最近还真是三体人的好日子啊……
众所周知，三体人是从半人马阿尔法星来的。这颗星是一个三星体系。不过现实中，以前一直没有发现过围绕它运行的行星——直到现在。
这颗行星被命名为Alpha Centauri Bb，它的质量是地球的113%，围绕Alpha Centauri B星运行。可惜离得太近了，表面温度大概高达1200度。这要是有生命的话也得靠水星播种那种技术了吧……
艺术家想象图。
The star system closest to our own sun hosts a planet with roughly Earth's mass and may harbor other alien worlds as well, a new study reports.
Astronomers detected the alien planet around the sunlike star Alpha Centauri B, which is part of a three-star system just 4.3 light-years away from us. The newfound world is about as massive as Earth, but it's no Earth twin; its heat-blasted surface may be covered with molten rock, researchers said.
The mere existence of the planet, known as Alpha Centauri Bb, suggests that undiscovered worlds may lurk farther away from its star — perhaps in the habitable zone, that just-right range of distances where liquid water can exist.
"Most of the low-mass planets are in systems of two, three to six or seven planets, out to the habitable zone," study co-author Stephane Udry, of the Geneva Observatory, told reporters today (Oct. 16).
So the discovery "opens really good prospects for detecting planets in the habitable zone in a system that is very close to us," Udry added. "In that sense, this system is a landmark."
Alpha Centauri Bb zips around its star every 3.2 days, orbiting at a distance of just 3.6 million miles (6 million kilometers). For comparison, Earth orbits about 93 million miles, or 150 million km, from the sun. [Gallery: Nearby Alien Planet Alpha Centauri Bb]
This wide-field view of the sky around the bright star Alpha Centauri was created from photographic images forming part of the Digitized Sky Survey 2. The star appears so big just because of the scattering of light by the telescope's optics as well as in the photographic emulsion. Alpha Centauri is the closest star system to the Solar System. Image released Oct. 17, 2012.
CREDIT: ESO/Digitized Sky Survey 2
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A difficult detection
The research team, led by Xavier Dumusque of Geneva Observatory and the University of Porto in Portugal, spotted Alpha Centauri Bb using an instrument called the High Accuracy Radial velocity Planet Searcher, or HARPS.
HARPS is part of the European Southern Observatory's 11.8-foot (3.6 meters) telescope at the La Silla Observatory in Chile. The instrument allows astronomers to pick up the tiny gravitational wobbles an orbiting planet induces in its parent star.
In the case of Alpha Centauri Bb, these wobbles are very tiny indeed; the planet causes its star to move back and forth at no more than 1.1 mph (1.8 kph). It took more than 450 HARPS measurements spread out over four years of observing to detect the planet's signal, Dumusque said.
"It’s an extraordinary discovery, and it has pushed our technique to the limit," he said in a statement.
The detection, to be published tomorrow (Oct. 17) in the journal Nature, was so difficult that some astronomers aren't yet convinced that Alpha Centauri Bb exists.
For example, Artie Hatzes of the Thuringian State Observatory in Germany lauded the discoverers' technical achievement but said he believes the jury is still out.
"As the American astronomer Carl Sagan once said, 'Extraordinary claims require extraordinary evidence,'" Hatzes wrote in a commentary piece in the same issue of Nature. "Although a planetlike signal is present in the data, the discovery does not quite provide the 'extraordinary evidence.' It is a weak signal in the presence of a larger, more complicated signal. In my opinion, the matter is still open to debate."
Udry, however, said that the team's statistical analyses show a "false alarm probability" of just one in 1,000 — meaning there's a 99.9 percent chance that the planet exists.
And some experts don't agree with Hatzes that Alpha Centauri Bb requires extraordinary supporting evidence.
"The reason why this seems to be an extraordinary claim is because everyone has heard of Alpha Centauri B; it's a household name," said Greg Laughlin of the University of California, Santa Cruz, who was not part of the discovery team. "It's extraordinary not so much in terms of the robustness of the result, but rather just in terms of the fact that it's a well-known nearby star."
