control team at ESOC are in regular contact with their colleagues of the Beagle 2 team and the Jodrell Bank telescope in the UK, with NASA ground stations and with several other European partners (UK, Germany, Netherlands, etc.). Many international offers have been forthcoming to support the search for the Beagle 2 lander.

Original Source: ESA News Release

Image credit: ESA

Controllers have made two more attempts to reach the Beagle 2 lander, which was thought to have entered Mars’ atmosphere on December 25: once with both the Jodrell Bank radio telescope and again with Mars Odyssey. Although they’re disappointed, the engineers still have a few tricks up their sleeves. A special team has been put together, and is working around the clock to devise solutions for potential problems with the lander; if there are hardware or software problems, or if it’s ended up at an unusual angle. People will really start to lose hope in early January when Mars Express reaches its final polar orbit – it’s the spacecraft Beagle 2 was designed to communicate with.

Two attempts to communicate with Beagle 2 during the last 24 hours – first with the 76 metre (250 feet) Lovell Telescope at Jodrell Bank Observatory in Cheshire, UK, and then this morning with the Mars Odyssey orbiter – ended without receiving a signal. Despite this outcome, fresh attempts to scan for a signal from Beagle 2 will be made over the coming days.

Meanwhile, scientists and engineers are eagerly awaiting ESA’s Mars Express spacecraft return close enough to Mars to try to establish contact with Beagle 2. This may be possible from 4 January 2004.

Mars Express was always intended to be the prime communication relay for Beagle 2, and the lander team is hopeful that a link can be established at that time if it has not already been achieved with Mars Odyssey.

“We need to get Beagle 2 into a period when it can broadcast for a much longer period,” says Professor Colin Pillinger, Beagle 2 lead scientist. “This will happen around the 4 January after the spacecraft has experienced a sufficient number of communication failures to switch to automatic transmission mode.”

Both Professor Pillinger and Professor David Southwood, ESA Director of Science, agreed that the best chance to establish communication with Beagle 2 would now seem to be through Mars Express.

At present, Mars Express is far from the planet and preparing to fire its engines for a major trajectory change that will move it into a polar orbit around Mars.

“We will have no satisfaction until we have a full mission” said Professor Southwood. “Today I’m certainly frustrated, but I’m still confident: let’s wait now until the mothership will have the possibility to get in contact with her baby. With Mars Express we will be using a system that we have fully tested and understand.”

Original Source: ESA News Release

Image credit: PPARC

After NASA’s Mars Odyssey failed to make contact with the British-built Beagle 2 lander on Christmas morning, all hopes were pinned on the Earth-based Jodrell Bank radio telescope to hear its faint signal. After listening for more than two hours, unfortunately, operators failed to tune into the spacecraft’s signal. Then another opportunity to communicate with Odyssey on December 26 failed as well. Mission controllers haven’t completely lost hope, though. When Mars Express reaches its final orbit in early January, it will be the best opportunity to communicate with Beagle 2 and help determine, once and for all, if the spacecraft survived its landing.

Scientists were hopeful that the 250 ft (76 m) Lovell Telescope, recently fitted with a highly sensitive receiver, would be able to pick up the outgoing call from the Mars lander between 19.00 GMT and midnight last night. An attempt to listen out for Beagle’s call home by the Westerbork telescope array in the Netherlands was unfortunately interrupted by strong radio interference.

The next window of opportunity to communicate via Mars Odyssey will open at 17.53 GMT and close at 18.33 GMT this evening, when the orbiter is within range of the targeted landing site on Isidis Planitia.

Another communication session from Jodrell Bank is scheduled between 18.15 GMT and midnight tonight, when Mars will be visible to the radio telescope. It is also hoped that the Stanford University radio telescope in California will be able to listen for the carrier signal on 27 December.

The Beagle 2 team plans to continue using the Mars Odyssey spacecraft as a Beagle 2 communications relay for the next 10 days, after which the European Space Agency’s Mars Express orbiter will become available.

Mars Express, which was always planned to be Beagle 2’s main communication link with Earth, successfully entered orbit around the planet on 25 December and is currently being manoeuvred into its operational polar orbit.

Meanwhile, 13 more attempts to contact Mars Odyssey have been programmed into Beagle 2’s computer. If there is still no contact established after that period, Beagle 2 is programmed to move into auto-transmission mode, when it will send a continuous on-off pulse signal throughout the Martian daylight hours.

The first window of opportunity to communicate with Beagle 2 took place at around 06.00 GMT yesterday, when NASA’s Mars Odyssey spacecraft flew over the planned landing site. In the absence of a signal from the 33 kg lander, the mission team contacted Jodrell Bank to put their contingency plan into operation.

At present, Beagle 2 should be sending a pulsing on-off signal once a minute (10 seconds on, 50 seconds off). Some 9 minutes later, this very slow “Morse Code” broadcast should reach Earth after a journey of some 98 million miles (157 million km).

Although the Beagle’s transmitter power is only 5 watts, little more than that of a mobile phone, scientists are confident that the signal can be detected by the state-of-the-art receiver recently installed on the Lovell Telescope. However, a significant drop in signal strength would require rigorous analysis of the data before it could be unambiguously identified.

Although the ground-based radio telescopes will not be able to send any reply, the new information provided by detection of the transmission from Beagle 2 would enable the mission team to determine a provisional location for Beagle 2. This, in turn, would allow the communications antenna on Mars Odyssey to be directed more accurately towards Beagle 2 during the orbiter’s subsequent overhead passes.

Original Source: PPARC News Release