Mostrando entradas con la etiqueta Planet Kepler-452b. Mostrar todas las entradas
Mostrando entradas con la etiqueta Planet Kepler-452b. Mostrar todas las entradas

domingo, 20 de diciembre de 2015

NASA : Meanwhile, in a galaxy not so far, far away….- Mientras tanto, en una galaxia no tan lejos, muy lejos ...

Hola amigos:  A VUELO DE UN QUINDE EL BLOG., Las creaciones de la fantasía del universo "Star Wars" son sorprendentemente similares a planetas reales en nuestra propia galaxia, la Vía Láctea. Un super Tierra en congelador? Piense hielo planeta "Hoth." Y ese mundo distante con dobles puestas de sol no puede dejar de citar a los pensamientos de arena "Tatooine."
More information.....
http://www.nasa.gov/feature/jpl/meanwhile-in-a-galaxy-not-so-far-far-away

Scene from the movie Star Wars: The Force Awakens
A scene from 'Star Wars: The Force Awakens.'
Credits: Disney
Artist's concept of Kepler-452b
The glittering city lights of Coruscant, the Star Wars core world, might have evolved on an older, near Earth-size planet like Kepler-452b. This real-life Earth cousin exists in a system 1.5 billion years older than Earth, giving any theoretical life plenty of time to develop an advanced technological civilization.
Credits: NASA/Ames/JPL-Caltech
Artist's concept of exoplanet CoRoT-7b
Molten exoplanet CoRoT-7b is a good analog for the Star Wars sizzling lava planet Mustafar. While you won’t see any lightsaber duels on CoRoT-7b, the planet’s temperature of 3,600 degrees Fahrenheit (1,982 Celsius) isn’t far off from the fictional magma mining station.
Credits: ESO/L. Calçada
Artist's concept of WASP-47
Fictional Hoth is a frozen tundra that briefly serves as a base for the hidden Rebel Alliance. It’s also the nickname of real exoplanet OGLE-2005-BLG-390, a cold super-Earth whose surface temperature clocks in at minus 364 degrees Fahrenheit (minus 220 Celsius).
Credits: NASA, ESA and G. Bacon (STScI)
587837main_Kepler16_transit_art2_full.jpg
Years before science discovered planets orbiting two stars, Star Wars showed Luke Skywalker facing a twin sunset on his home world Tatooine. Now NASA telescopes have found multiple planets orbiting binary star systems, including Kepler-16b.
Credits: NASA/JPL-Caltech
607694main_Kepler22bArtwork_full.jpg
Super-Earth Kepler-22b may not hide an army of clones, but it may resemble the grey water-world of Kamino with its own super ocean. While the true composition of Kepler-22b’s surface is unknown, an ocean world about the size of Earth could be comfortably habitable.
Credits: NASA/Ames/JPL-Caltech
Artist's concept of a planetary system
Rubble in space can signal either birth or death: the formation of a planetary system or the end of planet. For Alderaan, the Death Star’s fatal strike transformed the planet into an asteroid field. In this artist’s concept, the swirling disk of debris is part of the formation of a new star system, and plays a key role in the creation of new planets.
Credits: NASA/JPL-Caltech
 
 
The fantasy creations of the "Star Wars" universe are strikingly similar to real planets in our own Milky Way galaxy. A super Earth in deep freeze? Think ice-planet "Hoth." And that distant world with double sunsets can't help but summon thoughts of sandy "Tatooine."

No indications of life have yet been detected on any of the nearly 2,000 scientifically confirmed exoplanets, so we don't know if any of them are inhabited by Wookiees or mynocks, or play host to exotic alien bar scenes (or even bacteria, for that matter).

Still, a quick spin around the real exoplanet universe offers tantalizing similarities to several Star Wars counterparts.

A more ancient Earth?

The most recently revealed exoplanet possessing Earth-like properties, Kepler-452b, might make a good stand-in for Coruscant -- the high-tech world seen in several Star Wars films whose surface is encased in a single, globe-spanning city. Kepler-452b belongs to a star system 1.5 billion years older than Earth's. That would give any technologically adept species more than a billion-year jump ahead of us. The denizens of Coruscant not only have an entirely engineered planetary surface, but an engineered climate as well. On Kepler-452b, conditions are growing markedly warmer as its star's energy output increases, a symptom of advanced age. If this planet (which is 1.6 times the size of Earth) were truly Earth-like, and if technological life forms were present, some climate engineering might be needed there as well.

