Dodson-Robinson wants to use Twinkle’s light-spectrum data to develop
a complementary way to search for Earth-like exoplanets and involve UD
students in the process. (Besides her complex research, Dodson-Robinson
teaches a course called “Introduction to Astronomy.”)
Her focus is on a star’s radial velocity — the ever-so slight
elliptical movements of a star in response to a planet’s gravitational
tug. This wobbling, as if the star is using a hula hoop, affects the
star’s light signature. A star moving toward us during that wobble has
light of slightly shorter wavelength, which reads bluer in color, versus
a star moving slightly away from us, which will have a longer
wavelength and thus be redder.
“The surface of a star is a very active place – bubbles arise from
convection, there are flares, areas of strong magnetic fields, the
stalling of gases. If we’re looking at motion,” Dodson-Robinson said,
“how do you separate out this ‘noise’ versus the gravitational pull of a
planet? That’s a big challenge because the wobbling of stars caused by
the tugs from small, Earth-like exoplanets are minuscule and can easily
be masked by this noise.”
Twinkle’s mission is explained in this video provided by Blue Skies Space Ltd.
The hypothesis she’s working on is that at some wavelengths, or
colors of light, you will get more “noise,” or up-and-down motions,
reflecting natural activity on a star’s surface rather than an
exoplanet’s tugging.
“My hope is that, using Twinkle’s data, we can monitor specific
colors and by removing the noise, we can develop models of this stellar
variability and find Earth 2.0 right here from the ground,”
Dodson-Robinson said. “Many exoplanets have been found from the ground,
but not Earth-like ones orbiting sun-like stars.”
Twinkle is expected to provide more than 70,000 hours — nearly eight
years — of observational data once it launches in 2024. Robinson’s work
will complement other Twinkle research on the atmospheres of exoplanets
to determine their habitability.
Finding another Earth out there will take extensive searching and
validation. How close is a prospective candidate to its sun-like star?
Does it have an atmosphere rich in oxygen, an ozone layer for protection
against ultraviolet radiation, liquid water on the surface, and so on?
Such “checklists” for livability are very involved, Dodson-Robinson
said, driving intense climate modeling efforts in the search for other
planets that can sustain life.