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RIP and good planet hunting, Kepler

Very few experiments have changed the way we perceive our Universe, but the Kepler exoplanet survey telescope is one such example. Simply by monitoring a single patch of the sky continuously, it provided a new understanding of how many planets exist in the galaxy. Since its launch in 2009, Kepler identified 115 exoplanets with over 2,700 other potential planet candidates—including a number that are comparable in size to Earth or orbiting within the habitable zone where liquid water might exist.

However, Kepler is an orbiting telescope, unreachable by spacecraft for repairs. Today, NASA announced that a reaction wheel—required to keep the telescope pointed steadily in one direction—ceased functioning. This is the second reaction wheel failure, meaning Kepler can't continue to monitor the same stars and their exoplanets it has watched since 2009.

The Kepler engineering team had been anticipating this problem for some months, so this news was not unexpected. NASA associate administrator John Grunsfeld mentioned hope that engineers could restore communication with the control system managing the reaction wheel, but the fact that this state of failure has persisted for some days indicates how faint the hope is.

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RIP and good planet hunting, Kepler

Very few experiments have changed the way we perceive our Universe, but the Kepler exoplanet survey telescope is one such example. Simply by monitoring a single patch of the sky continuously, it provided a new understanding of how many planets exist in the galaxy. Since its launch in 2009, Kepler identified 115 exoplanets with over 2,700 other potential planet candidates—including a number that are comparable in size to Earth or orbiting within the habitable zone where liquid water might exist.

However, Kepler is an orbiting telescope, unreachable by spacecraft for repairs. Today, NASA announced that a reaction wheel—required to keep the telescope pointed steadily in one direction—ceased functioning. This is the second reaction wheel failure, meaning Kepler can't continue to monitor the same stars and their exoplanets it has watched since 2009.

The Kepler engineering team had been anticipating this problem for some months, so this news was not unexpected. NASA associate administrator John Grunsfeld mentioned hope that engineers could restore communication with the control system managing the reaction wheel, but the fact that this state of failure has persisted for some days indicates how faint the hope is.

Read 2 remaining paragraphs | Comments

RIP and good planet hunting, Kepler

Very few experiments have changed the way we perceive our Universe, but the Kepler exoplanet survey telescope is one such example. Simply by monitoring a single patch of the sky continuously, it provided a new understanding of how many planets exist in the galaxy. Since its launch in 2009, Kepler identified 115 exoplanets with over 2,700 other potential planet candidates—including a number that are comparable in size to Earth or orbiting within the habitable zone where liquid water might exist.

However, Kepler is an orbiting telescope, unreachable by spacecraft for repairs. Today, NASA announced that a reaction wheel—required to keep the telescope pointed steadily in one direction—ceased functioning. This is the second reaction wheel failure, meaning Kepler can't continue to monitor the same stars and their exoplanets it has watched since 2009.

The Kepler engineering team had been anticipating this problem for some months, so this news was not unexpected. NASA associate administrator John Grunsfeld mentioned hope that engineers could restore communication with the control system managing the reaction wheel, but the fact that this state of failure has persisted for some days indicates how faint the hope is.

Read 2 remaining paragraphs | Comments

RIP and good planet hunting, Kepler

Very few experiments have changed the way we perceive our Universe, but the Kepler exoplanet survey telescope is one such example. Simply by monitoring a single patch of the sky continuously, it provided a new understanding of how many planets exist in the galaxy. Since its launch in 2009, Kepler identified 115 exoplanets with over 2,700 other potential planet candidates—including a number that are comparable in size to Earth or orbiting within the habitable zone where liquid water might exist.

However, Kepler is an orbiting telescope, unreachable by spacecraft for repairs. Today, NASA announced that a reaction wheel—required to keep the telescope pointed steadily in one direction—ceased functioning. This is the second reaction wheel failure, meaning Kepler can't continue to monitor the same stars and their exoplanets it has watched since 2009.

The Kepler engineering team had been anticipating this problem for some months, so this news was not unexpected. NASA associate administrator John Grunsfeld mentioned hope that engineers could restore communication with the control system managing the reaction wheel, but the fact that this state of failure has persisted for some days indicates how faint the hope is.

Read 2 remaining paragraphs | Comments

RIP and good planet hunting, Kepler

Very few experiments have changed the way we perceive our Universe, but the Kepler exoplanet survey telescope is one such example. Simply by monitoring a single patch of the sky continuously, it provided a new understanding of how many planets exist in the galaxy. Since its launch in 2009, Kepler identified 115 exoplanets with over 2,700 other potential planet candidates—including a number that are comparable in size to Earth or orbiting within the habitable zone where liquid water might exist.

However, Kepler is an orbiting telescope, unreachable by spacecraft for repairs. Today, NASA announced that a reaction wheel—required to keep the telescope pointed steadily in one direction—ceased functioning. This is the second reaction wheel failure, meaning Kepler can't continue to monitor the same stars and their exoplanets it has watched since 2009.

The Kepler engineering team had been anticipating this problem for some months, so this news was not unexpected. NASA associate administrator John Grunsfeld mentioned hope that engineers could restore communication with the control system managing the reaction wheel, but the fact that this state of failure has persisted for some days indicates how faint the hope is.

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Gearing up to search for gravity waves

A simulation of merging black holes.

In the Newtonian view of the world, binary star systems should remain in a stable orbit in perpetuity, no matter how massive the objects or how close the orbit. But with general relativity, that changes; energy gets carried away from the system in the form of gravity waves, which gradually causes the orbit to decay, ultimately leading to a merger.