City in the sky

Mining the atmospheres of giant gas planets is a staple of science fiction. NASA, too, has examined the question, and found that gases such as helium-3 and hydrogen could be extracted from the atmospheres of Uranus and Neptune. Gas giants of all stripes populate the real exoplanet universe; in "The Empire Strikes Back," a gas giant called Bespin is home to a "Cloud City" actively involved in atmospheric mining. The toadstool-shaped city provides apparent refuge for a fleeing Princess Leia and company -- at least until Darth Vader wreaks his usual havoc.

Many of the gas giants found so far by instruments such as NASA's Kepler Space Telescope are so-called "hot Jupiters" -- star-hugging behemoths far too thoroughly barbecued to be proper sites for floating cities. One recent discovery, however, shows that gas "exogiants" can orbit their stars at distances remarkably similar to those in our solar system. An international astronomical team discovered a twin of our own Jupiter, orbiting its star at about the same distance as Jupiter is from the sun. The star, HIP 11915, is about the same age and composition as our sun, raising the possibility that its entire planetary system might be similar to ours. This not-so-hot Jupiter, about 186 light-years away from Earth, was detected using the 11.8-foot (3.6-meter) telescope at La Silla Observatory in Chile.

Bespin's atmospheric layers include a band of breathable air, ideal for floating cities. In our galaxy, emerging technology allows us to read out the components of real exoplanet atmospheres -- including gas giants (though so far none show signs of habitable layers). And tasting the atmospheres of smaller, rocky, potentially habitable exoplanets soon could be within reach. Astronomers using K2, the second planet-finding mission of the Kepler space telescope, recently detected three such planets orbiting a nearby dwarf star. The starlight shining through the atmospheres of these planets could reveal their composition in future observations.  

Turn up the heat

The planet Mustafar, scene of an epic duel between Obi-Wan Kenobi and Anakin Skywalker in "Revenge of the Sith," has a number of exoplanet counterparts. These molten, lava-covered worlds, such as Kepler-10b and Kepler-78b, are rocky planets in Earth's size range whose surfaces could well be perpetual infernos. Kepler-78b, roughly 20 percent larger than Earth, weighs in at twice Earth's mass; a comparable density means it could be composed of rock and iron. That might make it, like Mustafar, suitable for mining, although its extremely tight orbit around its sun-like star, along with scorching temperatures, provides an unlikely arena for industrial operations -- or for fencing with lightsabers.

Kepler-10b isn't much more pleasant. The first rocky world discovered using the Kepler telescope, it also hugs its sun, some 20 times closer than Mercury orbits ours. A balmy day on Kepler-10b means daytime highs of more than 2,500 Fahrenheit (1,371 Celsius), even hotter than lava flowing on Earth. The surface, free of any kind of atmosphere, might be boiling with iron and silicates.

At 3,600 degrees Fahrenheit (1,982 Celsius), however, CoRoT-7b has Kepler-10b beat. This well-grilled planet, discovered in 2010 with France's CoRoT satellite, lies some 480 light-years away, and has a diameter 70 percent larger than Earth's, with nearly five times the mass. Possibly the boiled-down remnant of a Saturn-sized planet, its orbit is so tight that its star looms much larger in its sky than our sun appears to us, keeping its sun-facing surface molten. (http://sci.esa.int/corot/)

Deep freeze

The planet OGLE-2005-BLG-390, nicknamed "Hoth," is a cold super-Earth that might be a failed Jupiter. Unable to grow large enough, it had to settle for a mass five times that of Earth and a surface locked in the deepest of deep freezes, with a surface temperature estimated at minus 364 degrees Fahrenheit (minus 220 Celsius). That most likely means no "Hoth"-style tauntauns to ride, or even formidably fanged abominable snowmen (aka "wampas"). Astronomers used an extraordinary planet-finding technique known as microlensing to find this world in 2005, one of the early demonstrations of this technique's ability to reveal exoplanets. In microlensing, backlight from a distant star is used to reveal planets around a star closer to us.

The planet lies toward the heart of the Milky Way, where a greater density of stars makes microlensing events more likely. The one-time event revealing the distant Hoth was captured by the Optical Gravitational Lensing Experiment, or OGLE, and confirmed by other instruments.

