It's been less than a year since NASA launched the Kepler Space Telescope, and the device is already paying off with new discoveries. In particular, NASA scientists have identified a planet with the consistency of styrofoam, a gaggle of exoplanets, and two never-before-observed objects too small to be stars, but too hot to be planets.
NASA researchers revealed these discoveries yesterday, during a meeting of the American Astronomical Society. These revelations cover the first data sets produced by the Kepler Telescope, which launched in March 2009.
The styrofoam planet, called Kepler 7b, is 1.6 times the size of Jupiter, and less dense than water. If that wasn't weird enough, Kepler 7b also maintains a toasty 2300-degree Fahrenheit surface temperature, roughly hot enough to melt gold.
But those planets weren't even the hottest objects Kepler found. Two of the objects Kepler detected were hotter than the stars they orbited, thus failing to resemble any previously observed astronomical bodies.The objects are far smaller than stars, but much too hot to be planets. Some astronomers think that they might be newly formed planets, still hot from their chaotic birth. However, others think they might be white dwarf stars, slowly shrinking and dying as they orbit a more stable twin star at the center of their solar system.
And while these exotic bodies are certainly interesting, the most exciting discoveries announced yesterday were of something incredibly common to us Earthlings: sun-like stars. Based on measurements taken through Kepler, the NASA astronomers determined that only one third of 43,000 observed sun-like stars emit periodic life-killing bursts of radiation. This number is far lower than the previous estimate, and greatly expands the number of known solar systems potentially capable of harboring alien life.
Despite all the fascinating discoveries, the rate of discoveries coming out of Kepler may have been the most impressive revelation of the talk. Within the first six weeks of operation, scientists had already used Kepler to confirm five new exoplanets, a rate of discovery that makes Kepler a worthy successor to the Hubble.
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I like how the scientist say it's to small to be a star and then say it could be a white dwarf "star" LMAO!
ou have a point hessbri, something doesn't quite add up in the article.
They appear to know enough about some of these planets to state their size and density (eg "Kepler 7b, is 1.6 times the size of Jupiter, and less dense than water"), so they must also know the mass. But the mass of a white dwarf is nearly that of a star, so should be easy to tell.
A couple of White Dwarf factoids from wikipedia:
"Although white dwarfs are known with estimated masses as low as 0.17[27] and as high as 1.33[28] solar masses, the mass distribution is strongly peaked at 0.6 solar mass, and the majority lie between 0.5 to 0.7 solar mass"
"The estimated radii of observed white dwarfs, however, are typically between 0.008 and 0.02 times the radius of the Sun this is comparable to the Earth's radius of approximately 0.009 solar radius"
"White dwarf effective surface temperatures extend from over 150,000 K to under 4,000 K"
""" You have a point hessbri, something doesn't quite add up in the article.
They appear to know enough about some of these planets to state their size and density (eg "Kepler 7b, is 1.6 times the size of Jupiter, and less dense than water"), so they must also know the mass. But the mass of a white dwarf is nearly that of a star, so should be easy to tell.
A couple of White Dwarf factoids from wikipedia:
"Although white dwarfs are known with estimated masses as low as 0.17[27] and as high as 1.33[28] solar masses, the mass distribution is strongly peaked at 0.6 solar mass, and the majority lie between 0.5 to 0.7 solar mass"
"The estimated radii of observed white dwarfs, however, are typically between 0.008 and 0.02 times the radius of the Sun this is comparable to the Earth's radius of approximately 0.009 solar radius"
"White dwarf effective surface temperatures extend from over 150,000 K to under 4,000 K"""
' - Citation Needed - '
The comment in the article implying that white dwarfs weren't stars may have been a mistatement. White dwarfs are not "main sequence stars." Basically, they're what you get when a star not much bigger or smaller than the sun casts off its outer shell after swelling into a red giant at the end of its hydrogen burning cycle. They would be on the other end of the density scale from the "styrofoam planet," however, with as much matter as a mountain packed into a spoonful of white dwarf. Anyway, these oddballs are only the easiest things for Keppler to have spotted in a few weeks of observations. After a few months, it should have a record of objects with orbits more like Mercury, then maybe Venus. Because the scientists want three transits for confirmation, a planet orbiting a sunlike star at Earth's distance will take about three years to confirm. However, smaller stars have habitable zones closer in to the star, so there may be anouncements of planets in the habitable zones of these stars within the next year or two.
Good point about the smaller stars. Also the smaller stars tend to last longer, so planets in the habitable zones may have had several billion more years in which to develop life.
dont talk about billions of years like its a useful timescale, normally you could say a few million or hundred million, but considering by saying a few billion you could be exceeding the lifespan of the universe in counting the lifespan of objects within that universe, i wouldnt say thats an approperite scale...however informal
What I don't understand is how can scientists claim that they are observing the spectrum of a planet and only the planet. What if the star that is providing the back lighting has elements which are not common to sun like stars and the spectrum reflects the elements from the star? I understand that most of astrophysics and the study of exoplanets is highly theoretical so it would seem that most of what the scientists are discovering are educated guesses. In addition, who can say if the Kepler Telescope is 100% accurate in its observations? When the Hubble first came online it had several glitches that took quite a bit of time to resolve. I find the discoveries mentioned in this article fascinating but I can't help but be a bit skeptical of the information's accuracy. On the other hand, these types of discoveries often turn conventional wisdom on its head.