Showing posts with label Earthlike. Show all posts
Showing posts with label Earthlike. Show all posts

Thursday, 27 October 2011

Kepler Analysis Projects One-Third of Sun-Like Stars Have an Earth-Like Planet Orbiting

Kepler Analysis Projects One-Third of Sun-Like Stars Have an Earth-Like Planet Orbiting | Popular Science@import "/files/css/1857af3413d9ad8bd2f9d3926af8ec39.css";@import "/files/css/33f6b7ecb4513ed2fe6c670880a27187.css"; home Login/Register Newsletter Subscribe RSS GadgetsComputersCamerasSmartphonesVideo GamesCarsConceptsHybridsElectric CarsScienceFuture of the EnvironmentEnergyHealthPopSci Eco TourTechnologyMilitaryAviationSpaceRobotsEngineeringDIYProjectsHacksToolsAuto DIYMore From Our Partner: Toolmonger GalleriesVideosColumnsThe GrouseSex FilesGreen Dream Innovation ChallengesHow It WorksFeatures Tweet Digg Kepler Analysis Projects One-Third of Sun-Like Stars Have an Earth-Like Planet Orbiting By Clay Dillow Posted 09.28.2011 at 2:57 pm 27 Comments
Exoplanets Around HD 10180 An artist's rendering. ESO

One of the fun things about astronomy is that we can only know so much through empirical observation, yet we can “know” so much more through enlightened, mathematical guesswork. Such is the nature of the most interesting new science paper I’ve come across on the Internet today. In it, Wesley Traub of CalTech crunches some Kepler data and makes a tantalizing mathematical prediction: one-third of sun-like stars have at least one earth-like terrestrial planet orbiting in their habitable zones.

If that turns out to be the case, that’s big news of course. The habitable zone, or the “goldilocks zone” as it’s often known (not to close to the star, not too far away), is the orbital range where it’s possible for liquid water to exist. Thus, it’s the range where life as we know it could feasibly take root.

Related ArticlesAstronomers Capture First Images of an Exoplanet Orbiting Its Star Largest Known Exoplanet DiscoveredKepler Sightings of New 'Earth-Like' Exoplanets Are Not ConfirmedTagsTechnology, Clay Dillow, exoplanets, goldilocks zone, habitable zone, kepler space telescope, SpaceThe planet-hunting Kepler observatory is designed specifically to seek out planets orbiting distant stars, and thus far its been a boon for exoplanetary science. In 136 days it has scanned some 150,000 target stars looking for the signature wobble exerted on those stars by orbiting satellites. In doing so, it has found 1,235 potential planets.

It’s from that data that Traub has extracted his conclusion. He looked particularly at the stars that are most like our sun--those classified F, G, or K. He then looked at the kinds of planets that are most often found orbiting them and at what ranges they orbit. In his analysis, he notes many interesting (and somewhat expected) things, like the fact that nearly a third of the planets Kepler has found orbit their stars in less than 42 days, putting them too close to be in the habitable zone (this is also because planets closer to their stars are easier for Kepler to see).

Larger terrestrial planets out there in the habitable zone are harder for Kepler to spot, but that doesn’t mean they’re not there. And Traub says his number crunching allows us to get a pretty good idea of how many there should be. Using some math we don’t pretend to understand, he plugged in the numbers for longer orbits--orbits in the habitable zone--into his analysis. The finding: "About one-third of FGK stars are predicted to have at least one terrestrial, habitable-zone planet."

That’s not to say they are inhabited, or that they do have liquid water, or that they even exist. But Traub’s math suggests that they should exist, at least until more data changes the equation. And for now, that spells a lot of potential goldilocks planets. Read the full paper via arXiv.

[Technology Review]

Previous Article: NASA's Falling UARS Satellite Found in Remote South PacificNext Article: Army Developing Drones That Can Recognize Your Face From a Distance 27 Comments Link to this comment eregorn8 09/28/11 at 3:39 pm

Interstellar colonization, anyone?

Link to this comment Lord Elliot the... 09/28/11 at 3:41 pm

I'm going to apply these numbers to the drake equation...
-Spouting a fountain of nonsense since 1995-

Link to this comment mp 09/28/11 at 4:07 pm

I just want them to find the mythical Planet X. And its not the recently found 10th dwarf planet Eris. Once we find planet X, we will found our 2nd earth home, YEA!

Link to this comment pheonix1012 09/28/11 at 4:30 pm

I'm not surprised. three decades ago most astronomers would agree that our existence in the universe was fairly unique. With better scientific equipment and more accurate empirical data, we find that we are not unique, but we (like the multitude of atoms in the universe) are only one of many.

I think most stars have planets around them and a good deal of them (regardless of whether they are FGK category stars) with the potential of harboring life. Thus proving the lack of random order to the universe. We are simply the byproduct of a logical design. Therefore, there must be other worlds like ours. We are seeing living proof through the discovery of terrestrial and jovian worlds.