We won't have to travel 20,000 light years, however, to visit icy worlds. Saturn's smoggy moon, Titan, where the Cassini spacecraft's Huygens probe landed in 2005, is pocked with methane lakes and socked in permanently with thick, hydrocarbon haze. The freeze is so deep that water ice is no different from rock. Another Saturn moon, Enceladus, looks like a snowball but harbors a subsurface ocean much like Jupiter's moon Europa, another ice ball with a likely ocean underneath. That ocean would be warmed by tidal flexing as the little moon orbits Jupiter.

Sunset? Make it a double

Luke Skywalker's home planet, Tatooine, is said to possess a harsh, desert environment, swept by sandstorms as it roasts under the glare of twin suns. Real exoplanets in the thrall of two or more suns are even harsher. Kepler-16b was the Kepler telescope's first discovery of a planet in a "circumbinary" orbit -- circling both stars, as opposed to just one, in a double-star system. This planet, however, is likely cold, about the size of Saturn, and gaseous, though partly composed of rock. It lies outside its two stars' "habitable zone," where liquid water could exist. And its stars are cooler than our sun, and probably render the planet lifeless. Of course, we could look on the bright side (so to speak). When the discovery was announced in 2011, Bill Borucki, the now-retired NASA principal investigator for Kepler at Ames Research Center, Moffett Field, California, said finding the new planet might actually broaden the prospects for life in our galaxy. About half of all stars belong to binary systems, so the fact that planets form around these, as well as around single stars, can only increase the odds.

A more recently announced exoplanet, Kepler-453b, is also a circumbinary and a gas giant, though its orbit within its star's habitable zone means any moons it might have could be hospitable to life. It was the tenth circumbinary planet discovered using the Kepler telescope.

Ocean world

Kepler-22b, analog to the Star Wars planet Kamino (birthplace of the army of clone soldiers)), is a super-Earth that could be covered in a super ocean. Watery, storm-drenched Kamino makes its appearance in "Attack of the Clones."

The jury is still out on Kepler-22b's true nature; at 2.4 times Earth's radius, it might even be gaseous. But if the ocean world idea turns out to be right, we can envision a physically plausible Kamino-like planet, with the help of scientists at the Massachusetts Institute of Technology in Cambridge. An ocean world tipped on its side -- a bit like our solar system's ice giant, Uranus -- turns out to be comfortably habitable based on recent computer modeling. Researchers found that an exoplanet in Earth's size range, at a comparable distance from its sun and covered in water, could have an average surface temperature of about 60 degrees Fahrenheit (15.5 degrees Celsius). Because of its radical tilt, its north and south poles would be alternately bathed in sunlight and darkness, for half a year each, as the planet circled its star.

Scientists previously thought such a planet would seesaw between boiling and freezing, rendering it uninhabitable. But the MIT scientists' three-dimensional model showed that the planet, even with a relatively shallow ocean of about 160 feet (50 meters), would absorb heat during its odd polar summer and release it in winter. That would keep the overall climate mild and spring-like year round.

The shallow depth, by the way, would be ideal for Kamino-style ocean platforms, allowing construction of covered cities at the ocean surface, where armies of clones could march and drill in peace.

Fly me to the exomoon

Endor, the forested realm of the Ewoks, orbits a gas giant and was introduced in "Return of the Jedi." Detection of exomoons -- that is, moons circling distant planets -- is still in its infancy for scientists here on Earth. A possible exomoon was observed in 2014 via microlensing. It will remain forever unconfirmed, however, since each microlensing event can be seen only once. If the exomoon is real, it orbits a rogue planet, unattached to a star and wandering freely through space. The planet might have hung on to its moon after somehow being ejected during the early history of a forgotten planetary system. A team of Japanese, New Zealand, and American astronomers analyzed data gathered in 2011 with telescopes in New Zealand and Tasmania, and suggested the possible exomoon. They said a small star accompanied by a large planet also could have caused the same lensing effect.

More exomoons might soon be popping out from the depths of space. The Harvard-based Hunt for Exomoons with Kepler, or HEK, has begun to scour data from Kepler for signs of them. In early 2015, the researchers examined about 60 Kepler planets and determined that existing technology is sufficient to capture evidence of exomoons.

The hunt could have powerful implications in the search for life beyond Earth. If exomoons are shown to be potentially habitable, it would open another avenue for biology; habitable moons might even outnumber habitable planets. Could they have bustling ecosystems, with life forms even more exotic than Endor's living teddy bears, swinging between trees Tarzan-style? Stay tuned.

