Skip to main content

Help find alien worlds: Astronomers release huge dataset of nearby stars

Exoplanets
NASA/JPL-Caltech/T. Pyle
A team of astronomers led by the Carnegie Institution for Science made public on Monday an immense catalog of observations on nearby stars. The dataset is intended to be easily accessible for citizen scientists to engage in the search for exoplanets.

More than 61,000 measurements on over 1,600 stars are included in the catalog, which was complied during more than two decades by Hawaii’s W.M. Keck Observatory. Along with the dataset, the public is encouraged to download open-source software and an online tutorial to assist in analysis.

Recommended Videos

“[These] data likely contain even more planets that didn’t meet our statistical significant testing, but that more observing may reveal with time,” Paul Butler, staff scientists at Carnegie’s Department of Terrestrial Magnetism, told Digital Trends. “In that sense, these data will likely ‘keep on giving’ for a long time.”

MoreKepler finds 104 exoplanets in the largest single haul of confirmed planets

The huge catalog — the largest ever released using a method called radial velocity (RV), the slight movements some stars make in response to internal or external forces (such as the gravitational pull of an exoplanet) — was made possible thanks to a little bit of outside-of-the-box thinking. Keck’s High-Resolution Echelle Spectrometer (HIRES) instrument wasn’t initially designed to measure RV, but astronomers quickly realized it could be used for such studies.

“Although HIRES was originally designed to look at faint galaxies, my teammates had plans to use HIRES for planet hunting before it was even installed,” Jennifer Burt, an MIT postdoctoral fellow who’s involved in the project, told Digital Trends. “Which is why Steve Vogt, who designed the instrument, made sure there was an iodine cell — which is one of the methods for doing precision RV science — installed at first light.”

That’s a good thing too, since HIRES has facilitated a handful of notable exoplanet discoveries since the mid-1990s, according to Burt.

The researchers have been busy combing through the data collected by HIRES and have recently detected more than 100 potential exoplanets. In a paper that will soon be published in the Astronomical Journal, Burt and her colleagues describe the discovery of a 3.8 Earth-mass planet orbiting our fourth closest star. “[This] really drives home the point that almost all of our nearby stars likely have planets around them,” she said.

However, the researchers hope the catalog’s release will inspire citizen scientists around the world to join the hunt, because there’s simply too much data for them to effectively sift through alone.

“My hope is that this data will give people who might not deal with science in their every day lives the incentive to investigate the data analysis and fitting process,” Burt said. “I think that exoplanets are both a very tangible and very exciting area of science, and one in which we are making new discoveries almost every day. Because of that, this field is a great way to introduce the community, especially the kids in grade school and high school, to cutting edge research and show them that anyone can be a scientist!”

Dyllan Furness
Former Digital Trends Contributor
Dyllan Furness is a freelance writer from Florida. He covers strange science and emerging tech for Digital Trends, focusing…
Astronomers catch the destruction of a red supergiant star in real time
an artist’s impression of a red supergiant star in the final year of its life emitting a tumultuous cloud of gas. this suggests at least some of these stars undergo significant internal changes before going supernova.

When very large stars run out of fuel and reach the end of their lives, they can explode in massive, dramatic events called supernovas. These explosions throw off enormous amounts of light and energy, but there's much we still don't know about how this process happens. Now, astronomers have observed a red supergiant star going supernova for the first time, catching a glimpse of the massive star's final moments of life.

“This is a breakthrough in our understanding of what massive stars do moments before they die,” said Wynn Jacobson-Galán, lead author of the study, in a statement. “Direct detection of pre-supernova activity in a red supergiant star has never been observed before in an ordinary Type II supernova. For the first time, we watched a red supergiant star explode!”

Read more
Astronomers discover enormous planet in extreme, massive star system
This artist’s impression shows a close up of the planet b Centauri b, which orbits a binary system with mass at least six times that of the Sun. This is the most massive and hottest planet-hosting star system found to date. The planet is ten times as massive as Jupiter and orbits the two-star system at 100 times the distance Jupiter orbits the Sun.

Astronomers have discovered a planet some previously thought to be impossible, orbiting an enormous and extremely hot star system. The planet, which orbits the two-star system b Centauri, is challenging assumptions about where planets can form.

This artist’s impression shows a close-up of the planet b Centauri b, which orbits a binary system with mass at least six times that of the Sun. This is the most massive and hottest planet-hosting star system found to date. The planet is ten times as massive as Jupiter and orbits the two-star system at 100 times the distance Jupiter orbits the Sun. ESO/L. Calçada

Read more
Astronomers use new method to discover planet orbiting two stars
Illustration of TIC 172900988b, a planet orbiting two stars.

Astronomers using NASA's Transiting Exoplanet Survey Satellite (TESS) telescope have used a new detection technique to discover an unusual planet that orbits two stars. The planet TIC 172900988b has two suns, making it a type of planet called a circumbinary, and it is the first of its kind to be detected using TESS observing just two transits.

Exoplanets, or planets outside our solar system, are usually too small and faint to be seen directly. But astronomers can infer their existence using a variety of techniques including transits. A transit is an event when an exoplanet passes between Earth and its host star, temporarily blocking out some of the star's light. Astronomers look for these drops in light and use them to predict the presence of a planet.

Read more