The most random and/or rare things tend to be extremely improbable to impossible to find.

@mp

Planet X was a concept developed following the discovery of Neptune in 1846. It was born from the possibility that there was in fact another planet outside of its orbit. The search for Planet X did not start until the turn of the 20th Century leading to Pluto's discover in 1930.

Since then Planet X has been the title for any unknown planet beyond the common knowledge of the initial nine. During the previous two decades three plutonian objects were discovered and named within this solar system; two outside of Pluto's orbit in the Kuiper Belt, and one in the Prime Belt between Mars and Jupiter. In succession, there names are Eris, Haumea, and Makemake.

There are possibly several dwarf planets/plutonian objects/planetoids that rest within the Prime and the Kuiper Belt. They are probably not subjected to be named unless used as they possibly range in the thousands. Every planetary discovery following has been extrasolar (i.e. planetary discovery in a foreign star system).

Planet X is a tagline for a sci-fi character that has no clue what planet they're on (i.e. Kurt Russell portraying Col. Jack O'Neil in the 1994 film Stargate).

Link to this comment cholin3947 09/28/11 at 5:49 pm

I'd like to know how broadly "earth-like" is defined. Would Venus and Mars qualify as earth like? Would a planet like Gliese 581 d with a mass of 5.6 to 7.7 times that of Earth qualify as earth like?

Link to this comment mp 09/28/11 at 5:49 pm

pheonix1012,
Ok, ok, there you go being all factual and informative and everything.

Second, I want our science community to find the mythical planet X that is earth sister planet of which earth was seeded with human DNA. You know the science fiction planet X. I adore the Stargate series, don't you? It's real right, planet X?

I do appreciate the extra information you just provided. ;)

Link to this comment aarontco 09/28/11 at 6:28 pm

These planets are far too far away to colonize any time soon. It would be far easier to build on the moon, mars, the moons of mars, or to situate orbital colonies in LaGrange regions and in the asteroid belt(s). Of course, before we do that, there are still plenty of places on Earth too. But off-world colonies have the advantage of spreading humanity's eggs into other baskets, so we can not be so easily wiped out by a single mega-catastrophe. Orbital colonies also have great access to energy and transportation, so long as we can solve major problems, such as adequate radiation shielding, and life support system self-sufficiency.

Link to this comment mp 09/28/11 at 7:16 pm

As we clearly identify these goldilocks, perhaps we could point our satellite dishes at each of them for a while and try to hear some good chatter...

Link to this comment Toran 09/28/11 at 11:19 pm

It's sad that we proceed with presumptions and limit our search to our definition of a habital zone. Even if we want to assume that liquid water is required for life, we cannot be sure of temperatures at these distant locals. Other elements and forces we have yet to experience may be on effect.

Link to this comment inaka_rob 09/28/11 at 11:32 pm

"Ok, ok, there you go being all factual and informative and everything. "
well its is called popular science, not popular science fiction.
but yes thank you phoenix for the info. That is why I thought eris was planet X. it was only "planet X" in the fact that for a brief period they thought it was the 10th planet, hence the X, but not THE mythical planet X. thank you for the explanation.

Link to this comment inaka_rob 09/28/11 at 11:36 pm

@Toran that is a good point. Time and time agian here on Earth the definition of life has surprised us and grown (just look at the taxonmy of "life" it has grown from a 3 kingdom system to a 5 or 6 kingdom system depending on if you study in the USA or the UK. plus it was only a couple decades ago they they realized archea evolved from a totally separate track than other prokaryotes). We have found life in the most improbably places thought for thousands of years to be 100% void of life.
but I suppose they figure these goldilocks zones have a higher probability of life. So far the only life we have found is on a Goldilocks planet. Earth.

Link to this comment pheonix1012 09/29/11 at 8:47 am

@mp

Of course I like science fiction. It logically stands to motivate imaginative youth into academic interest in science.

It's just that by definition Pluto is Planet X, and Planet X is just a traditional verification of the unknown. The term is more common place for candid or satirical statements regarding unspecified worlds. For that matter their are several thousand Planet Xs.

Link to this comment boka 09/29/11 at 11:08 am

It makes more sense to develop high speed space travel to other solar systems that have earth planets than trying to build on any of the planets in our system.

Link to this comment marcoreid 09/29/11 at 11:30 am

I love science and space travel as much as the next guy, and I sure do enjoy daydreaming about what we might be able to do one day.

However... I have to question whether or not this mission's life-cycle cost of US$600 million (including funding for 3.5 years of operation) really is really justified by what we're getting out of it. Great, we get to add a bunch of planets to our long list of known exoplanets. But what does that really do for us anytime in the next few hundred years?

We take that money away from people who work very hard, many of them to make sure they have the essentials of life from day to day. Then we dump it into a project that has no hope of ever doing anything remotely useful for these people. I would think there are some serious ethical issues with that, I know there are in my mind.

