Nature 527, 7577 (2015). doi:10.1038/527134a
Conflict at the Arecibo Observatory highlights the need for funders to become more flexible.
Astronomy: A small star with an Earth-like planet
Nature 527, 7577 (2015). doi:10.1038/527169a
Authors: Drake Deming
A rocky planet close in size to Earth has been discovered in the cosmic vicinity of our Sun. The small size and proximity of the associated star bode well for studies of the planet's atmosphere. See Letter p.204
A rocky planet transiting a nearby low-mass star
Nature 527, 7577 (2015). doi:10.1038/nature15762
Authors: Zachory K. Berta-Thompson, Jonathan Irwin, David Charbonneau, Elisabeth R. Newton, Jason A. Dittmann, Nicola Astudillo-Defru, Xavier Bonfils, Michaël Gillon, Emmanuël Jehin, Antony A. Stark, Brian Stalder, Francois Bouchy, Xavier Delfosse, Thierry Forveille, Christophe Lovis, Michel Mayor, Vasco Neves, Francesco Pepe, Nuno C. Santos, Stéphane Udry & Anaël Wünsche
M-dwarf stars—hydrogen-burning stars that are smaller than 60 per cent of the size of the Sun—are the most common class of star in our Galaxy and outnumber Sun-like stars by a ratio of 12:1. Recent results have shown that M dwarfs host Earth-sized planets in great numbers: the average number of M-dwarf planets that are between 0.5 to 1.5 times the size of Earth is at least 1.4 per star. The nearest such planets known to transit their star are 39 parsecs away, too distant for detailed follow-up observations to measure the planetary masses or to study their atmospheres. Here we report observations of GJ 1132b, a planet with a size of 1.2 Earth radii that is transiting a small star 12 parsecs away. Our Doppler mass measurement of GJ 1132b yields a density consistent with an Earth-like bulk composition, similar to the compositions of the six known exoplanets with masses less than six times that of the Earth and precisely measured densities. Receiving 19 times more stellar radiation than the Earth, the planet is too hot to be habitable but is cool enough to support a substantial atmosphere, one that has probably been considerably depleted of hydrogen. Because the host star is nearby and only 21 per cent the radius of the Sun, existing and upcoming telescopes will be able to observe the composition and dynamics of the planetary atmosphere.
Planetary science: How Mars loses its atmosphere
Nature 527, 7577 (2015). doi:10.1038/527136a
Solar storms have blasted much of Mars's tenuous atmosphere into space over billions of years, making the planet the barren world it is today.A series of papers has outlined the first results from NASA's Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft, which has been
An international team of astronomers, led researchers from the University of Cambridge and the Australian National University, have identified some of the oldest stars in our galaxy, which could contain vital clues about the early Universe, including an indication of how the first stars died.
These stars, which have been at the very centre of the Milky Way for billions of years, contain extremely low amounts of metal: one of the stars is the most metal-poor star yet discovered in the centre of our galaxy. These stars also contain chemical fingerprints which indicate that the very first stars may have died in spectacular deaths known as hypernovae, which were ten times more energetic than a regular supernova. The findings, reported today (11 November) in the journal Nature, could aid in understanding just how much the Universe has changed over the past 13.7 billion years.
For decades, astronomers have been trying to determine what the Universe was like soon after the Big Bang – understanding how the first stars and galaxies formed is crucial to this goal. While some astronomers are looking outward to galaxies billions of light years away to untangle this mystery, others are looking inward to the centre of our galaxy.
If you’ve ever looked up at the night sky from a dark place you might see the centre of the Milky Way. There are billions of stars in our galaxy, and astronomers are interested in picking out the oldest stars and finding out about their chemical composition and movements.
Soon after the Big Bang, the Universe was entirely made up of only hydrogen, helium and small amounts of lithium. All of the other elements, like the oxygen we breathe or the sodium in our toothpaste, have been made inside stars or when they die as supernovae. This has led astronomers to search for extremely metal-poor stars: stars with lots of hydrogen, but very little of any other element.
It had been thought that the very first stars formed in the centre of the galaxy, where the effects of gravity are strongest. But after decades of searches, astronomers found that most stars in the centre of our galaxy have a similar metal content of those much closer to us. While the stars at the centre of the galaxy are about seven billion years older than the Sun, they’re still not old enough to understand what the conditions were like in the early Universe.
Using telescopes in Australia and Chile, astronomers may have landed on a winning strategy to find the oldest stars in the galaxy. Stars with a low metal content look slightly bluer than other stars: a key difference that can be used to sift through the millions of stars at the centre of the Milky Way.
Using images taken with the ANU SkyMapper telescope in Australia, the team selected 14,000 promising stars to look at in more detail, with a spectrograph on a bigger telescope. A spectrograph breaks up the light of the star, much like a prism, allowing astronomers to make detailed measurements.
Their best 23 candidates were all very metal-poor, leading the researchers to a larger telescope in the Atacama desert in Chile. From this data the team identified nine stars with a metal content less than one-thousandth of the amount seen in the Sun, including one with one-ten-thousandth the amount – now the record breaker for the most metal-poor star in the centre of the galaxy.
“If you could compress all the iron in the Sun to the size of your fist, some of these stars would contain just a tiny pebble by comparison,” said Dr Andrew Casey of Cambridge’s Institute of Astronomy, one of the study’s co-authors. “They’re very, very different kinds of stars.”
However, knowing that these stars have low amounts of metal wasn’t enough to be certain that they formed very early in the Universe. They could be stars that formed much later in other parts of the galaxy that weren’t as dense, and they are just now passing through the centre. To separate those possibilities, researchers measured distances and used precise measurements of the stars’ movement in the sky to predict how the stars were moving, and where they had been in the past.
They found that while some stars were just passing through, seven of the stars had spent their entire lives in the very centre of our galaxy. Computer simulations suggest that stars like this must have formed in the very early Universe.
“There are so many stars in the centre of our Galaxy – finding these rare stars is really like looking for a needle in a haystack,” said Casey. “But if we select these stars in the right way, it’s like burning down the farm and sweeping up the needles with a magnet.”
When the very first stars in the galaxy died, they left a chemical signature on the generation of stars reported on in this latest study. This chemical fingerprint suggests the very first stars may have died in spectacular deaths known as hypernovae, an explosion ten times more energetic than a regular supernova. This would make it one of the most energetic things in the Universe, and very different from the kinds of stellar explosions we see today.
“This work confirms that there are ancient stars in the centre of our Galaxy. The chemical signature imprinted on those stars tells us about an epoch in the Universe that’s otherwise completely inaccessible,” said Casey. “The Universe was probably very different early on, but to know by how much, we’ve really just got to find more of these stars: more needles in bigger haystacks.”
L.M. Howes et. al. ‘Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way.’ Nature (2015). DOI: 10.1038/nature15747
Astronomers have discovered some of the oldest stars in the galaxy, whose chemical composition and movements could tell us what the Universe was like soon after the Big Bang.Finding these rare stars is really like looking for a needle in a haystack. But if we select these stars in the right way, it’s like burning down the farm and sweeping up the needles with a magnetAndrew CaseyESOAn artist's impression of a hypernova, an explosive death of a star roughly ten times more energetic than a normal supernova.
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