Breaking up is hard to do

In “A New Hope,” Princess Leia’s home planet, Alderaan, is blown to smithereens by the Empire’s Death Star as she watches in horror. Real exoplanets also can experience extreme destruction. A white dwarf star was caught in the act of devouring the last bits of a small planet in 2015, observed with the help of NASA's Chandra X-ray Observatory. White dwarfs are super-dense stellar remnants about the size of Earth, but with gravity more than 10,000 times that of our sun's surface. Tidal forces could rip a planet caught in its pull to shreds.


Observers thought at first they were seeing a black hole in the act of feeding inside a star cluster on the Milky Way's rim. X-ray observations, however, matched theoretical models of a planet being torn apart by a white dwarf. 

A similar observation of a closer white dwarf was made by K2 in 2014. In this case, a tiny rocky object, probably an asteroid, was being vaporized into little more than a dusty ring as it whipped around the star every 4.5 hours.

NASA's Spitzer Space Telescope also picked up signs of debris from a likely asteroid collision in 2014. But rather than a sign of planetary destruction, the colliding asteroids could be part of a construction site. This young star -- about 1,200 light years away and only 35 million years old -- is surrounded by a ring of dust where such collisions are frequent. The smashed and broken bits fuse into larger and larger agglomerations, eventually forming full-sized planets.

Our own solar system might once have looked very similar, if anyone was watching.

NASA's Ames Research Center in Moffett Field, California, manages the Kepler and K2 missions for NASA's Science Mission Directorate. NASA's Jet Propulsion Laboratory in Pasadena, California, managed Kepler mission development. Ball Aerospace & Technologies Corp. operates the flight system with support from the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder.

JPL, a division of the California Institute of Technology in Pasadena, manages the Spitzer Space Telescope for NASA.
Whitney Clavin, 818-354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.b.clavin@jpl.nasa.gov
Michele Johnson, 650-604-6982
Ames Research Center, Moffett Field, Calif.
michele.johnson@nasa.gov

Written by Pat Brennan
2015-372
Last Updated: Dec. 16, 2015
Editor: Tony Greicius
NASA
Guillermo Gonzalo Sánchez Achutegui
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domingo, 2 de agosto de 2015

NASA : Kepler Descubre un Primo de la Tierra Mayor y más Viejo

Hola amigos: A VUELO DE UN QUINDE EL BLOG., La misión Kepler de la NASA ha confirmado el descubrimiento del primer planeta casi del tamaño de la Tierra en la "zona habitable" alrededor de una estrella como nuestro Sol. Este descubrimiento y el de otros 11 nuevos candidatos a planetas pequeños en zonas habitables marcan otro hito en la búsqueda de otra "Tierra".
El planeta recién descubierto, Kepler-452b, es el más pequeño hasta la fecha encontrado en órbita dentro de la zona habitable -- la región alrededor de la estrella donde el agua líquida podría acumularse en la superficie de un planeta en órbita -- de una estrella de tipo G2, como nuestro Sol. La confirmación de Kepler-452b eleva el número total de planetas confirmados a 1030.
Kepler-452b es un 60 por ciento mayor en diámetro que la Tierra y es considerado un planeta supertierra. Aunque su masa y composición no han sido todavía determinados, las investigaciones previas sugieren que los planetas del tamaño de Kepler-452b tienen una buena probabilidad de ser rocosos.
Aunque Kepler-452b es mayor que la Tierra, su órbita de 385 días es sólo un 5 por ciento más larga. El planeta está un 5 por ciento más lejos de su estrella Kepler-452 que la Tierra del Sol. Kepler-452 tiene 6 mil millones de años de edad, 1.500 millones de años más que nuestro Sol, tiene la misma temperatura, es un 20 por ciento más brillante y su diámetro es un 10 por ciento mayor.
 