That $600 million could provide enough immunizations and basic supplies in 3rd world countries to save hundreds of thousands of children from early and painful deaths. Or it could be used in the US to build thousands of homes for homeless families. Or to provide educations to tens of thousands of kids who then have the potential of becoming scientists themselves, etc.

As fun and exciting as it is to "discover" these planets that we have absolutely no means of getting to for hundreds of years, I'd rather turn more kids into scientists now so that we can more quickly develop the technology to actually visit some of these exoplanets one day.

Link to this comment Nonapod 09/29/11 at 12:05 pm

I wish they'd get a little more specific by what the term "Sun-Like". Do they generally mean all G-Type main-sequence yellow dwarf stars, or a more broader solar analogue? It's significant since something like 90% of the stars out there are cooler red or orange dwarf stars and stars like our Sun are probably more like 5-7% of the total population of stars out there.

Link to this comment JediMindset 09/29/11 at 1:39 pm

@mp
planet x is very real.
youtube.com/watch?v=8S0bj76389U
youtube.com/watch?v=xpPP9Z9LOBU

_________________
The people of the world only divide into two kinds, One sort with brains who hold no religion, The other with religion and no brain.

- Abu-al-Ala al-Marri

Link to this comment dquad 09/29/11 at 2:07 pm

I guess it is time we start constructing neutrino space ships/yawn.

Link to this comment pheonix1012 09/29/11 at 3:18 pm

@Nonapod

The star types they mention in the article are F,G, and K. You gotta read the fine print. That's how they get ya.

@boka

We already know we can survive on a carbon copy of Earth. The real trick is trying to survive in "magnificent desolation."

Besides it's easier to get to these destinations now because they are closer. We still have to develop a relativistically quick means of journeying across stellar distances before we could ever consider mounting a mission outside of the solar system.

@marcoreid

Your sentiment is noble, but we are not going to solve all of the world's problem over night. Besides, there are already organizations that exists to try and solve these problems and they get sufficient government funding which is provided in part by yours truly (the taxpayer). Just be thankful to whatever deity you may pray to that you are fortunate enough to be surrounded by luxuries such as a computer wired to the internet.

As for astronomical research, if you don't have the strategic vision to understand why we do this let me paint you a picture:

Humanity's knowledge in physics has evolved over time and it has achieved a level of mastery over the forces of the spacetime continuum. The once impossible has been proven possible and made into a reality, much as is with many instances in the history of the advancement of human civilization on Earth.

Humanity has achieved the ability to traverse interstellar distances within the blink of an eye. Following the first two successful missions to 581 Gliese d and g, a new mission is underway to HD85512 to verify the planet's potential for harboring life...

Moral of the short story: Making these discoveries now lays the foundation for exploration in the future. To cease such scientific research for lack of long term vision would prove ultimately detrimental to the future, setting us back several hundreds to thousands of years after we develop the means of instellar travel. By the time we develop these methods (especially after several hundreds of years) continued planet hunting will provide us with a library of known star systems that could range from the millions to the billions.

This would be better than the Louis and Clarke approach because space is otherwise featureless. Wondering aimlessly can trap you in a void indefinitely and send you on a trajectory clear of the galaxy without every reaching a star system. In order explore space, you gotta know where your going and the search for destinations starts here on solid ground.

Link to this comment Cookiees453 09/29/11 at 6:45 pm

In May of 2010 6.7 Billion U.S. dollars was being spent in Afghanistan a month.....1 month. This is 600 million dollars over a couple of years.....600 million is pocket change.

Link to this comment Cookiees453 09/29/11 at 6:46 pm

If the government wants to cut cost, cut the war in the middle east. (Yeah, yeah, it's not as simple as that...but whatever)

Link to this comment mp 09/29/11 at 10:37 pm

pheonix1012,
I wish to give you the award of long ranting and commentaries. First I like to say most WOA! YO DUDE, you write a lot of words and stuff! Followed how you write so much and not piss off inaka_rob. He is like such a jealous bandit for the lime light and all? Yo, friend, I am just playing. Be happy! ;)

But back to topic, I was looking at the picture in the article and I wondered why the sun is attacking the planet with these cosmic plasma balls of light and stuff. Does the sun have a beef with the planet?

I hope soon earth points our satellites towards these potentially life giving planets to hear some kind of chatter of communication. Now wouldn't that be cool to hear a new version of Star Wars from a different planet and all!

Seriously, I appreciate the extra information you provide, thanks!

Link to this comment rlb2 09/30/11 at 2:46 am

"About one-third of FGK stars are predicted to have at least one terrestrial, habitable-zone planet."

