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Old 29-09-10, 10:47 PM
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Default Newly Discovered Planet May Be First Truly Habitable Exoplanet

Newly Discovered Planet May Be First Truly Habitable Exoplanet

ScienceDaily (Sep. 29, 2010) — A team of planet hunters led by astronomers at the University of California, Santa Cruz, and the Carnegie Institution of Washington has announced the discovery of an Earth-sized planet (three times the mass of Earth) orbiting a nearby star at a distance that places it squarely in the middle of the star's "habitable zone," where liquid water could exist on the planet's surface. If confirmed, this would be the most Earth-like exoplanet yet discovered and the first strong case for a potentially habitable one.

To astronomers, a "potentially habitable" planet is one that could sustain life, not necessarily one that humans would consider a nice place to live. Habitability depends on many factors, but liquid water and an atmosphere are among the most important.

"Our findings offer a very compelling case for a potentially habitable planet," said Steven Vogt, professor of astronomy and astrophysics at UC Santa Cruz. "The fact that we were able to detect this planet so quickly and so nearby tells us that planets like this must be really common."

The findings are based on 11 years of observations at the W. M. Keck Observatory in Hawaii. "Advanced techniques combined with old-fashioned ground-based telescopes continue to lead the exoplanet revolution," said Paul Butler of the Carnegie Institution. "Our ability to find potentially habitable worlds is now limited only by our telescope time."

Vogt and Butler lead the Lick-Carnegie Exoplanet Survey. The team's new findings are reported in a paper to be published in The Astrophysical Journal and posted online at arXiv.org. Coauthors include associate research scientist Eugenio Rivera of UC Santa Cruz; associate astronomer Nader Haghighipour of the University of Hawaii-Manoa; and research scientists Gregory Henry and Michael Williamson of Tennessee State University.

The paper reports the discovery of two new planets around the nearby red dwarf star Gliese 581. This brings the total number of known planets around this star to six, the most yet discovered in a planetary system other than our own solar system. Like our solar system, the planets around Gliese 581 have nearly circular orbits.

The most interesting of the two new planets is Gliese 581g, with a mass three to four times that of the Earth and an orbital period of just under 37 days. Its mass indicates that it is probably a rocky planet with a definite surface and that it has enough gravity to hold on to an atmosphere, according to Vogt.

Gliese 581, located 20 light years away from Earth in the constellation Libra, has a somewhat checkered history of habitable-planet claims. Two previously detected planets in the system lie at the edges of the habitable zone, one on the hot side (planet c) and one on the cold side (planet d). While some astronomers still think planet d may be habitable if it has a thick atmosphere with a strong greenhouse effect to warm it up, others are skeptical. The newly discovered planet g, however, lies right in the middle of the habitable zone.

"We had planets on both sides of the habitable zone--one too hot and one too cold--and now we have one in the middle that's just right," Vogt said.

The planet is tidally locked to the star, meaning that one side is always facing the star and basking in perpetual daylight, while the side facing away from the star is in perpetual darkness. One effect of this is to stabilize the planet's surface climates, according to Vogt. The most habitable zone on the planet's surface would be the line between shadow and light (known as the "terminator"), with surface temperatures decreasing toward the dark side and increasing toward the light side.

"Any emerging life forms would have a wide range of stable climates to choose from and to evolve around, depending on their longitude," Vogt said.

The researchers estimate that the average surface temperature of the planet is between -24 and 10 degrees Fahrenheit (-31 to -12 degrees Celsius). Actual temperatures would range from blazing hot on the side facing the star to freezing cold on the dark side.

If Gliese 581g has a rocky composition similar to the Earth's, its diameter would be about 1.2 to 1.4 times that of the Earth. The surface gravity would be about the same or slightly higher than Earth's, so that a person could easily walk upright on the planet, Vogt said.

The new findings are based on 11 years of observations of Gliese 581 using the HIRES spectrometer (designed by Vogt) on the Keck I Telescope at the W. M. Keck Observatory in Hawaii. The spectrometer allows precise measurements of a star's radial velocity (its motion along the line of sight from Earth), which can reveal the presence of planets. The gravitational tug of an orbiting planet causes periodic changes in the radial velocity of the host star. Multiple planets induce complex wobbles in the star's motion, and astronomers use sophisticated analyses to detect planets and determine their orbits and masses.

