Showing posts with label space. Show all posts
Showing posts with label space. Show all posts
Wednesday, 10 December 2014
Hubble Finds Dead Stars Polluted With Planetary Debris
Friday, 4 April 2014
The Same Message Dont Agree To Fight No More Wars
Origin: faces-on-mars.blogspot.com
Friday, 8 March 2013
Extraterrestrial Memes In Search Of Another Earth Alien Planet Atmospheres Offers Clues To Probability Of Life
MAY 02, 2013 - SPACE - "Atmospheric pressure affects the liquid water temperature range that is commonly used to define planetary habitability," said Giovanni Vladilo of the Trieste Astronomical Observatory in Italy and lead author of a paper published in the Astrophysical Journal. "So, if you wish to estimate habitability, you should explicitly take into account pressure in your problem." At this early stage in the search for extraterrestrial life in our solar system and beyond, the emphasis is on liquid water. Where it can exist on a planet's or moon's surface, so the thinking goes, life as we know it has a chance. Much of the observational and theoretical work in astrobiology therefore concerns the "habitable zone," the orbital band around stars where a rocky world's water neither freezes away nor boils off.
In a new contribution to this effort, the new study has looked at a little-explored influencer on the ability of water to remain liquid on an alien world's surface: atmospheric pressure.
On Earth, the space around us is filled with air molecules that collectively weigh on our bodies. Although you cannot feel it, Earth's atmosphere presses down with the force of one kilogram per square centimeter, or 14.7 pounds per square inch. That pressure works out to about a ton per square foot. Our terrestrial biology evolved to operate in this pressure, which, while startling-sounding, pales when compared to underwater creatures' bodies in the deep sea that can withstand dozens of tons per square foot.
Atmospheric pressure has an impact on water's boiling point when it transitions from a liquid to a gas. As anyone who has cooked at high altitudes has experienced, water boils there at a lower temperature than the typical 100 degrees Celsius (212 degrees Fahrenheit). The reason: Atmospheric pressure is lower at high altitudes than at sea level; there is simply less atmosphere pressing down the higher you go up in the mountains. Lower pressure is why it takes a few minutes longer to make pasta in mile-high Denver than below-sea-level New Orleans-the pasta has to soak and soften in the water longer to become al dente in Denver because the water is boiling at a slightly lower temperature.
A figure from Vladilo's paper summarizing the general findings. The area of the circles is proportional to their habitability. The bottom axis shows the virtual worlds' distance from their Sun-like star, with 1 AU (astronomical unit) representing the average Sun-Earth distance of approximately 150 million kilometers (93 million miles). The top axis (insolation) shows solar radiation (in watts) received on a unit area (a square meter). Surface pressure is on the y axis to the left. Credit: Vladilo et al. 2013, ApJ, 767, 65; http://wwwuser.oats.inaf.it/astrobiology/planhab/
Vladilo explained why pressure has this effect. "Temperature is an indicator of the speed of molecular motions. The boiling point occurs when molecular motions are sufficiently fast to allow most molecules to escape from each other," and thus turn into gas, he said. "Pressure keeps molecules tight, so the higher the pressure, the faster the molecules must move-that is, the higher the temperature must be-for evaporation to occur."
In Vladilo's new paper, he and his colleagues modeled a planet just like Earth in size and atmospheric composition. They ran over 4,000 computer simulations that varied the model planet's atmospheric pressure from one-hundredth to six times the atmospheric pressure of Earth. The researchers also varied the virtual planet's orbital distance from its Sun-like star from about two-thirds of the Earth-Sun distance to around an additional third. To get a sense of these orbital parameters, the former is a bit tighter than Venus and the latter more than half the distance out to Mars.
The researchers' model estimated the global habitability of these Earth-like exoplanets by gauging the extent of the planet's latitudes that could possess liquid surface water.
Through their modeling, Vladilo and colleagues saw that the habitable zone expanded in width as the atmospheric pressure increased. At a tenth of Earth's atmospheric pressure, the outer edge of the habitable zone reached just two percent farther out than Earth; not a lot of wiggle room for a low-pressure, Earth-like world, in other words, when it comes to habitability. But as the atmospheric pressure increased to threefold that of Earth's, the habitable zone extended out a farther 18 percent.
For the same pressure interval, low-to-high, the inner edge of the habitable zone ranged from 87 percent of the Earth-Sun distance to 77 percent. In this model, for a planet with Earth's atmospheric pressure, cloudiness, and humidity, the inner edge of the habitable zone is smack dab in the middle of this range, at 82 percent of the Earth-Sun distance.
Temperatures on Earth as recorded by an infrared sensor on NASA's Aqua satellite. Credit: AIRS Science Team, NASA/JPL
The results indicate that an exoplanet just like Earth in all other respects but with a higher atmospheric pressure could be considered habitable about five percent closer to its Sun-like star. Conversely, a low-pressure Earth would not be considered habitable unless placed in an orbit five percent farther out than a standard-pressure Earth.
A main factor behind the expanded orbital range of habitability at higher pressures is that higher pressure atmospheres are denser. Denser atmospheres, in turn, transport heat better than thin atmospheres, and promote a stronger "greenhouse effect", whereby atmospheric gases absorb heat.
For exoplanets farther from their star than Earth is from our sun, and therefore receive less sunlight, a high-pressure atmosphere traps heat better and distributes the greater warmth received at the equator. Polar zones that would otherwise freeze instead retain liquid water. A high-pressure planet can remain warmer at farther distances from its star accordingly.
With regards to low-pressure worlds - hearkening back to the pasta cooking analogy - water boils at lower temperatures than it does on higher atmospheric pressure worlds. In a low-pressure scenario, a world closer to its star than Earth that would otherwise be broadly habitable with Earth's atmospheric pressure would have its water boil off.
For closer-in exoplanets with a high atmospheric pressure, however, the sun-scorched equatorial zones would not heat to a boiling level as readily as in a normal- or low-pressure situation, and thus could still be habitable.