A total of 22.7 percent of all the stars in our galaxy are class FGK stars, F = 3%, G=7.6%, K=12.1%, it was suggested that 33 percent may be within the habitable-zone.
There are approximately 300 billion, 300,000,000,000, stars in our Milky Way galaxy, 150 billion in the average size Galaxy. There's approximately 200 billion galaxy's in our know universe. That would mean that there are about 22.70 billion, 22,700,000,000 planets, in our Milky Way's habitable-zone or approximately 2.27X10²¹, 2,270,000,000,000,000,000,000 planets in our universe within a class FGK stars rated habitable zone.

Ron Bennett

Link to this comment Oakspar77777 09/30/11 at 9:06 am

Of course, a "habitable zone" is a nebulous term, as things like atmospheric gas can greatly affect the surface temperature of a planet. As well, internal temperature can create a "crust" effect (as is hypothesized about Europa).

Still, 22.7 billion planets in the Milky is not going to give you a good shot at a planet where you can take off your helmet and breathe (we are very fragile in what we breathe).

As for the 600m being spent on vaccines - to what end? Save them from Malaria to insure their starvation of resource competition, or 100m for vaccines on some with 500m for food support? Of course, what about the antibiotic when their population density gives them cholera?

You cannot and will not alieviate human suffering.

Link to this comment pheonix1012 09/30/11 at 11:23 am

@mp

I'm a wealth of knowledge seeking to educate those without. I wouldn't call much of what I do ranting (though a lot of it is). I just legitimize my general platforms with details and evidence. That often takes a lot of words, but might be shorter when spoken.

Link to this comment barclay109 09/30/11 at 12:13 pm

i saw on "The Universe" that there are more than 3 suns, this is interesting, good thing I'm going to college to be an astrophysicist

Link to this comment mp 09/30/11 at 3:40 pm

I really do hope some science community finds intelligent life we earthlings can communicate in my life time!!!

.................................
pheonix1012,
If my wording sounded less complimentary, I like to rephrase myself and just say, I enjoy the additional input you provide and say thanks. ;)

Link to this comment Pasha582 10/02/11 at 2:25 pm

Marcoreid writes: We take that money away from people who work very hard, many of them to make sure they have the essentials of life from day to day.

Not really. Although the poor pay payroll taxes which CAN amount to as high a percent as hedge fund managers pay on their entire salary... The point I want to make is that science is boring, without cool projects like Kepler to stimulate the minds of budding scientists, who would want to get involved in it? What would be the point? We need research like Kepler to whet the appetites and fire the imaginations of children into pursuing careers in science. Without that, who would want to do it?

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October 2011: The Search for Alien Life

This month, we examine all the ways we're looking for extraterrestrial life, within our solar system and beyond.

Plus: Our annual Brilliant 10 list of young researchers, the story behind that "arsenic-based life form found" story, birth control for wildlife, and much more.

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Saturday, 18 June 2011

New SETI survey focuses on Kepler's top Earth-like planets

ScienceDaily (May 16, 2011) — Now that NASA's Kepler space telescope has identified 1,235 possible planets around stars in our galaxy, astronomers at the University of California, Berkeley, are aiming a radio telescope at the most Earth-like of these worlds to see if they can detect signals from an advanced civilization.

The search began on May 8, when the Robert C. Byrd Green Bank Telescope -- the largest steerable radio telescope in the world -- dedicated an hour to eight stars with possible planets. Once UC Berkeley astronomers acquire 24 hours of data on a total of 86 Earth-like planets, they'll initiate a coarse analysis and then, in about two months, ask an estimated 1 million SETI@home users to conduct a more detailed analysis on their home computers.

"It's not absolutely certain that all of these stars have habitable planetary systems, but they're very good places to look for ET," said UC Berkeley graduate student Andrew Siemion.

The Green Bank telescope will stare for about five minutes at stars in the Kepler survey that have a candidate planet in the star's habitable zone -- that is, the planet has a surface temperature at which liquid water could be maintained.

"We've picked out the planets with nice temperatures -- between zero and 100 degrees Celsius -- because they are a lot more likely to harbor life," said physicist Dan Werthimer, chief scientist for SETI@home and a veteran SETI researcher.

Werthimer leads a 30-year-old SETI project on the world's largest radio telescope, the Arecibo receiver in Puerto Rico, which feeds data to SETI@home for a detailed analysis that could only be done on the world's largest distributed computer. He was involved in an early SETI project with the previous Green Bank telescope, which collapsed in 1988, as well as with the Allen Telescope Array (ATA) , which also conducted a broader search for intelligent signals from space run by the SETI Institute of Mountain View, Calif. The ATA went into hibernation mode last month after the SETI Institute and UC Berkeley ran out of money to operate it.

"With Arecibo, we focus on stars like our sun, hoping that they have planets around them that emit intelligent signals," Werthimer said. "But we've never had a list of planets like this before."

The radio dish in rural West Virginia was needed for the new search because the Arecibo dish cannot view the area of the northern sky on which Kepler focuses. But the Green Bank telescope also offers advantages over Arecibo. UC Berkeley's SETI observations piggyback on other astronomical observations at Arecibo, and is limited in the wavelength range it can observe, which centers on the 21 centimeter (1420 MHz) line where hydrogen emits light. These wavelengths easily pass through the dust clouds that obscure much of the galaxy.