By observing binary systems of massive objects, we've determined that general relativity gets it right. These systems behave just as general relativity predicts, giving us confidence that the theory is correct. What's missing is the other half of the confirmation: gravity waves. We haven't detected any originating from these systems. In fact, we haven't detected any, period.

It's not for lack of trying. For nearly a decade, the Laser Interferometer Gravitational-Wave Observatory, or LIGO, searched for gravity waves from astronomical events, like the merger of two black holes (a number of other detectors have also engaged in the search, but all have come up empty). Now, scientists are readying a worldwide network of LIGO-like detectors that should start coming online in 2017. A short perspective in Science outlines the project's plans.

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Tonight: Get the clearest, brightest view of Saturn in years

Saturn-watchers take note. Tonight is not only the best time to view the striking ringed planet in 2013, but experts say it's the best chance to get a clear, bright view from an Earth-based telescope in years.

This evening Saturn will stand "at opposition" to the Sun, meaning Earth is sitting almost perfectly in line between the Sun and the sixth planet in our solar system. Saturn will be only about 808 million miles from Earth tonight, making the planet appear as bright as nearby stars such as Betelgeuse. The apparent magnitude will be between 0.1 to 0.3.

Because of the opposition, Saturn will be visible throughout the evening when looking to the southeast, rising in the East and reaching its highest elevation at midnight. The planet will continue to appear in the night sky through much of May, but tonight offers the best viewing opportunity to see Saturn's marvelous rings. Through telescope, you'll also be able to make out many of Saturn's 60 moons, including Titan, Rhea, and Tehtys. Even the hexagonal cloud pattern surrounding its north pole should be visible.

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Kepler spots two super Earths, one squarely in the habitable zone

Liquid water is one of the essential ingredients of life on Earth and it has properties conducive to life in general, so researchers have defined the concept of a habitable zone with water as its focus. For astronomers, the habitable zone is the area far enough from a host star that a planet would be cool enough to support liquid water, but not so far that the water would be frozen. Although there are many caveats to this definition—everything from the presence of greenhouse gasses to clouds will shift a planet's average surface temperature—the concept helps drive the search for a planet capable of supporting life.

The caveats, however, have led to a number of arguments over whether a given exoplanet is likely able to host liquid water, with some candidates shifting in and out of the habitable zone more than once. Still, it's pretty clear that, given the large number of reported candidate exoplanets, the odds suggest we've already spotted one. Today, scientists are announcing an exosolar system that has two planets that are both likely to be within the habitable zone, along with three others that are closer to the host star.

The findings come from the Kepler mission, which is dealing with a backlog of roughly 2,000 planet candidates to sort through and confirm. Normally, confirmation requires observing changes in the light emitted by the host star, which gets dragged closer to and further from the Earth as the planets circle it. However, this method requires that the planets either be large or orbiting close to the star so that their gravitational influence is big enough to shift it.

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Want to name an exoplanet after your cat? IAU says dream on

It has been incredibly exciting to bring you the latest news on the hunt for planets outside our Solar System. Over the past few years, the planets we've spotted have gotten closer to Earth's size, closer to the Solar System, and far, far more numerous. There's almost nothing that could dull the excitement—except, perhaps, the planets' names. Monikers like KOI-135 b and HAT-P-5 b don't exactly inspire a sense of the mysterious unknown.

Even the International Astronomical Union (IAU) admits they're a bit dull. "While exoplanet names such as 16 Cygni Bb or HD 41004 Ab may seem boring when considering the names of planets in our own Solar System, the vast number of objects in our Universe—galaxies, stars, and planets to name just a few—means that a clear and systematic system for naming these objects is vital," the organization has noted. But at least one company has decided that clear and systematic is not its thing, and it has started selling the chance to name a planet.

Or rather nominate a name and download a certificate of said nomination. People can then vote on the nominees, with voting closing on Monday night. The company running the process says it donates some of its funds to astronomy research and education efforts.

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Hubble telescope spots death of a white dwarf 10 billion years ago

Hubble Space Telescope image of a supernova more than 10 billion light-years away. This explosion, known as a white dwarf or type Ia supernova, is the most distant of its kind yet seen.

When a white dwarf explodes as a type Ia supernova, its death is so bright that its light can be detected across the Universe. A new observation using the Hubble Space Telescope identified the farthest type Ia supernova yet seen, at a distance of greater than 10 billion light-years. In the tradition of supernova surveys, this event was nicknamed for Woodrow Wilson, 28th President of the United States. The previous record-holder, Supernova Mingus, was about 350 million light-years closer to Earth.

White dwarfs are the remains of stars similar in mass to the Sun. Since such a star would have to live out its entire life to form a white dwarf, there are limits to how early in the Universe's history a type Ia supernova can explode. Only 8 white dwarf supernovas have been identified farther than 9 billion light-years away. (Some core-collapse supernovas, which are the explosions of very massive stars, have been seen farther than Supernova Wilson.) Since all such explosions happen in a similar way, cosmologists use them to measure the expansion rate of the Universe.

Astronomers found this violent event by comparing the light from several separate long exposures of the same patch of the sky, known as CANDELS (the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey). Bright as it was, the distance was so great that Supernova Wilson appeared as an enhancement of the luminosity of its host galaxy. The researchers subtracted the light of the galaxy without the supernova from the combined supernova-galaxy combination, then analyzed the residual light to identify it as type Ia.

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