"It's really hard to detect a planet like this," Vogt said. "Every time we measure the radial velocity, that's an evening on the telescope, and it took more than 200 observations with a precision of about 1.6 meters per second to detect this planet."

To get that many radial velocity measurements (238 in total), Vogt's team combined their HIRES observations with published data from another group led by the Geneva Observatory (HARPS, the High Accuracy Radial velocity Planetary Search project).

In addition to the radial velocity observations, coauthors Henry and Williamson made precise night-to-night brightness measurements of the star with one of Tennessee State University's robotic telescopes. "Our brightness measurements verify that the radial velocity variations are caused by the new orbiting planet and not by any process within the star itself," Henry said.

The researchers also explored the implications of this discovery with respect to the number of stars that are likely to have at least one potentially habitable planet. Given the relatively small number of stars that have been carefully monitored by planet hunters, this discovery has come surprisingly soon.

"If these are rare, we shouldn't have found one so quickly and so nearby," Vogt said. "The number of systems with potentially habitable planets is probably on the order of 10 or 20 percent, and when you multiply that by the hundreds of billions of stars in the Milky Way, that's a large number. There could be tens of billions of these systems in our galaxy."

This research was supported by grants from the National Science Foundation and NASA.

http://www.sciencedaily.com/releases...0929170503.htm
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Old 29-09-10, 11:00 PM
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So: solid surface, livable temperatures, and viable surface gravity: that makes it substantially better than Mars, for our purposes. If it's in the habitable zone, the atmospheric gasses should be the ones we are familiar with; the actual composition should therefore depend on what type of life is present, if any.

It might still be a pretty rough environment; with one face always toward the sun, there might be large convection air currents circulating atmosphere from pole to pole, at very high wind speeds. What sort of influence this would all have on the pattern of any life evolving can only be speculated. Organisms here are heavily influenced by annual and daily cycles, which would not exist there at all. Well I suppose there might be some annual change, but it may well be insignificant.
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Old 01-10-10, 07:35 PM
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Odds of Alien Life on Newly Spotted Exoplanet Are "100 Percent" Says Its Discoverer
By Clay Dillow Posted 09.30.2010 at 11:17 am 31 Comments


Gliese 581 Artist's rendering of the star Gliese 581, with exoplanet Gliese 581c (neighbor to newly discovered Gliese 581g) in the foreground. ESO

As if there wasn't enough excitement swirling around the discovery of a potentially habitable planet circling the star Gliese 581 just 20 light years away, one of the scientists behind yesterday's announcement upped the ante during a press briefing yesterday afternoon, declaring "my own personal feeling is that the chances of life on this planet are 100 percent."

Steven Vogt, a professor of astronomy and astrophysics at UC Santa Cruz, said he had "almost no doubt" (which seems slightly different than 100 percent sure) that life exists on Gliese 581g, an exoplanet Vogt and colleagues discovered via the Keck Observatory that is orbiting in the "habitable zone" surrounding the red dwarf Gliese 581. The "habitable zone" -- a term some scientists are loath to use given the many variables at play in planetary science -- is the sweet spot that is neither too far or too close to the star such that surface water might exist there.

Vogt's statement might make for a bold prediction -- especially given the number of life-bearing planets we've found thus far -- but his statement is more an endorsement for the persistence of life than a declaration that he's found it elsewhere in the galaxy. "Personally, given the ubiquity and propensity of life to flourish wherever it can, I would say, my own personal feeling is that the chances of life on this planet are 100 percent," Vogt said to reporters.

Meaning, even if there is life on the planet as Vogt seems to think there is, there's no telling what kind of life it might be or whether it might be any degree of intelligent -- though an Australian sky-watcher did pick up a mysterious radio signal from nearby Gliese 581e a couple of years ago. Just to be safe, we'd like to extend warmest greetings to our Gliesian readers.

