Simulation of a
planet transiting its host star by Exoplanet Watch volunteer Guiseppe Conzo.
Credits: Guiseppe Conzo
Exoplanets, look out! Two
NASA-funded teams of amateur astronomers are tracking you with their backyard
telescopes.
These two teams, called UNITE (UNISTELLAR Network Investigating TESS
Exoplanets) and Exoplanet
Watch, have
combined forces to confirm a new planetary discovery—a toasty "warm
Jupiter".
"I pinch myself every day when
I recall that I have made a meaningful scientific contribution to astronomy by
helping professional astronomers confirm and characterize a new exoplanet,”
said Darren Rivett, a volunteer from Australia who contributed to the
effort.
Planets around other stars, called
exoplanets, sometimes block the light from the stars they orbit. When this
happens, it’s called a “transit”. Amateur astronomers can observe exoplanet
transits with their own telescopes by watching for the light from a nearby star
to dim.
NASA's Transiting
Exoplanet Survey Satellite (TESS) sees these dimming events, too—many
thousands of them. But just seeing a star dim once is not enough. You need to
catch multiple dimming events (and perform various other checks) to
know that you’ve found a new exoplanet.
That’s where volunteers from
the UNITE and Exoplanet Watch projects come in.
These two teams of amateur
astronomers have collaborated with the SETI Institute to detect the transit of
an object called TIC 393818343 b (aka TOI 6883 b)---proving to the world that
this object does indeed contain a planet orbiting a star.
First, the
UNISTELLAR and SETI Institute team saw a single transit signal
detected by the TESS space telescope. They gathered data to predict when the
planet would transit again. They then alerted the UNITE and Exoplanet Watch amateurs to help observe the host star for signs of a transiting
planet during the predicted time. The observations from the two networks
showed two new transit detections, confirming the predictions, and
demonstrating that a planet indeed causes the signals.
This newly discovered giant planet
falls into the "warm Jupiter" category of exoplanets, meaning
it orbits closer to its host star than Jupiter, or even the Earth does.
Astronomers have even predicted that it might, under certain circumstances,
migrate still further inward toward its star to become a "hot Jupiter.”
Hot or not, thanks to some terrific teamwork, we are now one step closer to
understanding the population of planets that lies outside our own Solar
System. The news is now published in the Astronomical Journal,
and all the citizen scientists involved, including a high school student,
are co-authors on this scientific
publication, “Confirmation and Characterization of the Eccentric, Warm Jupiter
TIC 393818343 b with a Network of Citizen Scientists”.
UNITE (UNISTELLAR Network Investigating TESS
Exoplanets) uses the global network of observers with UNISTELLAR telescopes to
gather data on TESS exoplanet candidates and long-duration exoplanet transits.
To get involved, no matter what kind of telescope you have, visit https://science.unistellar.com/exoplanets/unite/ or reach out to citizenscience@unistellaroptics.com.
Participation is open to everyone,
regardless of citizenship. “What I find amazing about the NASA citizen science
project is that they involve people from all around the world contributing
meaningful observation data that leads to incredible discoveries!” Sophie
Saibi, a high school student from California who
participated. “Researching as a citizen scientist is something I highly
recommend to anyone who gazes at the night sky with awe and wonder,” said
Rivett.
Congratulations to everyone on the
team! The amateur astronomers who coauthored this paper are listed below.
- Mario Billiani
- Robert Gagliano
- Martti H. Kristiansen
- Thomas Lee Jacobs
- Daryll M. LaCourse
- Georgios Lekkas
- Margaret Loose
- Bryan Martin
- Nicola Meneghelli
- Mark Omohundro
- Darren Rivett
- Fadi Saibi
- Sophie Saibi
- Hans M. Schwengeler
- Ivan A. Terentev
- Daniel Zaharevitz
By: NASA Science Editorial Team
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