"Searching for ET around the 21 centimeter line works if civilizations are broadcasting intentionally, but what if planets are leaking signals like 'I Love Lucy'?" Werthimer said. "With a new data recorder on the Green Bank telescope, we can scan a 800 megaHertz range of frequencies simultaneously, which is 300 times the range we can get at Arecibo."

Thus, one day on the Green Bank telescope provides as much data as one year's worth of observations at Arecibo: about 60 terabytes (60,000 gigabytes) in all, Siemion said. If they recorded a similar chunk of the radio spectrum from Arecibo, SETI@home would be overwhelmed with data, since the Arecibo sky survey observes nearly full time for years on end.

"It's also great that we will completely span the water hole, a canonical place to look for intentional signals from intelligent civilizations," Siemion said.

The water hole is a relatively quiet region of the radio spectrum in the universe and a range of wavelengths not significantly absorbed by material between the stars and galaxies. The water hole is bounded on one end by the 21 cm emissions from neutral hydrogen and on the other by the 18 cm emissions from the hydroxyl ion (OH). Because life is presumed to require the existence of liquid water, and water is composed of hydrogen and hydroxyl, this range was dubbed the water hole and seen as a natural window in which water-based life forms would signal their existence. That makes the water hole is a favorite of SETI projects.

"This is an interesting place, perhaps a beacon frequency, to look for signals from extraterrestrial civilizations," Siemion added.

The 86 stars were chosen from the 1,235 candidate planetary systems -- called Kepler Objects of Interest, or KOIs with the help of Kepler team member Geoffrey Marcy, professor of astronomy at UC Berkeley. UC Berkeley's targets include the 54 KOIs identified by the Kepler team as being in the habitable temperature range and with sizes ranging from Earth-size to larger than Jupiter; 10 KOIs not on the Kepler team's habitable list but with orbits less than three times Earth's orbit and orbital periods greater than 50 days; and all systems with four or more possible planets.

After the Green Bank telescope has targeted each star, it will scan the entire Kepler field for signals from planets other than the 86 targets.

A coarse analysis of the data by Werthimer and his team will be followed by a more thorough analysis by SETI@home users, who will be able to see whether they are analyzing Green Bank data as opposed to Arecibo data. The complete analysis for intelligent signals could take a year, Werthimer said.

"If you extrapolate from the Kepler data, there could be 50 billion planets in the galaxy," he said. "It's really exciting to be able to look at this first batch of Earth-like planets."

The Green Bank telescope is operated by the National Radio Astronomy Observatory, with funds provided by the National Science Foundation (NSF). SETI@home is supported by NSF, NASA and private donations.

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The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by University of California - Berkeley.

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


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Sunday, 12 June 2011

First habitable exoplanet? Climate simulation reveals new candidate that could support Earth-like life

ScienceDaily (May 16, 2011) — The planetary system around the red dwarf Gliese 581, one of the closest stars to the Sun in the galaxy, has been the subject of several studies aiming to detect the first potentially habitable exoplanet. Two candidates have already been discarded, but a third planet, Gliese 581d, can be considered the first confirmed exoplanet that could support Earth-like life. This is the conclusion of a team of scientists from the Institut Pierre Simon Laplace (CNRS, UPMC, ENS Paris, Ecole Polytechnique) in Paris, France, whose study is published in The Astrophysical Journal Letters.

Are there other planets inhabited like Earth, or at least habitable? The discovery of the first habitable planet has become a quest for many astrophysicists who look for rocky planets in the "habitable zone" around stars, the range of distances in which planets are neither too cold nor too hot for life to flourish.

In this quest, the red dwarf star Gliese 581 has already received a huge amount of attention. In 2007, scientists reported the detection of two planets orbiting not far from the inner and outer edge of its habitable zone. While the more distant planet, Gliese 581d, was initially judged to be too cold for life, the closer-in planet was thought to be potentially habitable by its discoverers. However, later analysis by atmospheric experts showed that if it had liquid oceans like Earth, they would rapidly evaporate in a 'runaway greenhouse' effect similar to that which gave Venus the hot, inhospitable climate it has today. A new possibility emerged late in 2010, when a team of observers led by Steven Vogt at the University of California, Santa Cruz, announced that they had discovered a new planet, which they dubbed Gliese 581g, or 'Zarmina's World'. This planet, they claimed, had a mass similar to that of Earth and was close to the centre of the habitable zone. For several months, the discovery of the first potential Earth twin outside the Solar System seemed to have been achieved. Unfortunately, later analysis by independent teams has raised serious doubts on this extremely difficult detection. Many now believe that Gliese 581g may not exist at all. Instead, it may simply be a result of noise in the ultra-fine measurements of stellar 'wobble' needed to detect exoplanets in this system.