Odds of Alien Life on Newly Spotted Exoplanet Are "100 Percent" Says Its Discoverer | Popular Science
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Old 01-10-10, 07:37 PM
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Linked from "mysterious radio signal", although sadly not that informative about the signal itself.

Watch this space

* Greg Callaghan
* From: The Australian
* May 09, 2009 12:00AM


AFTER you've spent more than 20 years hunting for an alien signal, you think you'd be celebrating if you noticed a mysterious pulse suddenly rising up on your computer readouts. A regular pulse, amid the random clatter of the cosmos, suggests that someone very smart at the other end is sending a message.

But when Ragbir Bhathal, an astrophysicist at the University of Western Sydney, who teaches the only university-based course on SETI (search for extraterrestrial intelligence) in Australia, detected the suspicious signal on a clear night last December, he knew better than to crack open the special bottle of champagne he has tucked away for the history-making occasion.

Instead, he's spent the past few months meticulously investigating whether the unrecognised signature was caused by a glitch in his instrumentation, a rogue astrophysical phenomenon, or some unknown random noise.

Even if he picks up the signal again - he's been scouring the same co-ordinates of the night sky on an almost daily basis since - the scientific rule book dictates he'll need to get it peer-reviewed before he can take his announcement to the world. "And that is a lot of ifs," he concedes.

The hunt for extraterrestrial life has been boosted recently by the discovery last month of a rocky world not unlike our own, about 20 light years away, which its Swiss discoverers have dubbed Gliese 581e, the latest in a long line of planet discoveries during the past decade (350 and counting).

Although Gliese 581e is too close to its host sun to support life, it's the first planet believed to be rocky like our own, a kind of super-hot Earth quite unlike the long line of gas and ice giants discovered to date.

With the launch of NASA's Kepler space telescope in March, specifically designed to detect smaller Earth-like planets, astronomers are confident that the discovery of a blue planet, orbiting in the so-called Goldilocks zone, where liquid water can support life, is edging closer by the day. But it will still be up to ground-based telescopes to confirm the mass of the planet, as space-based telescopes such as the Kepler can only yield its approximate diameter.

The quest of SETI astronomers, however, is not just for the discovery of an Earth-like planet but for life intelligent enough to transmit meaningful signals across vast stretches of space. For more than 40 years, they have been doggedly searching for alien transmissions via radio telescope, tracking tens of millions of radio signals across different sections of the night sky, but so far the results have been, by any scientific standard, dismal.

There has been a handful of false alarms - the detection of short, intense bursts of electromagnetic energy that might be transmitted by an advanced civilisation - but these have been later shown to be caused by other cosmic phenomena, such as quasars.

The belief that an alien civilisation might also be listening to our television and radio signals has also been dashed by the recent discovery that the signals don't, as once thought, reach into deep space: they eventually become so weak that they disappear in the roar of the electromagnetic noise.

That is partly why the OZ OSETI (o for optical) project and a handful of its US counterparts have turned to laser pulse technology in what is the most ambitious effort yet to detect a signal from an alien species. "For an advanced civilisation, radio wave technology would be old hat," Bhathal says. "My strong feeling is that if there are (extraterrestrial intelligence) civilisations out there, they will send the signal by laser pulses or laser flashes."

In 2000, science fiction writer Arthur C. Clarke, a former patron of the Australian SETI project, advised Bhathal to "let the better spectrum, light" drive his search for ET. Bhathal's OZ OSETI project is the only dedicated project for searching for ET in the optical spectrum in the southern hemisphere.

"NASA is already using lasers for space communication and it's not unrealistic to imagine that an extraterrestrial intelligence might be using them as well," Bhathal says.

"In terms of Earth technology today, we have achieved a maximum of 1015 watts of laser power for a brief period, butan advanced civilisation could have lasers with powers of 1025." He admits, however, that our failure to pick up any interstellar signals so far could mean that advanced civilisations are using a communications technique still not discovered on Earth.

"It is risky to judge everything by our own technology," he says.

The search field of the OZ OSETI project is 100 light years from Earth: a short walk around the block in galactic terms, but an area large enough to contain at least 1000 stars and possibly 20 times as many planets.

