A Possible New Planet Around the Second Closest Star System to Earth

An international team of astronomers is announcing the possible discovery of a planet around the second closest star system to us, Barnard’s Star. A mere 6 light-years away, the star is a faint red dwarf which gives off only four hundredths of a percent of the Sun’s light energy. The planet, which could be as massive as 3 Earths, is orbiting at the same distance as Mercury is from the Sun, but is still colder than Saturn and unlikely to harbor life as we know it.

Since the closest star system to us also has a known planet in it, this discovery (if it is confirmed) would make it even more likely that planets are “more common than dirt” out there. Four planetary systems would then be known among the stars 10 light-years or closer. Some 2900 planetary systems (containing almost 4,000 planets) have now been found in our galactic neighborhood.

The new planet, which takes 233 days to orbit, was detected from the very slight “wiggles” that the planet’s gravity (as it goes around) gives to the motion of its star. The wiggles are so small that it took 20 years of observations, using special equipment on various telescopes around the world, to identify them. While it’s still possible that their combined observations have another explanation, the 63 authors on the paper announcing the planet have dug deeply into their data statistics and claim that the planet idea is the most likely explanation. Not all experts in the field agree that this is a definite detection. Instruments of the future, with better ability to detect tiny star wiggles, will ultimately decide if the planet is real.

Our image shows an artist conception of what the the “cold, hostile desert” surface of the planet around Barnard’s Star, with a temperature of -270 degrees Centigrade, might look like. (You will need to take your parka if you go.)

Hot Discovery: Venus-like Planet around Red Dwarf Star

A newly discovered planet is as hot as your oven at full strength and takes less than two days to orbit its star.

As the number of confirmed planets orbiting other stars nears 2000 (when just twenty years ago, that number was zero), we are finding many planets that are not like any we know in our own solar system. The new planet orbits a red dwarf, a star 200 times fainter than our Sun, called GJ1132. (GJ stands for Gliese-Jahreiss, the name of two German astronomers who produced a remarkable catalog of the stars closest to our Sun.)

Astronomers used telescopes around the world to pin down the characteristics of the new planet, which is just 39 light years away, very close by cosmic standards. It turns out to be a rocky planet, a little bigger and more massive than Earth.

But it is so close to its star it takes only 1.6 days to go around. (In other words, a year on that planet would be just 1.6 Earth days. That means an Earth 10-year old would be about 2280 years old on that planet!)

At so close a distance (only a million and a half miles away from its star), the planet experiences temperatures on the order of 450 degrees Fahrenheit. So it reminds us more of superhot Venus in our solar system than our own Earth. Interestingly, other planets known to be rocky that we have discovered orbiting other stars are even hotter. (Hot, close planets are easier to find, so they are over-represented among our early discoveries.)

Still, if for some reason, you need a turkey cooked really fast this week, perhaps a quick trip to GJ 1132b (as the planet is boringly designated) would be in order. Or just give thanks that you live in a cooler planet which takes its time orbiting the Sun.

[P.S. The image is just an artist's impression. We can't photograph such small close in planets -- they are lost in the glare of their star.]

A Nearby Faint Star With 6 or 7 Planets

Big news today from astronomers studying "exoplanets" -- planets that orbit other stars in the sky. Groups of astronomers in Europe and America, working together, have found a faint nearby star which has 6 or maybe even 7 planets orbiting it, three of which are in the "habitable zone" -- where water can be a liquid.

The name of the star is Gliese 667C (part of a system of three stars that orbit around each other). Only the faintest of the three stars has been found to have planets, but that faint one has quite a family of them. You can see the planets and the star on our diagram.

The way astronomers name these things is by giving each object a letter in order of discovery. So in this Gliese 667 system, capital A, B, and C are the letters for the three stars. Then the planets around star C are given lower-case letters, starting with b. (Planet "h" is not fully confirmed, so it has a question mark next to it.) The green zone is where the planets are that have the right temperature for life as we know it.

The three planets in the green zone of this star are what we call "super-Earths" -- they are bigger than Earth, but smaller than Uranus and Neptune. The method we use to discover these planets only gives us an estimate of their mass, but given how crowded the habitable zone seems to be, scientists are feeling reasonably sure that these planets are no bigger than about 10 Earth masses.

This is the largest number of planets ever found in the habitable zone of another star. (Planet h, the one that is not yet confirmed, is just tantalizingly at the edge of that zone.)

All the planets and the three stars are about 22 light years away in the constellation of Scorpius. (The closest star is 4 light years away, so, in the cosmic scheme of things, Gliese 667 is one of our closest neighbors!)

What's especially interesting about this discovery is that the faint star that has all the planets is what astronomers call an M-type star -- it has only 1/3 the mass of our Sun and shines with only about 2% of our Sun's light output. So the habitable zone is much closer to the cool star than our Sun's is. The planets in the habitable zone take between 28 and 62 days to orbit the star. (Recall that the Earth takes 365 days to go around our much hotter Sun!)

The interesting part is that M type stars are much more common in the universe than stars like our Sun. So if an M type star like Gliese 667C can have 6 or 7 planets crowded around it, that means that perhaps other such M type stars also have families of planets and the number of sites we can look for life in the universe has just gone up.

For more technical details, more pictures, and even short videos, see: http://www.eso.org/public/news/eso1328/

(By the way, Gliese comes from the name Wilhelm Gliese, a German astronomer, who constructed one of the most important catalogs of nearby stars. Many faint stars near us have Gliese numbers from his catalog.)