A warm Jupiter orbiting a cool star

Date:
September 14, 2020
Source:
Penn State
Summary:
A planet observed crossing in front of, or transiting, a low-mass
star has been determined to be about the size of Jupiter.



FULL STORY ==========================================================================
A planet observed crossing in front of, or transiting, a low-mass star
has been determined to be about the size of Jupiter. While hundreds of Jupiter-sized planets have been discovered orbiting larger sun-like stars,
it is rare to see these planets orbiting low-mass host stars and the
discovery could help astronomers to better understand how these giant
planets form.


========================================================================== "This is only the fifth Jupiter-sized planet transiting a low-mass star
that has been observed and the first with such a long orbital period,
which makes this discovery really exciting," said Caleb Can~as, lead
author of the paper and a Ph.D. student at Penn State and NASA Earth
and Space Science Fellow.

Originally detected by NASA's Transiting Exoplanet Survey Satellite
(TESS) spacecraft, astronomers characterized the planet's mass, radius,
and its orbital period using the Habitable-zone Planet Finder (HPF),
an astronomical spectrograph built by a Penn State team and installed
on the 10m Hobby-Eberly Telescope at McDonald Observatory in Texas. A
paper describing the research appears in the September 2020 issue of
the Astronomical Journal and is publicly accessible on arXiv.

"A transiting Jupiter-sized planet is amenable to further observations
to see how well the orbit is aligned with the spin-axis of the host star
and to constrain how it could have formed," said Can~as. "Furthermore, the
low mass of the host star and the long orbital period result in a Jupiter
with a moderate temperature compared to similar planets detected with
NASA's Kepler space telescope." The host star, TOI-1899, is a low-mass
(M dwarf) star about 419 light years away from Earth. The planet, TOI-1899
b, is two-thirds the mass of Jupiter, ten percent larger in radius than Jupiter, and is 0.16 astronomical units (AU) -- a measure defined as
the distance between the Earth and the sun -- from its host star such
that a full year on TOI-1899 takes only 29 Earth days. For comparison,
the four other transiting Jupiter-size planets around comparable stars
complete their orbits in less than 4 days.

The planet was detected by TESS using the transit method, which searches
for stars showing periodic dips in their brightness as a telltale sign of
an orbiting object crossing in front of the star and blocking a portion
of its light. The signal was later confirmed as a planet using precision observations from the HPF spectrograph that measure the planet's mass
by analyzing how it causes its host start to the wobble.

From a formation and orbital evolution perspective, there is not a clear dividing line between warm Jupiters and the large planets even closer
to their host stars, the more commonly discovered hot Jupiters.

"Warm Jupiters like TOI-1899 b orbit surprisingly close to their star,"
said Rebekah Dawson, assistant professor of astronomy and astrophysics
at Penn State and an author of the paper. "Even though the planet's
orbital period is long compared to many other giant planets detected
and characterized through the transit method, it still places the giant
planet much closer to its star than we'd expect from classical formation theories. Detailed characterization of their physical and orbital
properties, system architecture, and host stars - - as the HPF team
has done for TOI-1899 b -- allow us test theories for how giant planets
can form or be displaced so close to their star." The Habitable-zone
Planet Finder was delivered to the 10m Hobby Eberly Telescope at
McDonald Observatory in late 2017, and started full science operations
in late 2018. HPF is designed to detect and characterize planets in
the Habitable-zone -- the region around the star where a planet could
sustain liquid water on its surface -- around nearby M-dwarf stars,
but is also capable of making sensitive measurements for planets outside
the habitable zone.

"This warm Jupiter is a compelling target for atmospheric characterization
with upcoming missions like the James Webb Space Telescope," said Suvrath Mahadevan, professor of astronomy and astrophysics at Penn State, the
principal investigator of the HPF spectrograph, and an author of the
paper. "HPF was critical in helping us to confirm this, but detecting
a second transit is important to very precisely pin down its period."
In addition to data from HPF, additional data were obtained with the
3.5m Telescope at the Kitt Peak National Observatory (KPNO) in Arizona
and the 3m Shane Telescope at Lick Observatory for high contrast imaging
and photometric observations with the 0.9m WIYN Telescope at KPNO, 0.5
m ARCSAT telescope at Apache Point Observatory, and the 0.43 m telescope
at the Richard S. Perkin Observatory in New York.


========================================================================== Story Source: Materials provided by Penn_State. Original written by Sam Sholtis. Note: Content may be edited for style and length.


========================================================================== Journal Reference:
1. Caleb I. Can~as, Gudmundur Stefansson, Shubham Kanodia, Suvrath
Mahadevan, William D. Cochran, Michael Endl, Paul Robertson, Chad F.

Bender, Joe P. Ninan, Corey Beard, Jack Lubin, Arvind F. Gupta,
Mark E.

Everett, Andrew Monson, Robert F. Wilson, Hannah M. Lewis,
Mary Brewer, Steven R. Majewski, Leslie Hebb, Rebekah I. Dawson,
Scott A. Diddams, Eric B. Ford, Connor Fredrick, Samuel Halverson,
Fred Hearty, Andrea S.

J. Lin, Andrew J. Metcalf, Jayadev Rajagopal, Lawrence W. Ramsey,
Arpita Roy, Christian Schwab, Ryan C. Terrien, Jason T. Wright. A
Warm Jupiter Transiting an M Dwarf: A TESS Single-transit Event
Confirmed with the Habitable-zone Planet Finder. The Astronomical
Journal, 2020; 160 (3): 147 DOI: 10.3847/1538-3881/abac67 ==========================================================================

Link to news story: https://www.sciencedaily.com/releases/2020/09/200914114122.htm

--- up 3 weeks, 6 hours, 50 minutes
* Origin: -=> Castle Rock BBS <=- Now Husky HPT Powered! (1337:3/111)