While the discovery of worlds outside our solar system has given weight to the idea that the universe may be teeming with life - albeit sprinkled across an incomprehensibly wide area - it's the key cosmic numbers that have astronomers in disagreement.

For example, how often do the magic ingredients for life - a rocky planet, located at just the right distance from its sun at justthe right moment in the sun's life - come together?

If the answer is very often, there ought to be lots of planets like our own, and life may be more the rule than a miraculous accident. In 1960, Frank Drake, now a professor of astronomy at the University of Southern California, estimated that there could be up to a million technological civilisations in the Milky Way galaxy alone. But Bhathal believes "we are nowhere near being able to put a sensible figure on how common life may be".

What we do know is that our sun is a perfectly ordinary star in a rotating island of 100 billion stars, the Milky Way galaxy, which in turn is just one of 100 billion or so galaxies in the observable universe. The laws of mathematics weigh heavily in favour of the idea that we are not alone. Moreover, the discovery of more than 300 planets suggests that solar systems such as ours may not be all that unusual. It's very likely that smaller and rockier worlds are more common than the gas giants, which are easier to find because of the greater wriggle they exert in a star's path.

"The low-mass planets are much harder to find because they have a smaller Doppler amplitude," says Chris Tinney of the department of astrophysics at the University of NSW. "It might also mean we are not looking in the right way. But we're now certain that low-mass planets are more common. The Kepler space telescope will no doubt help usfind them."

Tinney explains that while the basic techniques for detecting planets have been around for some time, what's revolutionised the field has been the dramatic technological improvements in spectrographs and telescopic power.

"Planet searching has now become a sexy field and private donors in the US are putting money into it," Tinney says.

Other satellite projects such as the Allen telescope array, named after Paul Allen, the Microsoft co-founder who donated $US13million towards its creation, are also coming online. The array uses an incredible 350 satellite dishes to scan the sky for the faintwhisper of radio signals from celestial objects such as quasars.

There's also the hardware already in space if ET happens to be passing through our neighbourhood. The Pioneer 10 spacecraft, launched in 1972, included an aluminium plate with human figures, a drawing of the planets and an outline of the spacecraft's course. The last, extremely weak signal from this surprisingly robust spacecraft was received in 2006. If it's still around, Pioneer 10 would now be hurtling somewhere in the interstellar void outside our solar system.

With the discovery of more planets, the relatively new science of exobiology, dedicated to the study of extraterrestrial life, has gained the gleam of scientific respectability.

But the field is still trying to overcome the UFO stigma, laments Ain de Horta, a project scientist with the Australian SETI Institute.

"There are still those in the scientific community who look down their noses at us, but that's increasingly unusual these days. There's a growing recognition that this is important science, with the potential to answer one of the most fundamental questions facing humanity. Those who lump us in with the UFO nuts tend not to be scientists," says de Horta.

"We're counting on the physics being the same elsewhere in the universe."

De Horta's institute is, in collaboration with CSIRO's Parkes telescope, scouring radio waves in its search for ET.

"If an alien civilisation has developed technology it's likely to be based on most ofthe same principles as our own. Like us, forexample, they would have discovered radio waves."

Even so, de Horta concedes, life elsewhere in the universe might resemble nothing we know on Earth. It could be moulded by different chemistries, different gravity and different climatic environments.

In any case, it's highly unlikely we'll ever have a face-to-face meeting, as space travel even at Star Trek's warp drive wouldn't get us there in less than thousands of years. A two-way conversation would take decades. And even for that to happen, says de Horta, we would need intelligent life to be reaching its technological prime at the same time as ours and transmitting radio waves at a wavelength that we can detect.

"The whole argument about communication hinges on the longevity of a species and their use of a technology that is recognisable to us," he says.

What all the planet hunters and SETI have in common is a white-hot passion for discovering alien worlds. Bhathal knows that the odds of finding anything are long and the area he is scanning, as big as it is, may still not be extensive enough to yield anything, but he's determined to keep his eyes on the sky.

"There (have) to be other Earth-like worlds. Otherwise what do we have? A whole lot of wasted space."

