The Penn State-led Habitable Zone Planet
Finder (HPF) provides the highest precision measurements to date of infrared
signals from nearby stars. Pictured: The HPF instrument during installation in
its clean-room enclosure in the Hobby Eberly Telescope at McDonald Observatory.
Credit: Guðmundur Stefánssonn/Penn State
The
discovery of a possible "super-Earth" less than 20 light-years from
our own planet is offering scientists new hope in the hunt for other worlds
that could harbor life, according to an international team including
researchers from Penn State. They dubbed the exoplanet, named GJ 251 c, a
"super-Earth" as data suggest it is almost four times as massive as
Earth, and likely to be a rocky planet.
"We look for these types of planets
because they are our best chance at finding life elsewhere," said Suvrath
Mahadevan, the Verne M. Willaman Professor of Astronomy at Penn State and
co-author of a paper about the discovery published in The Astronomical Journal.
"The exoplanet is in the habitable
or the 'Goldilocks Zone,' the right distance from its star that liquid water
could exist on its surface, if it has the right atmosphere."
For decades, the search for planets that
might host liquid water, and perhaps life, has driven astronomers to design and
construct advanced telescopes and computational models capable of detecting
even the faintest signals from starlight.
This latest discovery was the result of
two decades of observational data and offers one of the most promising
prospects yet for searching for signs of life on other planets, Mahadevan said.
The exoplanet was found using data from
the Habitable-Zone Planet Finder (HPF), a high-precision, near-infrared
spectrograph—a complex prism that breaks apart signals from starlight—fixed to
the Hobby-Eberly Telescope at the McDonald Observatory in Texas.
Penn State researchers led the design
and construction of the HPF, built to detect Earth-like planets in the
habitable zones of nearby stars.
"We call it the Habitable Zone
Planet Finder, because we are looking for worlds that are at the right distance
from their star that liquid water could exist on their surface. This has been the
central goal of that survey," Mahadevan said.
"This
discovery represents one of the best candidates in the search for atmospheric
signature of life elsewhere in the next five to ten years."
Mahadevan
and his colleagues made the discovery by analyzing a vast collection of data,
spanning over 20 years and collected by telescopes around the world, focusing
on the slight movement, or "wobble," of the planet's host star, GJ
251. This "wobble" comprises tiny Doppler shifts in the star's light
caused by an orbiting planet's gravity.
They
used the baseline observations to first improve the "wobble"
measurements of a previously known inner planet, GJ 251 b, which circles the
star every 14 days.
They
then combined the baseline data with new high-precision data from the HPF to
reveal a second, stronger signal at 54 days—indicating there was another, far
more massive, planet in the system.
The
team further confirmed the planet's signal using the NEID spectrometer built by Penn State
researchers, which is attached to a telescope at the Kitt Peak National
Observatory in Arizona.
"We
are at the cutting edge of technology and analysis methods with this
system," said Corey Beard, corresponding author on the paper who conducted
the research while earning a doctorate in astrophysics from the University of
California, Irvine.
"We need the next generation of telescopes to directly image this candidate, but what we also need is community investment."
One
of the biggest challenges in finding distant worlds is disentangling the
planetary signal from its star's own activity, a kind of stellar weather,
Mahadevan explained.
Stellar activity, such as starspots, can
mimic the periodic motion of a planet, giving the false impression of a planet
where there is none.
To
distinguish signal from noise, the researchers applied advanced computational
modeling techniques to analyze how signals change across different wavelengths,
or colors, of light.
"This is a hard game in terms of
trying to beat down stellar activity as well as measuring its subtle signals,
teasing out slight signals from what is essentially this frothing,
magnetospheric cauldron of a star surface," Mahadevan said.
He explained that discovering exoplanets
like GJ 251 c requires advanced instruments and complex data analysis. The work
involves collaborations across multiple institutions and expertise throughout
the world, and most importantly, requires a sustained commitment from the
countries funding the research—which can often take decades to yield actionable
results.
"This discovery is a great example
of the power of multi-disciplinary research at Penn State," said Eric
Ford, distinguished professor of astronomy and astrophysics and director of
research for Penn State's Institute of Computational & Data Sciences
(ICDS).
"Mitigating stellar activity noise
required not just cutting-edge instrumentation and telescope access, but also
customizing the data science methods for the specific needs of this star and
combination of instruments. The combination of exquisite data and
state-of-the-art statistical methods enabled
our interdisciplinary team to transform data into an exciting discovery that
paves the way for future observatories to search for evidence of life beyond
our solar system."
While the exoplanet that the team
discovered is not possible to image with current instruments, Mahadevan said,
the next generation of telescopes would be able to analyze the planet's
atmosphere, which could potentially reveal chemical signs of life.
"We are always focused on the
future," he said. "Whether that's making sure the next generation of
students can engage in cutting-edge research or designing and building new
technology to detect potentially habitable planets."
The newly found exoplanet is perfectly
positioned for direct observation by more advanced technology. Mahadevan and
his students are already planning for when more powerful telescopes, the new
generation of 30-meter-class ground-based telescopes, come online. Equipped
with advanced instruments, the new telescopes are expected to have the
capability to image nearby rocky planets in habitable zones.
"While we can't yet confirm the
presence of an atmosphere or life on GJ 251 c, the planet represents a
promising target for future exploration," Mahadevan said.
"We made an exciting discovery, but there's still much more to learn about this planet."
Source: Newly discovered 'super-Earth' offers prime target in search for alien life


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