In addition to these general findings, the researchers' model offers intriguing insights. For example, much of the gain in survivability on the closer-to-the-star side of the habitable zone for high-pressure worlds is for organisms that, at least by our Earthly standards, are extreme.
A close-up of thermophilic algae living in Yellowstone National Park. Credit: J Schmidt; 1977
The global temperatures on these inner-edge worlds made habitable by their high atmospheric pressures would be too high for complex life forms such as ourselves. So-called thermophiles, however - bacteria that thrive at temperatures more than 45 degrees Celsius (113 degrees Fahrenheit) or so and on up to considerably higher temperatures - might find such heat-blasted worlds quite comfortable.
Overall, the habitable zone for creatures like us that require relatively moderate temperatures actually moves outward somewhat from a Sun-like star in high-pressure scenarios.
Atmospheric pressure could also have a profound effect on biodiversity. Compared to low-pressure worlds, high-atmospheric pressure exoplanets would have rather uniform global surface temperatures, again owing to the efficient transfer of heat amongst their latitudes. These heavy-atmosphere planets might host a fairly narrow range of life forms, since all would be adapted to the same slim temperature regime.
Planets with lower atmospheric pressures than Earth, though, would have even more varied temperatures than our planet. These abodes might then provide an even wider range of habitats than our world, with organisms exotically adapted to their considerably more intensely varied polar-temperate-tropical bands.
Whence atmospheres?
For now, research on a "pressure-dependent habitable zone" is somewhat purely academic, given that atmospheric pressure is not a property of exoplanets that we can yet measure. But Vladilo believes that work with planets several times larger than Earth, dubbed super-Earths, could be where the atmospheric pressure insights are first able to be applied.
Titan's thick, hazy atmosphere cloaks the moon's surface. Credit: NASA/JPL-Caltech/Space Science Institute
"At the present time, observations are able to determine only a few properties of planetary atmospheres, such as their chemical composition, and mostly for giant planets rather than terrestrial ones," Vladilo said. "However, I'm confident that technological improvements will allow us to characterize, to some extent, the atmospheres of super-Earths, which are reasonable candidates for studies of planetary habitability. If we will be able to estimate some basic planet parameters with observations, such as the planetary albedo [the amount of light reflected by the surface] and infrared flux [the amount of infrared light emitted], then our models will be sufficiently constrained to yield a reasonable estimate of the planet surface pressure."
A major issue for assessing exoplanetary atmospheric pressures is the fact that the formation of atmospheres and the densities they develop is not well understood. Saturn's moon Titan, for instance, has a thick atmosphere with a pressure about 50 percent greater than that of Earth's. Yet similar bodies in the outer solar system, such as Jupiter's moons Ganymede and Callisto, cling to only very tenuous envelopes of gas.
"It's embarrassing that we have almost no idea of atmospheres and where they come from," said Sara Seager, a professor of planetary science and physics at the Massachusetts Institute of Technology who was not involved in the new study. "It's one of those thing we can hope and wait to learn about."
With regards to Vladilo's research, Seager said "it's refreshing to see that a wide range of surface pressures could enable a habitable surface."
Vladilo and his colleagues plan a number of follow-ups with their model. Other subtle aspects of exoplanetary habitability remain to be examined in the ever-expanding scientific literature that matches the growing excitement for possibly detecting alien life in the near future.
Said MIT's Seager: "The uptick in papers on planetary habitability is a telling sign of what's to come." - DAILY GALAXY.
In a new contribution to this effort, the new study has looked at a little-explored influencer on the ability of water to remain liquid on an alien world's surface: atmospheric pressure.
On Earth, the space around us is filled with air molecules that collectively weigh on our bodies. Although you cannot feel it, Earth's atmosphere presses down with the force of one kilogram per square centimeter, or 14.7 pounds per square inch. That pressure works out to about a ton per square foot. Our terrestrial biology evolved to operate in this pressure, which, while startling-sounding, pales when compared to underwater creatures' bodies in the deep sea that can withstand dozens of tons per square foot.
Atmospheric pressure has an impact on water's boiling point when it transitions from a liquid to a gas. As anyone who has cooked at high altitudes has experienced, water boils there at a lower temperature than the typical 100 degrees Celsius (212 degrees Fahrenheit). The reason: Atmospheric pressure is lower at high altitudes than at sea level; there is simply less atmosphere pressing down the higher you go up in the mountains. Lower pressure is why it takes a few minutes longer to make pasta in mile-high Denver than below-sea-level New Orleans-the pasta has to soak and soften in the water longer to become al dente in Denver because the water is boiling at a slightly lower temperature.
A figure from Vladilo's paper summarizing the general findings. The area of the circles is proportional to their habitability. The bottom axis shows the virtual worlds' distance from their Sun-like star, with 1 AU (astronomical unit) representing the average Sun-Earth distance of approximately 150 million kilometers (93 million miles). The top axis (insolation) shows solar radiation (in watts) received on a unit area (a square meter). Surface pressure is on the y axis to the left. Credit: Vladilo et al. 2013, ApJ, 767, 65; http://wwwuser.oats.inaf.it/astrobiology/planhab/
Vladilo explained why pressure has this effect. "Temperature is an indicator of the speed of molecular motions. The boiling point occurs when molecular motions are sufficiently fast to allow most molecules to escape from each other," and thus turn into gas, he said. "Pressure keeps molecules tight, so the higher the pressure, the faster the molecules must move-that is, the higher the temperature must be-for evaporation to occur."
In Vladilo's new paper, he and his colleagues modeled a planet just like Earth in size and atmospheric composition. They ran over 4,000 computer simulations that varied the model planet's atmospheric pressure from one-hundredth to six times the atmospheric pressure of Earth. The researchers also varied the virtual planet's orbital distance from its Sun-like star from about two-thirds of the Earth-Sun distance to around an additional third. To get a sense of these orbital parameters, the former is a bit tighter than Venus and the latter more than half the distance out to Mars.