Watch this space | The Australian
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Old 01-10-10, 07:41 PM
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NASA image comparing the Gliese 581 system with ours.
http://www.nasa.gov/topics/universe/...81_System.html

I've not liked it as the raw image is large.
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Old 02-10-10, 12:17 PM
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There has been a handful of false alarms - the detection of short, intense bursts of electromagnetic energy that might be transmitted by an advanced civilisation - but these have been later shown to be caused by other cosmic phenomena, such as quasars.
I always wondered why they'd be doing this. "Hey I'm bored. Let's spend a ton of money sending meaningless signals to people who'll probably never receive or understand them, and with whom no meaningful communication would be possible even if they did."
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Old 02-10-10, 12:43 PM
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Well, not really. Of course we don't know, but the expectation is that you can start communicating by sending something universally identifiable, like a sequence of prime numbers. They don't occur in nature as a sequence and it would take an intelligence to have found them. With that as a base, we can establish a set of common symbols.

But that's not the only thing we look for either; any suitably artifiical emission would prove the existence of Someone Else.

As to why, partly it depends on how feasible interstellar travel is. If it's not, then signals make a lot of sense. If its very easy, then maybe they wouldn't bother. BNut we can only assume that they will be driven by the same genearl issues that drive us - wondering about life, the universe and everything. Ther existence of another technical species would be a very important data point, and may provide new perspectives.

Meaningful communiicaiton could certainly be established, even if there was a significant time lag. Which would in turn depend on how far away they are. It just wouldn't be like chatting on the phone, ionstead it couyle be constinuous transmissions by botrh sides.
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Old 02-10-10, 12:49 PM
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BNut we can only assume that they will be driven by the same genearl issues that drive us - wondering about life, the universe and everything.
But we don't beam prime numbers into space, and to be honest I can't say that any civilisation that would is one that I'd want anything to do with.
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Old 02-10-10, 01:00 PM
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Well, we have, we just don't do so constantly. Thinsg is though that we are not necessarily looking for messages directed at us - just any message at all. If we identified an alien transmitter, we could then deliberately start to talk.

There are also reasons they might not be deliberately sending.

Earth calling: A short history of radio messages to ET

* 18:00 20 January 2010 by Michael Marshall


The human race first deliberately advertised its existence on the outer panels of space probes, some of which were engraved with codes and images containing information about itself. These immediately prompted arguments about how much we should give away about ourselves.

However, if we really want to break the ice with our cosmic neighbours, it will probably be by sending messages that travel at the speed of light, not at the speed of a Pioneer probe.

A lot of effort has gone into some of the messages, with some researchers even developing an artificial language called Lincos – which so far has not been used in any actual messages.

As part of our special feature marking the 50th anniversary of the search for extraterrestrial life, we round up humanity's radio messages to the stars.

1974: Arecibo message

The first message to be transmitted in the hope of contacting an alien civilisation was quite short, containing just 1679 "bits" of information. This figure was used deliberately: it is the product of two prime numbers, 23 and 73, and if the message is displayed as a 23-by-73 grid it shows a series of simple pictures.

The message was transmitted by the Arecibo radio telescope. It was sent, just once, to the globular cluster M13, where it should arrive in the year 26,974.

1986: Poetica Vaginal

Joe Davis is an artist and a research affiliate at Massachusetts Institute of Technology. In the mid-1980s, he became concerned that no image of humans had been sent into space representing the details of human genitals or reproduction.

So he led a project to transmit the sounds of vaginal contractions towards neighbouring star systems. To do so, he recorded the vaginal contractions of ballet dancers.

The messages were to be sent from MIT's Millstone Hill Radar to Epsilon Eridani, Tau Ceti and two other stars. However, only a few minutes of footage was transmitted before the US air force, which had jurisdiction over the facility, shut the project down.

Nevertheless, the vaginal sounds that were sent will have reached Epsilon Eridani in 1996 and Tau Ceti in 1998. It is unclear what sort of reply we should expect.

