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Planet found in nearest star system to Earth

The observations extended over more than four years using the HARPS instrument and have revealed a tiny signal from a planet orbiting Alpha Centauri B every 3.2 days.
By ESO, Garching, Germany Published: October 17, 2012
Star-around-Alpha-Centauri-
This artist’s impression shows the planet orbiting the star Alpha Centauri B, a member of the triple star system that is the closest to Earth. Alpha Centauri B is the most brilliant object in the sky, and the other dazzling object is Alpha Centauri A. Our own Sun is visible to the upper right. The tiny signal of the planet was found with the HARPS spectrograph on the 3.6-meter telescope at ESO’s La Silla Observatory in Chile. // Credit: ESO/L. Calçada/N. Risinger
European astronomers have discovered a planet with about the mass of the Earth orbiting a star in the Alpha Centauri system — the nearest to Earth. It is also the lightest exoplanet ever discovered around a star like the Sun. The planet was detected using the HARPS instrument on the 3.6-meter telescope at the European Southern Observatory’s (ESO) La Silla Observatory in Chile.

Alpha Centauri is one of the brightest stars in the southern sky and is the nearest stellar system to our solar system, only 4.3 light-years away. It is actually a triple star — a system consisting of two stars similar to the Sun orbiting close to each other, designated Alpha Centauri A and B, and a more distant and faint red component known as Proxima Centauri. Since the 19th century, astronomers have speculated about planets orbiting these bodies, the closest possible abodes for life beyond the solar system, but searches of increasing precision had revealed nothing. Until now.

"Our observations extended over more than four years using the HARPS instrument and have revealed a tiny, but real, signal from a planet orbiting Alpha Centauri B every 3.2 days," said Xavier Dumusque from the Geneva Observatory in Switzerland and the University of Porto in Portugal. "It's an extraordinary discovery, and it has pushed our technique to the limit!"

The European team detected the planet by picking up the tiny wobbles in the motion of the star Alpha Centauri B created by the gravitational pull of the orbiting planet. The effect is minute. It causes the star to move back and forth by no more than 20 inches (51 centimeters) per second, about the speed of a baby crawling. This is the highest precision ever achieved using this method.

Alpha Centauri B is very similar to the Sun but slightly smaller and less bright. The newly discovered planet, with a mass of a little more than that of Earth, is orbiting about 3.7 million miles (6 million kilometers) away from the star, much closer than Mercury is to the Sun in the solar system. The orbit of the other bright component of the double star, Alpha Centauri A, keeps it hundreds of times farther away, but it would still be a brilliant object in the planet's skies.

This same team found the first exoplanet around a Sun-like star in 1995, and since then there have been more than 800 confirmed discoveries, but most are much bigger than Earth, and many are as big as Jupiter. The challenge astronomers now face is to detect and characterize a planet of mass comparable to Earth that is orbiting in the habitable zone around another star. The first step has now been taken.

"This is the first planet with a mass similar to Earth ever found around a star like the Sun. Its orbit is very close to its star, and it must be much too hot for life as we know it," said Stephane Udry from the Geneva Observatory, "but it may well be just one planet in a system of several. Our other HARPS results and new findings from Kepler both show clearly that the majority of low-mass planets are found in such systems."

"This result represents a major step towards the detection of a twin Earth in the immediate vicinity of the Sun. We live in exciting times!" said Dumusque.

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GARRY MEYER from UTAH said:
I have always felt I was born either to late in time or to soon to enjoy the advancement of technology where we will be at in 200 years from now. That is of course we don't destroy ourselves first. Imagine letting the mind go for the minute and exploring space. Wow, What will we know in time. Going to explore planets finding life forms of all kinds, shapes, and sizes. I read once that the cock roach almost became the dominating species of the planet. They would of been 6 feet tall. They would live in mud like structures on top of each other. Or visit a planet of those that have been visiting us. Te things they could share with us. Opps I just got back to earth. Yeah I have missed the time.
5 stars
LARS LINDSTROM from SWEDEN said:
"The majority of low-mass planets are found in such systems". Could this mean that our solar system was a double star system in the beginning? And could a planet exist in a goldilocks zone around either ACA or ACB or maybe both stars?
5 stars
RON CHINCHEN from AUSTRALIA (NSW) said:
The only reason we are reading of large planets revolving around stars and generally in very tight orbits is because it is far easier to detect a large object, such as a Jupiter sized planet, than an Earth sized planet. Further, with both the eclipse and wobble methods of detecting companions, it is far easier to detect close in planets because the period of the wobble or transit is frequent enough to gauge.

They are only now just being able to detect Earth sized planets, and then those close to their primary causing very minute but frequent variations. A planet Earth's distance from its primary causes one wobble or one transit in a year of observation. To detect even a large planet like Jupiter at that planet's distance from the Sun, would take over five years to detect one wobble or one transit. And that's dependent upon whether the planetary systems are aligned in such a manner that we can observe either a transit or wobble.

All we are getting so far is a sampling of planets whose systems are aligned with ours, a less than 10% chance, and that the planets are large enough and close enough so that we can detect their influence upon their star.