Concepto artístico en el cual se compara el tamaño de la Tierra (izquierda), y el nuevo planeta, llamado Kepler-452b, que es un 60 por ciento mayor en diámetro que la Tierra.
Concepto artístico en el cual se compara el tamaño de la Tierra (izquierda), y el nuevo planeta, llamado Kepler-452b, que es un 60 por ciento mayor en diámetro que la Tierra. Image Credit: NASA/JPL-CalTech
 
"Podemos pensar en Kepler-452b como un primo viejo y mayor de la Tierra que proporciona la oportunidad de comprender y reflexionar acerca de la evolución de la Tierra", dijo Jon Jenkins, jefe de análisis de datos de la misión Kepler en el Centro de Investigación Ames de la NASA. "Es asombroso considerar que este planeta ha pasado 6 mil millones de años en la zona habitable de su estrella, más tiempo que la Tierra. Se trata de una importante oportunidad para la aparición de la vida, en caso de que se dieran todos los ingredientes y condiciones necesarios para que la vida exista en este planeta".
Para ayudar a confirmar el hallazgo y determinar mejor las propiedades del sistema Kepler-452, el equipo llevó a cabo observaciones basadas en tierra en la Universidad de Texas en el Observatorio McDonald de Austin, el Observatorio Fred Lawrence Whipple en el Monte Hopkins, Arizona y el  Observatorio W. M. Keck en la cima de Mauna Kea en Hawai. Estas mediciones fueron clave para que los investigadores confirmasen la naturaleza planetaria de Kepler-452b, y para refinar el tamaño y el brillo de su estrella y precisar mejor el tamaño del planeta y su órbita. El sistema Kepler -452 se encuentra a 1.400 años luz de distancia en la constelación de Cygnus.
Además de confirmar a Kepler-452b, el equipo de Kepler ha incrementado el número de nuevos candidatos a exoplanetas en 521 desde su análisis de las observaciones realizadas desde Mayo de 2009 hasta Mayo de 2013, elevando el número de candidatos a planetas detectados por la misión Kepler en 4.696. Los candidatos requieren observaciones de seguimiento y análisis para verificar que son planetas reales.
 Doce de los nuevos candidatos a planetas tienen diámetros entre una a dos veces mayores que el de la Tierra y orbitan en la zona habitable de su estrella. De ellos, nueve orbitan estrellas que son similares a nuestro Sol en tamaño y temperatura.
"Hemos sido capaces de automatizar completamente nuestro proceso de identificación de planetas candidatos, lo que significa que por fin podemos evaluar todas las señales de tránsito en todo el conjunto de datos de Kepler rápida y uniformemente", dijo Jeff Coughlin, científico de Kepler en el Instituto SETI en Mountain View, California, quien dirigió el análisis de un nuevo catálogo de candidatos. "Esto le da a los astrónomos una población estadísticamente de planetas candidatos para determinar con precisión el número de planetas pequeños y posiblemente rocosos como la Tierra en nuestra galaxia, la Vía Láctea".
http://www.lanasa.net/
NASA
Guillermo Gonzalo Sánchez Achutegui

martes, 28 de julio de 2015

NASA : A Spin Around An Exoplanet Most Like Earth .- Una vuelta alrededor de un exoplaneta más igual que la Tierra (the planet Kepler-452b)

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia espacial NASA, sobre la investigación de un exo planeta, llamado : the planet Kepler-452b, ubicado en la Zona de Habitabilidad Galáctica en la Constelación del Cisne, que llevo a cabo el telescopio espacial Kepler;  según los últimos sondeos este exo planeta tiene similares condiciones a la Tierra, para que esta zona donde está el planeta tiene las probabilidadades de tener agua un ingrediente básico para sustentar la vida tal como sucede en La Tierra.

More information....

Kepler-452b rotating
This artistic animation depicts one possible appearance of the planet Kepler-452b, the first near-Earth-size world to be found in the habitable zone of star that is similar to our sun. The habitable zone is a region around a star where temperatures are right for water -- an essential ingredient for life as we know it -- to pool on the surface. Scientists do not know if Kepler-452b can support life or not. What is known about the planet is that it is about 60 percent larger than Earth, placing it in a class of planets dubbed "super-Earths." While its mass and composition are not yet determined, previous research suggests that planets the size of Kepler-452b have a better than even chance of being rocky. Kepler-452b orbits its star every 385 days. The planet's star is about 1,400 light-years away in the constellation Cygnus. It is a G2-type star like our sun, with nearly the same temperature and mass. This star is 6 billion years old, 1.5 billion years older than our sun. As stars age, they grow in size and give out more energy, warming up their planets over time. The planet's rotation is sped up.
Image credit: NASA Ames/JPL-Caltech/T. Pyle
Last Updated: July 28, 2015
Editor: Michele Johnson

Tags:  Kepler and K2
 NASA
Guillermo Gonzalo Sánchez Achutegui
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