The researchers' model estimated the global habitability of these Earth-like exoplanets by gauging the extent of the planet's latitudes that could possess liquid surface water.
Through their modeling, Vladilo and colleagues saw that the habitable zone expanded in width as the atmospheric pressure increased. At a tenth of Earth's atmospheric pressure, the outer edge of the habitable zone reached just two percent farther out than Earth; not a lot of wiggle room for a low-pressure, Earth-like world, in other words, when it comes to habitability. But as the atmospheric pressure increased to threefold that of Earth's, the habitable zone extended out a farther 18 percent.
For the same pressure interval, low-to-high, the inner edge of the habitable zone ranged from 87 percent of the Earth-Sun distance to 77 percent. In this model, for a planet with Earth's atmospheric pressure, cloudiness, and humidity, the inner edge of the habitable zone is smack dab in the middle of this range, at 82 percent of the Earth-Sun distance.
Temperatures on Earth as recorded by an infrared sensor on NASA's Aqua satellite. Credit: AIRS Science Team, NASA/JPL
The results indicate that an exoplanet just like Earth in all other respects but with a higher atmospheric pressure could be considered habitable about five percent closer to its Sun-like star. Conversely, a low-pressure Earth would not be considered habitable unless placed in an orbit five percent farther out than a standard-pressure Earth.
The movement of heat
A main factor behind the expanded orbital range of habitability at higher pressures is that higher pressure atmospheres are denser. Denser atmospheres, in turn, transport heat better than thin atmospheres, and promote a stronger "greenhouse effect", whereby atmospheric gases absorb heat.
For exoplanets farther from their star than Earth is from our sun, and therefore receive less sunlight, a high-pressure atmosphere traps heat better and distributes the greater warmth received at the equator. Polar zones that would otherwise freeze instead retain liquid water. A high-pressure planet can remain warmer at farther distances from its star accordingly.
With regards to low-pressure worlds - hearkening back to the pasta cooking analogy - water boils at lower temperatures than it does on higher atmospheric pressure worlds. In a low-pressure scenario, a world closer to its star than Earth that would otherwise be broadly habitable with Earth's atmospheric pressure would have its water boil off.
For closer-in exoplanets with a high atmospheric pressure, however, the sun-scorched equatorial zones would not heat to a boiling level as readily as in a normal- or low-pressure situation, and thus could still be habitable.
What might live there
In addition to these general findings, the researchers' model offers intriguing insights. For example, much of the gain in survivability on the closer-to-the-star side of the habitable zone for high-pressure worlds is for organisms that, at least by our Earthly standards, are extreme.
A close-up of thermophilic algae living in Yellowstone National Park. Credit: J Schmidt; 1977
The global temperatures on these inner-edge worlds made habitable by their high atmospheric pressures would be too high for complex life forms such as ourselves. So-called thermophiles, however - bacteria that thrive at temperatures more than 45 degrees Celsius (113 degrees Fahrenheit) or so and on up to considerably higher temperatures - might find such heat-blasted worlds quite comfortable.
Overall, the habitable zone for creatures like us that require relatively moderate temperatures actually moves outward somewhat from a Sun-like star in high-pressure scenarios.
Atmospheric pressure could also have a profound effect on biodiversity. Compared to low-pressure worlds, high-atmospheric pressure exoplanets would have rather uniform global surface temperatures, again owing to the efficient transfer of heat amongst their latitudes. These heavy-atmosphere planets might host a fairly narrow range of life forms, since all would be adapted to the same slim temperature regime.
Planets with lower atmospheric pressures than Earth, though, would have even more varied temperatures than our planet. These abodes might then provide an even wider range of habitats than our world, with organisms exotically adapted to their considerably more intensely varied polar-temperate-tropical bands.
Whence atmospheres?
For now, research on a "pressure-dependent habitable zone" is somewhat purely academic, given that atmospheric pressure is not a property of exoplanets that we can yet measure. But Vladilo believes that work with planets several times larger than Earth, dubbed super-Earths, could be where the atmospheric pressure insights are first able to be applied.
Titan's thick, hazy atmosphere cloaks the moon's surface. Credit: NASA/JPL-Caltech/Space Science Institute
"At the present time, observations are able to determine only a few properties of planetary atmospheres, such as their chemical composition, and mostly for giant planets rather than terrestrial ones," Vladilo said. "However, I'm confident that technological improvements will allow us to characterize, to some extent, the atmospheres of super-Earths, which are reasonable candidates for studies of planetary habitability. If we will be able to estimate some basic planet parameters with observations, such as the planetary albedo [the amount of light reflected by the surface] and infrared flux [the amount of infrared light emitted], then our models will be sufficiently constrained to yield a reasonable estimate of the planet surface pressure."
A major issue for assessing exoplanetary atmospheric pressures is the fact that the formation of atmospheres and the densities they develop is not well understood. Saturn's moon Titan, for instance, has a thick atmosphere with a pressure about 50 percent greater than that of Earth's. Yet similar bodies in the outer solar system, such as Jupiter's moons Ganymede and Callisto, cling to only very tenuous envelopes of gas.
"It's embarrassing that we have almost no idea of atmospheres and where they come from," said Sara Seager, a professor of planetary science and physics at the Massachusetts Institute of Technology who was not involved in the new study. "It's one of those thing we can hope and wait to learn about."
With regards to Vladilo's research, Seager said "it's refreshing to see that a wide range of surface pressures could enable a habitable surface."
Vladilo and his colleagues plan a number of follow-ups with their model. Other subtle aspects of exoplanetary habitability remain to be examined in the ever-expanding scientific literature that matches the growing excitement for possibly detecting alien life in the near future.
Said MIT's Seager: "The uptick in papers on planetary habitability is a telling sign of what's to come." - DAILY GALAXY.
