Controversial Clues of Two 'Goldilocks Planets' That Might Support Life are Proven False
This animation shows planets believed to orbit the red dwarf star Gliese 581. These detections, made with the Doppler technique, were published in scientific papers from 2004 to 2014 and put some of the claimed planets in or near the star's Habitable Zone, where it might be possible for life as we know it to exist.
Blue indicates detections of candidate planets in the just-right region inside or near the Habitable Zone, where liquid water could exist. Orange indicates detections in the too-hot region that is too close to the star. Green indicates detections in the too-cold region farther away from the star and outside the Habitable Zone.
New research led by astronomers at Penn State University and published in the journal Science has disproved the existence of two of these controversial "Goldilocks planets," showing, instead, that the signals resulted from magnetic activity of the star, not from an orbiting planet. The three planets shown in the 2014 frames of this animation are the only ones that the study found to be actual planets, while the other two detections result from the star's own activity signals.
The size of each planet in this figure corresponds to its minimum mass. Some simplifications have been made for illustrative purposes. The refereed literature provides a complete history of the scientific publications relevant to this star and its planets.
The background image is a composite photo of our Sun taken by Alan Friedman. The left side of the Sun is seen through a filter that allows the camera to see wavelengths of light only in the deep-blue range, while the right side is seen through a filter that blocks all wavelengths except those in the red range. While the blue region is traditionally used to detect stellar activity, this study used the red region of the light spectrum. This video contains no sound.
Credit: This animation was adapted from a d3 visualization by Mike Bostok.
Mysteries about controversial signals coming from a dwarf star considered to be a prime target in the search for extraterrestrial life now have been solved in research led by scientists at Penn State University. The scientists have proven, for the first time, that some of the signals, which were suspected to be coming from two planets orbiting the star at a distance where liquid water could potentially exist, actually are coming from events inside the star itself, not from so-called "Goldilocks planets" where conditions are just right for supporting life. The study will be published by the journal Science in its online Science Express issue on July 3, 2014 and in a future print edition of the journal.
"This result is exciting because it explains, for the first time, all the previous and somewhat conflicting observations of the intriguing dwarf star Gliese 581, a faint star with less mass than our Sun that is just 20 light years from Earth," said lead author Paul Robertson, a postdoctoral fellow at Penn State who is affiliated with Penn State's Center for Exoplanets and Habitable Worlds. As a result of this research, the planets now confirmed to be orbiting this dwarf star total exactly three.
"We also have proven that some of the other controversial signals are not coming from two additional proposed Goldilocks planets in the star's habitable zone, but instead are coming from activity within the star itself," said Suvrath Mahadevan, an assistant professor of astronomy and astrophysics at Penn State and a coauthor of the research paper. None of the three remaining planets, whose existence the research confirms, are solidly inside this star system's habitable zone, where liquid water could exist on a rocky planet like Earth.
This image shows the location of six candidate planets believed to orbit the red dwarf star Gliese as of 2010. Blue indicates candidate planets in the habitable zone where conditions might be able to support life, orange indicates detections in the too-hot region that is too close to the star, green indicates detections in the too-cold region farther away from the star. Credit: NASA/Penn State University
Astronomers search for exoplanets by measuring shifts in the pattern of a star's spectrum -- the different wavelengths of radiation that it emits as light. These "Doppler shifts" can result from subtle changes in the star's velocity caused by the gravitational tugs of orbiting planets. But Doppler shifts of a star’s "absorption lines" also can result from magnetic events like sunspots originating within the star itself -- giving false clues of a planet that does not actually exist. "In the search for low-mass planets," Mahadevan said, "accounting for the subtle signature of a magnetics events in the star is as important as obtaining the highest possible Doppler precision."
The research team made its discovery by analyzing Doppler shifts in existing spectroscopic observations of the star Gliese 581 obtained with the ESO HARPS and Keck HIRES spectrographs. The Doppler shifts that the scientists focused on were the ones most sensitive to magnetic activity. Using careful analyses and techniques, they boosted the signals of the three innermost planets around the star, but "the signals attributed to the existence of the two controversial planets disappeared, becoming indistinguishable from measurement noise," Mahadevan said. "The disappearance of these two signals after correcting for the star’s activity indicates that these signals in the original data must have been produced by the activity and rotation of the star itself, not by the presence of these two suspected planets.
This image shows the location of the three planets remaining in 2014. Research published in 2014, led by Penn State astronomers, shows that two of the signals previously attributed to planets in the habitable zone actually are created by activity within the star itself. The outer (green) planet shown in the 2010 image now also is believed not to exist, based on work by other researchers since 2010. Blue indicates candidate planets in the habitable zone where conditions might be able to support life, orange indicates detections in the too-hot region that is too close to the star. Credit: NASA/Penn State University
"Our improved detection of the real planets in this system gives us confidence that we are now beginning to sufficiently eliminate Doppler signals from stellar activity to discover new, habitable exoplanets, even when they are hidden beneath stellar noise, said Robertson. "While it is unfortunate to find that two such promising planets do not exist, we feel that the results of this study will ultimately lead to more Earth-like planets."
Older stars such as Gliese 581, an "M dwarf" star in the constellation Libra about one-third the mass of our Sun, have until now been considered highly attractive targets in the search for extraterrestrial life because they are generally less active and so are better targets for Doppler observations. "The new result from our research highlights a source of astrophysical noise even with old M dwarfs because the harmonics of the star's rotation can be in the same range as that of its habitable zone, raising the risk of false detections of nonexistent planets," Mahadevan said. "Higher-precision analysis for discovering Earth-like planets using spectrographs will be increasingly more necessary as next-generation spectrographs with the higher Doppler precision needed for detecting important subtle signatures come on line this decade -- like the Habitable Zone Planet Finder (HPF) that our team now is developing at Penn State." A description of this research is available on the Habitable-zone Planet Finder blog.
In addition to Mahadevan and Robertson, other coauthors of the research include Penn State Graduate Student Arpita Roy and McDonald Observatory Research Scientist Michael Endl at the University of Texas. Penn State coauthors have affiliations with the Center for Exoplanets and Habitable Worlds and with the Astrobiology Research Consortium, both at Penn State.
Additional information about this research and about the Habitable Zone Planet Finder Spectrograph is online. The research received support from the National Science Foundation, the NASA Astrobiology Institute, the Penn State Center for Exoplanets and Habitable Worlds, the Penn State Eberly College of Science, and the Pennsylvania Space Grant Consortium.
[ Barbara K. Kennedy ]