Today, it is finally Gliese 581g's big brother -- the larger and more distant Gliese 581d -- which has been shown to be the confirmed potentially habitable exoplanet by Robin Wordsworth, François Forget and co-workers from Laboratoire de Météorologie Dynamique (CNRS, UPMC, ENS Paris, Ecole Polytechnique) at the Institute Pierre Simon Laplace in Paris. Although it is likely to be a rocky planet, it has a mass at least seven times that of Earth, and is estimated to be about twice its size. At first glance, Gliese 581d is a pretty poor candidate in the hunt for life: it receives less than a third of the stellar energy Earth does and may be tidally locked, with a permanent day and night side. After its discovery, it was generally believed that any atmosphere thick enough to keep the planet warm would become cold enough on the night side to freeze out entirely, ruining any prospects for a habitable climate.

To test whether this intuition was correct, Wordsworth and colleagues developed a new kind of computer model capable of accurately simulating possible exoplanet climates. The model simulates a planet's atmosphere and surface in three dimensions, rather like those used to study climate change on Earth. However, it is based on more fundamental physical principles, allowing the simulation of a much wider range of conditions than would otherwise be possible, including any atmospheric cocktail of gases, clouds and aerosols.

To their surprise, they found that with a dense carbon dioxide atmosphere -- a likely scenario on such a large planet -- the climate of Gliese 581d is not only stable against collapse, but warm enough to have oceans, clouds and rainfall. One of the key factors in their results was Rayleigh scattering, the phenomenon that makes the sky blue on Earth. In the Solar System, Rayleigh scattering limits the amount of sunlight a thick atmosphere can absorb, because a large portion of the scattered blue light is immediately reflected back to space. However, as the starlight from Gliese 581 is red, it is almost unaffected. This means that it can penetrate much deeper into the atmosphere, where it heats the planet effectively due to the greenhouse effect of the CO2 atmosphere, combined with that of the carbon dioxide ice clouds predicted to form at high altitudes. Furthermore, the 3D circulation simulations showed that the daylight heating was efficiently redistributed across the planet by the atmosphere, preventing atmospheric collapse on the night side or at the poles.

Scientists are particularly excited by the fact that at 20 light years from Earth, Gliese 581d is one of our closest galactic neighbours. For now, this is of limited use for budding interstellar colonists -- the furthest-travelled human-made spacecraft, Voyager 1, would still take over 300,000 years to arrive there. However, it does mean that in the future telescopes will be able to detect the planet's atmosphere directly. While Gliese 581d may be habitable there are other possibilities; it could have kept some atmospheric hydrogen, like Uranus and Neptune, or the fierce wind from its star during its infancy could even have torn its atmosphere away entirely. To distinguish between these different scenarios, Wordsworth and co-workers came up with several simple tests that observers will be able to perform in future with a sufficiently powerful telescope.

If Gliese 581d does turn out to be habitable, it would still be a pretty strange place to visit -- the denser air and thick clouds would keep the surface in a perpetual murky red twilight, and its large mass means that surface gravity would be around double that on Earth. But the diversity of planetary climates in the galaxy is likely to be far wider than the few examples we are used to from the Solar System. In the long run, the most important implication of these results may be the idea that life-supporting planets do not in fact need to be particularly like Earth at all.

Story Source:

The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by CNRS (Délégation Paris Michel-Ange).

Journal Reference:

Robin D. Wordsworth, François Forget, Franck Selsis, Ehouarn Millour, Benjamin Charnay, Jean-Baptiste Madeleine. Gliese 581d is the first discovered terrestrial-mass exoplanet in the habitable zone. The Astrophysical Journal, 2011; 733 (2): L48 DOI: 10.1088/2041-8205/733/2/L48

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


View the original article here

Monday, 6 June 2011

New SETI survey focuses on Kepler's top Earth-like planets

ScienceDaily (May 16, 2011) — Now that NASA's Kepler space telescope has identified 1,235 possible planets around stars in our galaxy, astronomers at the University of California, Berkeley, are aiming a radio telescope at the most Earth-like of these worlds to see if they can detect signals from an advanced civilization.

The search began on May 8, when the Robert C. Byrd Green Bank Telescope -- the largest steerable radio telescope in the world -- dedicated an hour to eight stars with possible planets. Once UC Berkeley astronomers acquire 24 hours of data on a total of 86 Earth-like planets, they'll initiate a coarse analysis and then, in about two months, ask an estimated 1 million SETI@home users to conduct a more detailed analysis on their home computers.

"It's not absolutely certain that all of these stars have habitable planetary systems, but they're very good places to look for ET," said UC Berkeley graduate student Andrew Siemion.

The Green Bank telescope will stare for about five minutes at stars in the Kepler survey that have a candidate planet in the star's habitable zone -- that is, the planet has a surface temperature at which liquid water could be maintained.