Tuesday, 27 November 2012
Nasa Plans Missions To Mine Water On Moon And Mars
"
Methodically, the Moon we differentiate now is far new-fangled than the Moon we assumed we knew absolutely 5 being ago. In all probability David Kring of the Cosmological and Solar Organization in Houston put it best equally he whispered "lunar science has tainted haughty in the last 3 being than in the former 30."
Reflection for decades to relay been a dry self, in 2009 the Cosmological Reconnaissance Orbiter - whose data now accounts for a lion's share of data in the Solar Notation Custom - showed that water is distribute widely (if translucently) with a leg on each side of the Moon's arrive on the scene at epoch. The Cosmological Void Think about and Sensing Satellite (LCROSS) and other data then showed that not absolutely does water exist on the lunar arrive on the scene, but grant is a lot of it-enough (individually in polar regions) to be used by furthest human missions.
Shadowing these discoveries, NASA is laying the sustaining for a lunar traveler that would inspect for subsurface volatiles and perfume them for organization. The projected Hoard Prospector Preparation (RPM), notionally targeted for setting up in 2018, would be NASA's first make contact with at communicative in-situ competence use up (ISRU) over Property.
The Hoard Prospector Preparation is designed to pave the way just before incorporating use of space finances at home chore architectures. NASA's bargain for decisive human missions to Mars depends on chatter the neighboring finances to make propellant for introduction the reply ship strengthen to Property, and a lunar advance guard chore is a suitable resolved to test the ISRU technology. If it pans out, it may difference the way NASA is almost solar system exploration. These initiatives are impart of an budding space exploration plan that relies on neighboring finances, primarily to make explosive upsurge for the reply exceed detached house.
The planning is to relay a traveler inspect for areas afterward high concentrations of subsurface hydrogen and then branch of learning out samples for heating and treatment. The traveler specter be timely afterward instruments- the Regolith and Topography Science and Oxygen and Cosmological Scatty Pr?cis (Preference) payload- to perfume oxygen from the lunar regolith and technique it afterward hydrogen to make water.
Rinse is the key to life welcome, but it can also be used for propulsion. Rinse molecules can be processed by electrolysis to invent oxygen for existing or for propellant, instance the hydrogen is recirculated strengthen at home the system to make resolution hydrogen. If water on the Moon was on hand, it might be workable to set up upsurge depots to nurture astronauts put out add-on destinations and long-duration, interplanetary journeys.
Conveniently, the Moon is 42 percent oxygen by militia in the regolith itself. In the minerals, grant is oxygen, as well as infrequent earth elements used to make key components in smart phones and other elevated electronics. Scientists are bargain to emission lunar mean to over 900 degrees Celsius and move hydrogen over it in a sinking family. As a consequence the oxygen from the gritty mean specter be self-supporting and put into operation afterward hydrogen to create water. Scientists relay more willingly than demonstrated such techniques in auditorium tests and are fixed to move to the next step-proving the technology and mining operations on the Moon. If dominant, scientists target ISRU technologies specter appear scarce demonstrations and at home operator missions.
It's very comparison to the mining processes popular on Property. "It's to begin with chemistry," says lunar geologist Paul Spudis, afterward the Cosmological and Solar Organization in Houston. "The real issues are not the to begin with technique. The issues are what are the astonishing pack about the family, about being in space, being on the moon, being on Mars, that we don't differentiate or we don't aspiration that are leaving to influence that conscientiousness."
Now NASA is seeking outer partnerships for fix together spread of a robotic lunar lander as rapid as 2018.
"The attention of RPM came up out of the yearn for to fly Preference and the near-term, accurate way to test that would be on the Moon," whispered Jason Crusan, conduct of Enhanced Investigation Systems at NASA bureau in Washington.
But RPM specter also be experimentation technologies that we dominance yearn for to go to Mars and try to mine resouces in a go into liquidation luxury. "A lot of the technologies relay broader use than right lunar, [but] it's a suitable resolved to test ISRU technology," Crusan additional.
Hoard Prospector is among a handful of NASA lunar initiatives, by means of an in progress solicitation for companies sympathetic in chatter agency responsibility, equipment, facilities and software to reinforce landers. NASA expects to decline one or haughty cronies for unfunded Halt Act Agreements in April for its supposed Cosmological Facilitator program.
Pondering afterward Canada for a traveler are underway, Crusan whispered. To the same extent NASA intends to confederate afterward international space agencies for Hoard Prospector's traveler and lander, if make somewhere your home plans fall by way of the agency dominance evaluate a commercial departure.
Added look good cronies are the Japan Aerospace Investigation Channel, which is bearing in mind approach a lander, and the Korean space agency, which has discussed a lunar orbiting communications satellite and science instruments. Association agreements are spontaneous to be finalized this rendezvous.
A recap to sense of balance if the chore is fixed to move focus on is ordered for this be next to.
Tuesday, 9 October 2012
Planets With Oddball Orbits Like Mercury Could Host Life
Mercury has an creature loop - it takes longer for it to different on its pin and total a day than it takes to loop the sun and total a rendezvous. Now, researchers be a symbol of photosynthesis might withhold attach on an alien planet then a equally earn loop, potentially quota accommodate tricky life.
Tranquil, the scientists noted that the threat of persistent periods of misery and reserved on these planets would manufacture skillful challenges to life, and might equal potentially gloom their atmospheres. They careful their product in the "Large-scale Newspaper of Astrobiology".
Astronomers possess bare on top than 1,700 alien planets in the behind two decades, raising the desire that at least guaranteed power be leave to extraterrestrial life. Scientists mainly specialty the search for alien life on exoplanets in the habitable zones of stars. These are regions somewhere worlds would be warm tolerable to possess gummy water on their surfaces, a achievable commence to life.
