NASA's TESS tunes into an all-sky 'symphony' of red giant stars

Date:
August 5, 2021
Source:
NASA/Goddard Space Flight Center
Summary:
Using observations from NASA's Transiting Exoplanet Survey Satellite
(TESS), astronomers have identified an unprecedented collection
of pulsating red giant stars all across the sky. These stars,
whose rhythms arise from internal sound waves, provide the opening
chords of a symphonic exploration of our galactic neighborhood.



FULL STORY ========================================================================== Using observations from NASA's Transiting Exoplanet Survey Satellite
(TESS), astronomers have identified an unprecedented collection of
pulsating red giant stars all across the sky. These stars, whose rhythms
arise from internal sound waves, provide the opening chords of a symphonic exploration of our galactic neighborhood.


==========================================================================
TESS primarily hunts for worlds beyond our solar system, also known as exoplanets. But its sensitive measurements of stellar brightness make
TESS ideal for studying stellar oscillations, an area of research called asteroseismology.

Hon presented the research during the second TESS Science Conference,
an event supported by the Massachusetts Institute of Technology in
Cambridge -- held virtually from Aug. 2 to 6 -- where scientists discuss
all aspects of the mission. The Astrophysical Journal has accepted a
paper describing the findings, led by Hon.

Sound waves traveling through any object -- a guitar string, an organ
pipe, or the interiors of Earth and the Sun -- can reflect and interact, reinforcing some waves and canceling out others. This can result in
orderly motion called standing waves, which create the tones in musical instruments.

Just below the surfaces of stars like the Sun, hot gas rises, cools,
and then sinks, where it heats up again, much like a pan of boiling
water on a hot stove. This motion produces waves of changing pressure --
sound waves -- that interact, ultimately driving stable oscillations with periods of a few minutes that produce subtle brightness changes. For
the Sun, these variations amount to a few parts per million. Giant
stars with masses similar to the Sun's pulsate much more slowly, and
the corresponding brightness changes can be hundreds of times greater.

Oscillations in the Sun were first observed in the 1960s. Solar-like oscillations were detected in thousands of stars by the French-led
Convection, Rotation and planetary Transits (CoRoT) space telescope,
which operated from 2006 to 2013. NASA's Kepler and K2 missions, which
surveyed the sky from 2009 to 2018, found tens of thousands of oscillating giants. Now TESS extends this number by another 10 times.



========================================================================== "With a sample this large, giants that might occur only 1% of the time
become pretty common," said co-author Jamie Tayar, a Hubble Fellow at
the University of Hawaii. "Now we can start thinking about finding even
rarer examples." The physical differences between a cello and a violin
produce their distinctive voices. Similarly, the stellar oscillations astronomers observe depend on each star's interior structure, mass,
and size. This means asteroseismology can help determine fundamental
properties for large numbers of stars with accuracies not achievable in
any other way.

"Our initial result, using stellar measurements across TESS's first
two years, shows that we can determine the masses and sizes of these oscillating giants with precision that will only improve as TESS goes
on," said Marc Hon, a NASA Hubble Fellow at the University of Hawaii
in Honolulu. "What's really unparalleled here is that TESS's broad
coverage allows us to make these measurements uniformly across almost
the entire sky." When stars similar in mass to the Sun evolve into red
giants, the penultimate phase of their stellar lives, their outer layers
expand by 10 or more times.

These vast gaseous envelopes pulsate with longer periods and larger
amplitudes, which means their oscillations can be observed in fainter
and more numerous stars.

TESS monitors large swaths of the sky for about a month at a time using
its four cameras. During its two-year primary mission, TESS covered about
75% of the sky, each camera capturing a full image measuring 24-by-24
degrees every 30 minutes. In mid-2020, the cameras began collecting
these images at an even faster pace, every 10 minutes.



==========================================================================
The images were used to develop light curves -- graphs of changing
brightness - - for nearly 24 million stars over 27 days, the length of
time TESS stares at each swath of the sky. To sift through this immense accumulation of measurements, Hon and his colleagues taught a computer
to recognize pulsating giants. The team used machine learning, a form
of artificial intelligence that trains computers to make decisions based
on general patterns without explicitly programming them.

To train the system, the team used Kepler light curves for more than
150,000 stars, of which some 20,000 were oscillating red giants. When
the neural network finished processing all of the TESS data, it had
identified a chorus of 158,505 pulsating giants.

Next, the team found distances for each giant using data from ESA's (the European Space Agency's) Gaia mission, and plotted the masses of these
stars across the sky. Stars more massive than the Sun evolve faster,
becoming giants at younger ages. A fundamental prediction in galactic
astronomy is that younger, higher-mass stars should lie closer to the
plane of the galaxy, which is marked by the high density of stars that
create the glowing band of the Milky Way in the night sky.

"Our map demonstrates for the first time empirically that this is indeed
the case across nearly the whole sky," said co-author Daniel Huber,
an assistant professor for astronomy at the University of Hawaii. "With
the help of Gaia, TESS has now given us tickets to a red giant concert in
the sky." TESS is a NASA Astrophysics Explorer mission led and operated
by MIT in Cambridge, Massachusetts, and managed by NASA's Goddard Space
Flight Center.

Additional partners include Northrop Grumman, based in Falls Church,
Virginia; NASA's Ames Research Center in California's Silicon Valley;
the Center for Astrophysics | Harvard & Smithsonian in Cambridge, Massachusetts; MIT's Lincoln Laboratory; and the Space Telescope
Science Institute in Baltimore. More than a dozen universities, research institutes, and observatories worldwide are participants in the mission.

========================================================================== Story Source: Materials provided by
NASA/Goddard_Space_Flight_Center. Original written by Francis Reddy. Note: Content may be edited for style and length.


========================================================================== Related Multimedia:
*
Visualization_of_oscillating_red_giant_stars;_related_audio_and_images ========================================================================== Journal Reference:
1. Marc Hon, Daniel Huber, James S. Kuszlewicz, Dennis Stello, Sanjib
Sharma, Jamie Tayar, Joel C. Zinn, Mathieu Vrard, Marc
H. Pinsonneault. A 'Quick Look' at All-Sky Galactic Archeology
with TESS: 158,000 Oscillating Red Giants from the MIT Quick-Look
Pipeline. The Astrophysical Journal, 2021 (accepted); [abstract] ==========================================================================

Link to news story: https://www.sciencedaily.com/releases/2021/08/210805141136.htm

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