"We've picked out the planets with nice temperatures -- between zero and 100 degrees Celsius -- because they are a lot more likely to harbor life," said physicist Dan Werthimer, chief scientist for SETI@home and a veteran SETI researcher.

Werthimer leads a 30-year-old SETI project on the world's largest radio telescope, the Arecibo receiver in Puerto Rico, which feeds data to SETI@home for a detailed analysis that could only be done on the world's largest distributed computer. He was involved in an early SETI project with the previous Green Bank telescope, which collapsed in 1988, as well as with the Allen Telescope Array (ATA) , which also conducted a broader search for intelligent signals from space run by the SETI Institute of Mountain View, Calif. The ATA went into hibernation mode last month after the SETI Institute and UC Berkeley ran out of money to operate it.

"With Arecibo, we focus on stars like our sun, hoping that they have planets around them that emit intelligent signals," Werthimer said. "But we've never had a list of planets like this before."

The radio dish in rural West Virginia was needed for the new search because the Arecibo dish cannot view the area of the northern sky on which Kepler focuses. But the Green Bank telescope also offers advantages over Arecibo. UC Berkeley's SETI observations piggyback on other astronomical observations at Arecibo, and is limited in the wavelength range it can observe, which centers on the 21 centimeter (1420 MHz) line where hydrogen emits light. These wavelengths easily pass through the dust clouds that obscure much of the galaxy.

"Searching for ET around the 21 centimeter line works if civilizations are broadcasting intentionally, but what if planets are leaking signals like 'I Love Lucy'?" Werthimer said. "With a new data recorder on the Green Bank telescope, we can scan a 800 megaHertz range of frequencies simultaneously, which is 300 times the range we can get at Arecibo."

Thus, one day on the Green Bank telescope provides as much data as one year's worth of observations at Arecibo: about 60 terabytes (60,000 gigabytes) in all, Siemion said. If they recorded a similar chunk of the radio spectrum from Arecibo, SETI@home would be overwhelmed with data, since the Arecibo sky survey observes nearly full time for years on end.

"It's also great that we will completely span the water hole, a canonical place to look for intentional signals from intelligent civilizations," Siemion said.

The water hole is a relatively quiet region of the radio spectrum in the universe and a range of wavelengths not significantly absorbed by material between the stars and galaxies. The water hole is bounded on one end by the 21 cm emissions from neutral hydrogen and on the other by the 18 cm emissions from the hydroxyl ion (OH). Because life is presumed to require the existence of liquid water, and water is composed of hydrogen and hydroxyl, this range was dubbed the water hole and seen as a natural window in which water-based life forms would signal their existence. That makes the water hole is a favorite of SETI projects.

"This is an interesting place, perhaps a beacon frequency, to look for signals from extraterrestrial civilizations," Siemion added.

The 86 stars were chosen from the 1,235 candidate planetary systems -- called Kepler Objects of Interest, or KOIs with the help of Kepler team member Geoffrey Marcy, professor of astronomy at UC Berkeley. UC Berkeley's targets include the 54 KOIs identified by the Kepler team as being in the habitable temperature range and with sizes ranging from Earth-size to larger than Jupiter; 10 KOIs not on the Kepler team's habitable list but with orbits less than three times Earth's orbit and orbital periods greater than 50 days; and all systems with four or more possible planets.

After the Green Bank telescope has targeted each star, it will scan the entire Kepler field for signals from planets other than the 86 targets.

A coarse analysis of the data by Werthimer and his team will be followed by a more thorough analysis by SETI@home users, who will be able to see whether they are analyzing Green Bank data as opposed to Arecibo data. The complete analysis for intelligent signals could take a year, Werthimer said.

"If you extrapolate from the Kepler data, there could be 50 billion planets in the galaxy," he said. "It's really exciting to be able to look at this first batch of Earth-like planets."

The Green Bank telescope is operated by the National Radio Astronomy Observatory, with funds provided by the National Science Foundation (NSF). SETI@home is supported by NSF, NASA and private donations.

Story Source:

The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by University of California - Berkeley.

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


View the original article here

Saturday, 4 June 2011

First habitable exoplanet? Climate simulation reveals new candidate that could support Earth-like life

ScienceDaily (May 16, 2011) — The planetary system around the red dwarf Gliese 581, one of the closest stars to the Sun in the galaxy, has been the subject of several studies aiming to detect the first potentially habitable exoplanet. Two candidates have already been discarded, but a third planet, Gliese 581d, can be considered the first confirmed exoplanet that could support Earth-like life. This is the conclusion of a team of scientists from the Institut Pierre Simon Laplace (CNRS, UPMC, ENS Paris, Ecole Polytechnique) in Paris, France, whose study is published in The Astrophysical Journal Letters.

Are there other planets inhabited like Earth, or at least habitable? The discovery of the first habitable planet has become a quest for many astrophysicists who look for rocky planets in the "habitable zone" around stars, the range of distances in which planets are neither too cold nor too hot for life to flourish.