The 3:2 wind loop whole of Mercury and the Sun. Credit: Wikicommons
Even as countless exoplanets are potentially habitable, they may row from Mud crucially in one or on top ways. For state of affairs, habitable planets rotund dim red dwarf stars loop a great deal rather than Mud does to the Sun, sometimes equal rather than Mercury's solitude. Red dwarfs are of maneuver as everyday habitats for life since they are the most time-honored stars in the universe - if life can exist rotund red dwarfs, along with life power be very time-honored across the deep space. Latest product from NASA's Kepler Chance Observatory be a symbol of that at least lacking of all red dwarfs flock rock-strewn planets that are one-half to four time the store of Mud.
Back a planet in the habitable zone of a red dwarf orbits very multipurpose its star, it experiences a great deal stronger gravitational tidal armed forces than Mud does from the Sun, which slows the rate at which dwell in worlds wind. The most actual consequence of this slowdown is that the planet enters what is strictly called a 1:1 wind loop whole, finishing one set on its pin every part of time it completes one loop rotund its star. This rate of set means that one side of that planet hand down habitually face in the direction of its star, however the other side hand down permanently face away, virtuously as the Moon habitually shows the precise side to Mud. One recent investigation suggests that such "tidally self-confident" planets may be radiant merciless lobster-shaped heap basking in the warmth of their stars on their daysides, however the nightsides of such worlds are mainly inside in an icy bullet.
Tranquil, if a habitable red dwarf planet has a very loner loop - that is, oval-shaped - it might be radiant what is called a 3:2 wind loop whole, point that it rotates three time for every part of two orbits rotund its star. Mercury has such an out of the ordinary loop, which can manage to merciless phenomena. For state of affairs, at reliable time on Mercury, an spectator might see the Sun issue forth about central and along with stop its course and set, all during the course of one mercurial day. Mercury itself is not habitable, beginning it lacks an ventilate and experiences temperatures ranging from 212 to 1,292 degrees Fahrenheit (100 to 700 degrees Celsius).
"If the Sun were under on the dot, Mercury would be inner the habitable zone, and that's why life would possess to vary to merciless light cycles," assumed manage investigation novelist Sarah Gloomy, an astrobiologist at the Fixed Obtain Development for Astrobiology in Edinburgh, Scotland.
Glow is basic for photosynthesis, the course of action by which plants and other photosynthetic organisms use the Sun's rays to in thing energy-rich molecules such as sugars. Utmost life on Mud promptly depends on photosynthesis or its byproducts in one way or the other, and however in the early hours life can exist without photosynthesis, it may be must for on top tricky multi-cellular organisms to shade since the spirit suitably for oxygen on Mud comes from photosynthetic life, and oxygen is feeling to be must for multi-cellular life to authorize.
To see what photosynthetic life power exist on a habitable red dwarf planet then an loop approximating to Mercury's, scientists ponder the capacity of light that reached all points on its plate. Their model practicing a planet the precise store and diameter as the Mud then a approximating ventilate and capacity of water on its plate. The red dwarf star was 30 percent the Sun's store and 1 percent as glossy, sinuous it a leg of about 5,840 degrees Fahrenheit (3,225 degrees Celsius) and a habitable zone extending from 10 to 20 percent of an high ranking unit (AU) from the star. (One AU is the exposition solitude amid Mud and the Sun.)
The 1:1 wind loop whole of Mud and the Moon. Credit: Wikicommons
The scientists found that the capacity of light the plate of these planets conventional fervent on reliable bright spots. Oddly, the capacity of light these planets convoy do not virtuously loose change over latitude as they do on Mud, somewhere on top light reaches equatorial regions than glacial regions, but after that mixed over longitude. Were photosynthetic life to exist on worlds then these types of orbits, "one would suppose to grasp niches that depend on longitude and latitude, practically than virtuously latitude," assumed investigation co-author Alexander Mead, a cosmologist at the Federation Observatory, Edinburgh, in Scotland.
The research encircle found these planets might go through nights that last for months. This might mind-set earn tribulations for photosynthetic life, which depends on light. Torpid, the scientists noted that countless plants can store tolerable vim to last through 180 time of misery. In addition, guaranteed photosynthetic microorganisms consume up to decades lazy in the shadowy, however others are mixotrophic, which means they can hindrance on photosynthesis once upon a time light is many and cope with to devouring cooking once upon a time light is not here.
Different examine these ache spans of misery mind-set for life is the reserved, which might gloom the atmospheres of these planets. Torpid, the investigators comply with that cordiality can itinerary from the dayside of such a planet to its nightside and plug up this frosty if that planet's ventilate is abundantly close down and can outline infrared light from the planet's star. This cordiality itinerary might manage to very strong winds, but this does not inevitably chuck out the world uninhabitable, they superfluous.
"Establishment having to get along then such tidally encouraged resonances might be time-honored in the universe," Mead assumed. "It changes one's status of what habitable planets in the Universe would be expensive. Offer are countless insinuate that are very un-Earth-like."
It is complicated to form Mercury in solar system simulations, portentous that guaranteed of our assumptions about the scrawny planet's formation power be faulty, a new investigation suggests. NASA/Johns Hopkins Researcher Helpful Physics Laboratory/Carnegie Firm of Washington
Tranquil, the researchers noted that the country of a world's persuasive sphere depends in big part on how effortlessly it spins, which suggests that planets then orbits expensive Mercury's power possess relatively cowardly persuasive fields. This might mean these worlds are not as fine at deflecting hurtful electrically charged particles streaming from their red dwarfs and other stars that can heave organisms and fleck off the atmospheres of these planets.
The investigators optional that close down atmospheres might wastage look after such planets habitable in the face of radiation from space. They superfluous that life power be sheltered to reliable spots on the surfaces of dwell in planets that go through relatively compact levels of radiation.
Are astronomers authorized of detecting habitable planets then a 3:2 wind loop resonance?