To detect an Earth sized planet in an orbit around a rare G type star at the distance the earth is to the Sun, is probably yet years away from being achieved...and that's if we are very lucky.
ROGER CHAPRONIERE from UNITED KINGDOM said:
I think that when the astronomical community is presented with findings like this we can only step back in wonder and congratulate the HARPS team for their outstanding work. To detect a wobble of 20 inches a second out at 4.5 light years is truly an example exquisite precision. As the writer of the article concluded "We live in exciting times"
4 stars
CHRIS R BAKER from CALIFORNIA said:
Frank, you are misreading it. Proxima Centauri is closest to US but farthest from the 2 primary stars. What I want to know is, how long till it's not the closest to us in it's orbit?
5 stars
KEVIN L STARNES from COLORADO said:
I'm very curious as to why so many of these extrasolar planets have such short orbital periods and consequently have much higher orbital velocities. If Alpha Centauri B is approximately the same size as our Sun and this new planet is a little heavier than Earth and orbit at only 3.7 million miles then this planet must be traveling at an insane speed in its orbit. My calculations (3.7,000,000 X 3.14 divided by 3.2 days {77 hours}) show an orbital speed of roughly 150,800 mph. What would account for this and why is this so common for many of the extrasolars that have been discovered? I don't have a degree in orbital mechanics and math isn't my forte' so I'm open to any viable theories.
5 stars
RONALD L ENGLEHART from WISCONSIN said:
Alpha Centauri is the closest star system to our Sun.
If this article turns out to be true it means there is credence to the
theory that all stars have planets, plantesimals, comets, asteroids,
or other types of rotators. Of course some may still have clouds of gas that haven't coalesced yet.
5 stars
RON CHINCHEN from AUSTRALIA (NSW) said:
In response to Frank Fielder, firstly hello fellow enthusiast. Great to hear others excited by this event. Your two points though need addressing

1) The article's references to Proxima Centauri as a 'faint. more distant component' of the Alpha Centauri System, actually is referring to its distance from the centre of the system itself, not its proximity to the Solar System.

Whereas the two giants of the system orbit each other in an elliptical orbit that, if it was in our solar system would be the difference in distance from the sun to a little beyond Saturn and then drifting out to a little beyond Uranus or about 1-2 Billion kilometres, Proxima Centauri is between 1-2 Trillion kilometres from the centre of the system, or about a fifth of a light year away from it. Its orbit is so far from the two primary stars that it is still uncertain if it is actually gravitationally.part of that system.

2) In respect of our solar system though, Proxima Centauri in its orbit, that seems to take hundreds of thousands if not millions of years to complete one circuit, is at this stage and for tens of thousands of years in a position that places it close to a tenth of a light year closer to us than the two primaries.

3) There is no question that Proxima Centauri could hold planets and probably does so. However Proxima Centauri is a red dwarf star, about M5, making it a star significantly smaller than the Sun or Alpha Centauri A and B. It is significantly less massive and dimmer and redder.

Whereas we get a whitish-yellow impression of our sun, the night sky of a planet revolving around Proxima would see its sun as a dimmer reddish colour. Further, because it is so much cooler, a planet revolving in its 'Goldilocks Zone' where all three forms of water can exists, would have an orbit much closer than Mercury is to our Sun.

This would cause two problems. Firstly the planet would probably be therefore gravitationally locked so only one side of the planet perpetually faces the star, like our moon does with Earth, and reduces the chance of a radiation shield around the planet. Secondly it means the planet is much closer to its star's variable outpourings of energy and Proxima is thought to be a 'flare star'. Such an outpouring from our Sun would have little serious impact on Earth. But a planet so close to its primary star would be saturated with radiation on a regular basis.

The interest in the two inner stars of the Alpha Centauri system is because unlike about 95% of the stars in the galaxy, these two stars are very close to being like our Sun and therefore likely to develop what we understand as life. Of course life elsewhere may be very different and able to cope with Proxima's excesses.
KARSTEN BOMHOLT from DENMARK said:
Proxima Centauri is still the Sun's nearest stellar neighbor. 'Faint, more distant' means, that it is in an orbit far from the two main components of the Alpha Centauri system. Pluto actually has five moons, and the discovery of a planet around one of the closest stars increases the chance, that there are planets around almost all stars in the Milky Way. Kepler can not find other planets in the Alpha Centauri system, because it is looking in a completely different direction. Although the distance to Alpha Centauri is only slightly more than four light-years, it is still very far to travel, and visits from ET is SF-fantasy.
5 stars
SAM NAUMAN from TEXAS said:
Frank the faint and more distant is not relative to our solar system but to the other two stars, Alpha Centuri A and B and it is faint because it is red and dimmer not because it is further from us. I doubt if we can get to the Alpha Centuri system physically (heck, we have not yet gone to Mars and we have no colonies on the Moon). However, maybe they are getting our TV signals and watching the pre-election debates. Hey, maybe After that they don't want to have anything to do with us.
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