In this quest, the red dwarf star Gliese 581 has already received a huge amount of attention. In 2007, scientists reported the detection of two planets orbiting not far from the inner and outer edge of its habitable zone. While the more distant planet, Gliese 581d, was initially judged to be too cold for life, the closer-in planet was thought to be potentially habitable by its discoverers. However, later analysis by atmospheric experts showed that if it had liquid oceans like Earth, they would rapidly evaporate in a 'runaway greenhouse' effect similar to that which gave Venus the hot, inhospitable climate it has today. A new possibility emerged late in 2010, when a team of observers led by Steven Vogt at the University of California, Santa Cruz, announced that they had discovered a new planet, which they dubbed Gliese 581g, or 'Zarmina's World'. This planet, they claimed, had a mass similar to that of Earth and was close to the centre of the habitable zone. For several months, the discovery of the first potential Earth twin outside the Solar System seemed to have been achieved. Unfortunately, later analysis by independent teams has raised serious doubts on this extremely difficult detection. Many now believe that Gliese 581g may not exist at all. Instead, it may simply be a result of noise in the ultra-fine measurements of stellar 'wobble' needed to detect exoplanets in this system.

Today, it is finally Gliese 581g's big brother -- the larger and more distant Gliese 581d -- which has been shown to be the confirmed potentially habitable exoplanet by Robin Wordsworth, François Forget and co-workers from Laboratoire de Météorologie Dynamique (CNRS, UPMC, ENS Paris, Ecole Polytechnique) at the Institute Pierre Simon Laplace in Paris. Although it is likely to be a rocky planet, it has a mass at least seven times that of Earth, and is estimated to be about twice its size. At first glance, Gliese 581d is a pretty poor candidate in the hunt for life: it receives less than a third of the stellar energy Earth does and may be tidally locked, with a permanent day and night side. After its discovery, it was generally believed that any atmosphere thick enough to keep the planet warm would become cold enough on the night side to freeze out entirely, ruining any prospects for a habitable climate.

To test whether this intuition was correct, Wordsworth and colleagues developed a new kind of computer model capable of accurately simulating possible exoplanet climates. The model simulates a planet's atmosphere and surface in three dimensions, rather like those used to study climate change on Earth. However, it is based on more fundamental physical principles, allowing the simulation of a much wider range of conditions than would otherwise be possible, including any atmospheric cocktail of gases, clouds and aerosols.

To their surprise, they found that with a dense carbon dioxide atmosphere -- a likely scenario on such a large planet -- the climate of Gliese 581d is not only stable against collapse, but warm enough to have oceans, clouds and rainfall. One of the key factors in their results was Rayleigh scattering, the phenomenon that makes the sky blue on Earth. In the Solar System, Rayleigh scattering limits the amount of sunlight a thick atmosphere can absorb, because a large portion of the scattered blue light is immediately reflected back to space. However, as the starlight from Gliese 581 is red, it is almost unaffected. This means that it can penetrate much deeper into the atmosphere, where it heats the planet effectively due to the greenhouse effect of the CO2 atmosphere, combined with that of the carbon dioxide ice clouds predicted to form at high altitudes. Furthermore, the 3D circulation simulations showed that the daylight heating was efficiently redistributed across the planet by the atmosphere, preventing atmospheric collapse on the night side or at the poles.

Scientists are particularly excited by the fact that at 20 light years from Earth, Gliese 581d is one of our closest galactic neighbours. For now, this is of limited use for budding interstellar colonists -- the furthest-travelled human-made spacecraft, Voyager 1, would still take over 300,000 years to arrive there. However, it does mean that in the future telescopes will be able to detect the planet's atmosphere directly. While Gliese 581d may be habitable there are other possibilities; it could have kept some atmospheric hydrogen, like Uranus and Neptune, or the fierce wind from its star during its infancy could even have torn its atmosphere away entirely. To distinguish between these different scenarios, Wordsworth and co-workers came up with several simple tests that observers will be able to perform in future with a sufficiently powerful telescope.

If Gliese 581d does turn out to be habitable, it would still be a pretty strange place to visit -- the denser air and thick clouds would keep the surface in a perpetual murky red twilight, and its large mass means that surface gravity would be around double that on Earth. But the diversity of planetary climates in the galaxy is likely to be far wider than the few examples we are used to from the Solar System. In the long run, the most important implication of these results may be the idea that life-supporting planets do not in fact need to be particularly like Earth at all.

Story Source:

The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by CNRS (Délégation Paris Michel-Ange).

Journal Reference:

Robin D. Wordsworth, François Forget, Franck Selsis, Ehouarn Millour, Benjamin Charnay, Jean-Baptiste Madeleine. Gliese 581d is the first discovered terrestrial-mass exoplanet in the habitable zone. The Astrophysical Journal, 2011; 733 (2): L48 DOI: 10.1088/2041-8205/733/2/L48

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.


View the original article here