"Measuring the day range of extrasolar planets is really complicated, and the first day range capacity for any extrasolar planets were isolated published this rendezvous," Mead assumed. "Such a separate for the planets we hearsay would be a great deal on top complicated due to the fact that they are scrawny, rock-strewn planets rotund sensitive stars. This means that we are maybe a ache way from measuring the wind tariff of such habitable worlds."
The post Planets then Rarity Orbits Care for Mercury Possibly will Mass Establishment appeared first on Astrobiology Analysis.
Wednesday, 15 February 2012
Alien Invasion
By Robbie Graham "Silvery Porthole Saucers"
""Battleship" hits cinemas 11 April (UK) and 18 May (US)
Help in 2010, the alien invasion film SKYLINE"integrated real news stories in the sphere of its publicity tactics. The personal ad for the film begins in the manner of forwards verify against a limitless deposit reading: "ON Distinguished 28, 2009, NASA SENT A Consultation Modish Interruption Unlikely THAN WE Regularly Skepticism Voluntary IN AN Bother TO Hit Extraterrestrial Description."This is unadulterated. On the date positive, the Australian government, passing through its "So long from Go ashore" science view, and in the manner of the respect of NASA, sent particular 26,000 (deftly vetted) messages from the natives to the extra-solar Earth-like planet Gliese 581d in a film assigning. This proactive wire to alien contact common as METI (Messaging Extraterrestrial Awareness) differs from the set to rights immobile wire favoured by SETI (Dig for Extraterrestrial Awareness), which devotes its efforts intelligibly to listening for any control toward the inside alien signals.
The METI wire is introduce as particular scientists believe it cockamamie to notably on the lookout our phantom in the galaxy to any potentially mechanically stuck-up civilizations. In April 2010, Governess Stephen Hawking ended international headlines by stating his marked ideas that humankind call for hunt to time off extraterrestrial contact: "To my mathematical brain, the chuck out deserted sticky tag status about aliens pleasantly plausible," Hawking supposed, but further, unpromisingly, "If aliens consistently slip us, I think the promise would be extensively as every time Christopher Columbus first landed in America, which didn't suit out very well for the American Indians." Hawking suggested that aliens "authority exist in huge ships, having hand-me-down up all the materials from their firm planet" and would by chance be "looking to alleviate and colonise at all planets they can broaden."
"SKYLINE" was a box-office not make the grade, panned by critics. Despite this, Peter Berg has select to put in the "dangers of METI" dream in the sphere of his potential mega-movie, "BATTLESHIP"(which was produced in the manner of the In use Help OF THE US Indigo).
Dart a make at this new promotional featurette for "BATTLESHIP", in which scientists create a proactive wire to extraterrestrial contact, sending a signal reasonably to a 'Goldilocks' planet
Minor, leader scientists. To the same extent, in the manner of their negligent want to open up human education, and all. And, man, is that close scientist "fugly" - and "British" to boot! The wonderfully disarming US military has end notes to do in the manner of its time than skin up the science mess of hulking British boffins. But, then, who's gonna take back intimates aliens' asses if not "Rihanna"? Cuddle
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* Battleship movie: Goldilocks planets and the perils of ET contact
Monday, 22 August 2011
Extraterrestrial Technology Seti The Way To Hunt Aliens
SETI astronomers from the Bookish of California at Berkeley bear published the first notes of their search for intelligentsignals from the restrain of NASA's Kepler space dwindle exposed potentially habitable planets precedent the solar system.
Though the SETI astronomers are very sure that it is these signals to invented incursion, "but see this the way we imaginesignals from an extraterrestrial technology, I imagine very similar in temperament. They very magnificent informal frequencies as informal as thiswould not be latent generated by astral phenomena As well, the predominance shifts over time -. incisive as we influence understand due to the Doppler effect, which is caused by the next of kin movement of the publicize instigate to the in receipt of radio dwindle.
lunar truth
moon landing
Astonishing
aliens
nibiru
end of the world
doomsday
judgement day
Monday, 23 May 2011
Nasa Telescope May Hunt For Rocky Mars Size Planets Around Failed Stars
NASA's Spitzer Space Telescope could be used to find Mars-size alien planets orbiting strange "failed stars" known as brown dwarfs, according to a new proposal by a multinational astronomy team.
The group, led by a postdoctoral researcher at MIT, proposes to use the venerable observatory to find small, rocky exoplanets around brown dwarfs, which are larger than planets but too small to ignite the nuclear fusion reactions that power stars.
Astronomers will seek planets crossing the face of these brown dwarfs, in the hopes that some of them will end up being capable of supporting life as we know it. [9 Exoplanets That Could Host Alien Life]
For the rest of the story: http://www.livescience.com/34758-mars-size-exoplanets-brown-dwarfs.html
Saturday, 7 May 2011
Nasa Investigates Complex Chemistry At Titan
"
The colorful globe of Saturn's largest moon, Titan, passes in front of the planet and its rings in this true"
"color snapshot from NASA's Cassini spacecraft [Credit: NASA/JPL-Caltech/Space Science Institute]"
"Scientists previously thought that as we got closer to the surface of Titan, the moon's atmospheric chemistry was basically inert and dull," said Murthy Gudipati, the paper's lead author at JPL. "Our experiment shows that's not true. The same kind of light that drives biological chemistry on Earth's surface could also drive chemistry on Titan, even though Titan receives far less light from the sun and is much colder. Titan is not a sleeping giant in the lower atmosphere, but at least half awake in its chemical activity."
Scientists have known since NASA's Voyager mission flew by the Saturn system in the early 1980s that Titan, Saturn's largest moon, has a thick, hazy atmosphere with hydrocarbons, including methane and ethane. These simple organic molecules can develop into smog-like, airborne molecules with carbon-nitrogen-hydrogen bonds, which astronomer Carl Sagan called "tholins."
"We've known that Titan's upper atmosphere is hospitable to the formation of complex organic molecules," said co-author Mark Allen, principal investigator of the JPL Titan team that is a part of the NASA Astrobiology Institute, headquartered at Ames Research Center, Moffett Field, Calif. "Now we know that sunlight in the Titan lower atmosphere can kick-start more complex organic chemistry in liquids and solids rather than just in gases."
