MSGID: 1:317/3 6482ab1e
PID: hpt/lnx 1.9.0-cur 2019-01-08
TID: hpt/lnx 1.9.0-cur 2019-01-08
 'Hot Jupiters' may not be orbiting alone 

  Date:
      June 8, 2023
  Source:
      Indiana University
  Summary:
      Astronomers challenge longstanding beliefs about the isolation of
      'hot Jupiters' and proposes a new mechanism for understanding the
      exoplanets' evolution.


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FULL STORY
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Research led by an Indiana University astronomer challenges longstanding
beliefs about the isolation of "hot Jupiters" and proposes a new mechanism
for understanding the exoplanets' evolution.

While our Jupiter is far away from the sun, hot Jupiters are gas giant
planets that closely orbit stars outside our solar system for an orbital
period of less than 10 days. Previous studies suggested they rarely
have any nearby companion planets, leading scientists to believe that
hot Jupiters formed and evolved through a violent process that expelled
other planets from the area as they moved closer to their host stars. The
research team's findings reveal that hot Jupiters do not always orbit
alone.

"Our research shows that at least a fraction of hot Jupiters cannot form
through a violent process," said Songhu Wang, assistant professor of
astronomy in the College of Arts and Sciences. "This is a significant
contribution to advance our understanding of hot Jupiter formation,
which can help us learn more about our own solar system."  Wang presented
the results of the research at the June 2023 meeting of the American
Astronomical Society in Albuquerque, New Mexico.

Researchers analyzed the full, four-year data set for hot and warm
Jupiters from NASA's Kepler Mission. Warm Jupiters have a longer orbital
period that ranges from 10 to 300 days. Researchers used transit timing
variations to determine that at least 12% of hot Jupiters and 70% of
warm Jupiters have a nearby planetary companion orbiting their host stars.

Wang and his collaborators combined their results with existing
observational constraints to propose a new framework for explaining
the evolution of hot and warm Jupiters and why some have companion
planets. They determined that the makeup of hot and warm Jupiter systems
depends on the occurrence of gas giants in the system, which impacts
how much the planets interact and migrate.

The findings provide a launching point into future research about
exoplanets and our solar system's planets.

"The ultimate goal for astronomers is to set our solar system into
the bigger picture -- 'Are we unique?'" Wang said. "This helps us
to understand why we don't have a hot Jupiter in our solar system."
Additional collaborators are Dong-Hong Wu, lecturer in the Department of
Physics at Anhui Normal University, and Malena Rice, 51 Pegasi b Fellow
at the Massachusetts Institute of Technology and incoming professor at
Yale University.

Wang has long been interested in the configurations and demographics of
exoplanets. He uses observational research to try to understand their
dynamics and origins, helping astronomers better understand how our
solar system fits into a larger cosmic context.

    * RELATED_TOPICS
          o Space_&_Time
                # Extrasolar_Planets # Solar_System # Stars # Sun #
                Astronomy # Jupiter # Solar_Flare # Pluto
    * RELATED_TERMS
          o Astronomy o Extrasolar_planet o Radio_telescope
          o Antikythera_mechanism o Dysnomia_(moon_of_Eris) o
          Stellar_evolution o Astrobiology o Shape_of_the_Universe

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Story Source: Materials provided by Indiana_University. Note: Content
may be edited for style and length.


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Link to news story:
https://www.sciencedaily.com/releases/2023/06/230608195742.htm

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