1999: Cosmic Call 1

The Cosmic Call messages used the Interstellar Rosetta Stone developed by researchers Yvan Dutil and Stéphane Dumas (PDF). It was based on mathematical and scientific concepts that are thought to be universal, in the hope that any alien who intercepted the messages would understand them. It was followed by short text messages.

The messages were sent using the RT-70 Radio Astronomical Telescope in the Ukraine.

2001: Teen-Age Message

Alexander Zaitsev, a radio engineer at the Russian Academy of Sciences in Moscow and part of the team behind the Cosmic Call messages, was also responsible for this endeavour, in which a group of Russian teenagers sent a message into space.

It used the same transmitter as the Cosmic Call messages, but included analogue information, most notably a concert of electronic music played on the once-revolutionary instrument called the theremin.

The message was sent to six stars, including 47 Ursae Majoris, the first star to be found to have a solar system similar to ours, where any inhabitants will be able to listen to the concert in 2047.

2003: Cosmic Call 2

Four years after it was first transmitted, the Interstellar Rosetta Stone was sent out again, to another five stars. This time, the message included photos and other multimedia files.

Both sets of messages were funded by a company called Team Encounter, which also planned to launch a spacecraft equipped with a solar sail. This would have carried a payload of hair samples, photographs and other items into deep space. However, the company seems to have folded, and the launch never took place.

2005: Craigslist

For the first time, a website was beamed into space. The website in question was the classified listings service Craigslist.

The site was transmitted by a company called the Deep Space Communications Network, which specialises in beaming messages from members of the public into space. It sends its messages into open space, rather than to specific stars, so it is unlikely anybody will pick them up.

2008: Across the Universe

The Beatles song Across the Universe was sent out by NASA in February 2008, to commemorate the 50th anniversary of the agency's founding.

The message was aimed at Polaris, the Pole Star, and should arrive there in 2439. However, Zaitsev criticised the message, noting defects in the method of transmission and also that Polaris is a supergiant star that probably cannot support life.

2008: A Message from Earth

Not content with two Cosmic Calls and a Teen-Age Message, Zaitsev set up a new project called A Message from Earth. This sent out 501 messages selected by a competition on the social networking site Bebo.

As well as half a million members of the public, various celebrities suggested messages, including The X-Files actress Gillian Anderson and the pop band McFly. All these people are now effectively ambassadors for the human race.

The entire capsule was transmitted, again using the RT-70 Radio Astronomical Telescope, towards the planet Gliese 581c, which is so Earth-like it could have liquid water on its surface. The message should arrive in 2028.

2008: Doritos advert

It was a busy year for any extraterrestrial eavesdroppers. In June, radars in the Arctic circle spent 6 hours broadcasting an advert for Doritos into space. The research institute involved, EISCAT, was apparently paid for its efforts by Doritos, hopefully staving off a funding crisis.

Once again, the star 47 Ursae Majoris was chosen as the target of the message.

Later that year, in a second act of intragalactic spamming, the sci-fi movie The Day the Earth Stood Still was beamed towards Alpha Centauri.

2009: Hello from Earth

Last August, Cosmos magazine collected goodwill messages from members of the public and chose the best ones for inclusion in a message called Hello from Earth.

It was sent from the Canberra Deep Space Communication Complex in Australia to the planet Gliese 581d, which is one of the wettest and lightestMovie Camera extrasolar planets known to exist. As the name suggests, it is in the same system as Gliese 581c, which was the recipient of A Message from Earth. The message should arrive in 2029.

2009: RuBisCo message

Artist Joe Davis, who we met previously when he sent recordings of vaginal contractions to nearby stars, returned to the fray on the 25th anniversary of the original Arecibo message.

This time he was a little less racy, transmitting the genetic code for the plant enzyme RuBisCo, which is essential for photosynthesis. RuBisCo is the most abundant protein on Earth, largely because it is so slow and inefficient, so it is certainly representative of life on Earth.

Unlike Poetica Vaginal, this transmission went fairly smoothly – though Davis did have to use his iPhone to get the data into the radio telescope.

Earth calling: A short history of radio messages to ET - space - 20 January 2010 - New Scientist
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Old 02-10-10, 01:02 PM
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Content and structure of the Arecibo message is here.
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