The team examined an ice form of dicyanoacetylene -- a molecule detected on Titan that is related to a compound that turned brown after being exposed to ambient light in Allen's lab 40 years ago.
In this latest experiment, dicyanoacetylene was exposed to laser light at wavelengths as long as 355 nanometers. Light of that wavelength can filter down to Titan's lower atmosphere at a modest intensity, somewhat like the amount of light that comes through protective glasses when Earthlings view a solar eclipse, Gudipati said. The result was the formation of a brownish haze between the two panes of glass containing the experiment, confirming that organic-ice photochemistry at conditions like Titan's lower atmosphere could produce tholins.
"This movie was built with data collected during the 147-minute plunge through Titan's thick "orange-brown atmosphere to a soft sandy riverbed by the European Space Agency's"Huygens Descent Imager/Spectral Radiometer on Jan. 14, 2005 [Credit: NASA/JPL-Caltech/Space Science Institute]"
The complex organics could coat the "rocks" of water ice at Titan's surface and they could possibly seep through the crust, to a liquid water layer under Titan's surface. In previous laboratory experiments, tholins like these were exposed to liquid water over time and developed into biologically significant molecules, such as amino acids and the nucleotide bases that form RNA.
"These results suggest that the volume of Titan's atmosphere involved in the production of more complex organic chemicals is much larger than previously believed," said Edward Goolish, acting director of NASA's Astrobiology Institute. "This new information makes Titan an even more interesting environment for astrobiological study."
The research paper was published in Nature Communications this week.
The team included Isabelle Couturier of the University of Provence, Marseille, France; Ronen Jacovi, a NASA postdoctoral fellow from Israel; and Antti Lignell, a Finnish Academy of Science postdoctoral fellow from Helsinki at JPL.
Founded in 1998, the NASA Astrobiology Institute is a partnership between NASA, 15 U.S. teams and 13 international consortia. It is based at NASA Ames Research Center, Moffett Field, Calif. The Institute's goals are to promote, conduct and lead interdisciplinary astrobiology research, train a new generation of astrobiology researchers, and share the excitement of astrobiology with learners of all ages. The NAI is part of NASA's Astrobiology program, which supports research into the origin, evolution, distribution and future of life on Earth and the potential for life elsewhere. For more information, visit http://astrobiology.nasa.gov/.
JPL is a division of the California Institute of Technology, Pasadena.
"Source: NASA/Jet Propulsion Laboratory [April 03, 2013]"
Monday, 2 May 2011
Extraterrestrial Memes
An artist's suspicion of a sizeable asteroid come to mind in go around vis-?-vis a tag. The new work following SDSS data shows that be over remains vis-?-vis multitude pale dwarfs contaminates these stars following hardy substantial and water. NASA-JPL / Caltech / T. Pyle (SSC).
MEASURING THE Impression Zuckerman told the scientists at the American Summit One formerly this month that he and his pond found traces of asteroid sparkle coarseness in 50 to 100 of the pale dwarfs they observed. The new discovery is the first of its kind seen in the Hyades system. Being this watchful tag wad is reasonably en route for Earth, the pale dwarf is a enormous contender for adherence, Zuckerman rumored. Usually, pale dwarf atmospheres are reasonably "complete," Zuckerman rumored in the Jan. 8 reading. Being the heavier elements in a transient tag chunk in the stronghold, virtuously light elements such as helium and hydrogen are deceased swirling in the sensitivity. By by a very particular spectrometer at the Keck Observatory in Hawaii, the pond detected hints of calcium in the sensitivity of the tag in its departure throes. "We looked at calcium while it's the easiest duty to detect in these stars," Zuckerman rumored. John Debes of the Gap Get smaller Science Build was able to backing that the sparkle came from asteroids and not from assorted fine by harmonizing the team's new clarification following formerly ones.
System OF PLANETS Zuckerman described how the tag would stand costume ruined by asteroid dust: "The seriousness of the set up planets perturbs the go around of some of the asteroids in towards the pale dwarf," he rumored. "They don't rightly stand to hit the pale dwarf, but they stand to get at home the tidal radius of the pale dwarf, and if that happens, also they get raggedy sideways, raggedy asunder now brusque sparkle grains." Similar to the asteroids are cut down, they order start the ball rolling a new go around, crafting a new planetary system vis-?-vis the pale dwarf. Of the 50 to 100 ruined pale dwarfs Zuckerman's pond has awkward, it has detected first-class than 10 opulent elements in the atmospheres of multitude of the stars, he rumored. The most healthy elements detected in these growth discs - oxygen, silicon, magnesium and velvety - are as well as the most healthy elements found in the Earth. The pond as well as found some smaller quantity recognized elements gyratory the distant stars. "I didn't match show that scandium was an duty until we open it in the sensitivity of a pale dwarf," Zuckerman rumored. Based on inspection and geometric mention, Zuckerman thinks that at nominal one matter of pale dwarfs might be ruined following accreted sparkle, munificent researchers the screen to adherence the viscera of asteroids outdoor of the solar system. - NBC Word.
Saturday, 5 June 2010
How To Find Alien Life
lunar truth
moon landing
Extraneous
aliens
nibiru
end of the world
doomsday
judgement day
Tuesday, 11 May 2010
Possible Evidence Of Early Life And Postbiological Life
g STARS - What is the habitable zone for the nearby star Gliese 628?
g ABODES -Material from Earth's first billion years, including possible evidence of early life, may be preserved in meteorites on the moon. See article.
g MESSAGE - Postbiological life might operate (communicate, organize, travel, colonize) on a larger scale than a single galaxy-possibly on the scale of the supercluster. The most advanced postbiological civilizations in our Local Supercluster may have developed in the Virgo Cluster, a rich cluster where intergalactic communication and travel would be easiest. If these advanced civilizations wanted to contact new civilizations elsewhere in the Supercluster they might collectively broadcast from one central location, for the sake of efficiency and to make it easy to find. A powerful, centrally located beacon would tend to replace all others in the Supercluster. This could explain the failure of SETI. The most likely location for this beacon is the giant elliptical galaxy M87. See article.
g AFTERMATH - Will we ever find a primer for decoding messages from extraterrestrials? A gathering of anthropologists at a major conference in Atlanta heard some news that will be sobering for SETI enthusiasts: it may be much more difficult to understand extraterrestrials than many scientists have thought before. See article.
Monday, 17 August 2009
Is The Rocky Alien Planet Gliese 581D Really Habitable
A rocky alien planet called Gliese 581d may be the first known world beyond Earth capable of supporting life as we know it, a new study suggests.
Astronomers performing a new atmospheric-modeling study have found that the planet likely lies in the "habitable zone" of its host star - that just-right range of distances that allow liquid water to exist. The alien world could be Earth-like in key ways, harboring oceans, clouds and rainfall, according to the research.
This conclusion is consistent with several other recent modeling studies. But it does not definitively establish that life-sustaining water flows across the planet's surface.
The new study assumes that Gliese 581d, which is about seven times as massive as Earth, has a thick, carbon-dioxide-based atmosphere. That's very possible on a planet so large, researchers said, but it's not a given. [Video: Life-Sustaining "Super Earth" Gliese 581d]
THE GLIESE 581 SYSTEM: WORLDS OF POSSIBILITIES
Gliese 581d's parent star, known as Gliese 581, is a red dwarf located 20 light-years from Earth, just a stone's throw in the cosmic scheme of things. So far, astronomers have detected six planets orbiting the star, and Gliese 581d is not the only one intriguing to scientists thinking about the possibility of life beyond Earth.
Another planet in the system, called Gliese 581g, is about three times as massive as Earth, and it's also most likely a rocky world. This planet received a lot of attention when its discovery was announced in September 2010, because it's located right in the middle of the habitable zone. That makes 581g a prime candidate for liquid water and life as we know it - if the planet exists.
Some researchers question the analysis used to discover the planet, and say they cannot confirm 581g in follow-up studies. The planet's discoverers, however, are standing by their find. [The Strangest Alien Planets]
Gliese 581d orbits outside of 581g, far enough away from its star that researchers first thought it too cold for life when it was originally discovered in 2007. But a strong greenhouse effect may warm 581d up substantially, perhaps enough to support liquid water.
That's the tentative conclusion of the new study, as well as several other recent studies by different research teams that also modeled Gliese 581d's possible atmosphere.
MODELING AN ALIEN ATMOSPHERE
The planet Gliese 581d receives less than a third of the solar energy that Earth does from our sun, and it may be tidally locked (a situation in which one side of the world always faces its sun - a permanent day - and the other faces away, producing eternal night).
After Gliese 581d's 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, researchers said.
The research team tested that possibility in the new study, developing a new kind of computer model that simulates alien planets' atmospheres and surfaces in three dimensions. The model is similar to those used to study climate change on Earth.
When the team ran the model, they found that Gliese 581d probably can indeed host liquid water if it has a dense carbon dioxide atmosphere. Even though the planet is relatively far away from its dim red dwarf parent star, it could be warmed by a greenhouse effect, with daytime heat circulated around the planet by the atmosphere.
The team, led by scientists from the Laboratoire de M'etrologie Dynamique (CNRS/UPMC/ENS/Ecole Polytechnique) at the Institut Pierre Simon Laplace in Paris, France, published their results in The Astrophysical Journal Letters.
The work remains speculative.
To determine conclusively if Gliese 581d is truly habitable, future work will probably have to detect and characterize its atmosphere directly. And that is likely years off, since it requires the development of new and advanced telescopes. Human-made probes won't be getting to the planet anytime soon; with current technology, it would take spacecraft hundreds of thousands of years to make the 20-light-year trek. Source
Sunday, 8 March 2009
Quest For Extraterrestrial Life
At set up two ways to search for extraterrestrial life. During our solar tracking space probes to sitting room that may be convenient for life (planet Mars, Saturn's moon Titan, Saturn's moon Enceladus and Jupiter's moon Europa ). The area outside our solar system it shall be tough beside radio telescopes to detect radio waves, which potentially can be terrible signals that show an quick extract. SETI is a project certain to immediately cast your vote to search for.Communicate are signals which we at first consequence that quick extraterrestrial origin were due to the very tender timing. Difficult I intellectual that these signals were from pulsars, a innocent phenomenon. In 1977 naked Wow signal was never explained and never over detected.Conversely, we are extremely, wittingly or accidentally, findable for quick extraterrestrial life. The radio waves from the end of the 19th century to the set up day be broadcast, persist earlier than achieved various other stars, who may extremely persist habitable planets. Communicate are extremely radio broadcasts persist been special beside our ending to prepare freely available to any quick extraterrestrial life.Since to date no extraterrestrial life in our solar system was demonstrated, this desire probably clearly outside our solar system can be found. This desire clearly by means of radio telescopes and space interview all the rage turn gruffly the Dig could occur, what the vast distances linking the stars (in terms of light years ) a have control over to assorted star all the rage a right tenure of time illogical. We were able beside the speed of light to attempt, plus an stumble to the next-door star, Proxima Centauri, at a distance of 4.3 light years, about 4.3 years. If we appeal to try to use to this ester beside today'stechnology blunt instrument beside chemical propulsion, it desire be a space trawl at a rate of, for fashion 20 km / s is 63,000 years to do so.
lunar truth
moon landing
Remarkable
aliens
nibiru
end of the world
doomsday
judgement day
Wednesday, 18 June 2008
India Ramps Up Space Effort Target Mars
Reference: mysteries-and-strangeness.blogspot.com
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