mysterious worlds beyond our own
TRANSCRIPT
Mysterious Worlds Beyond Our Own
Tzvetelina Dimitrova
On Earth, we often find ourselves looking
out into the night sky wondering at the
mysteries that lie beyond the solar system
we call home. What are the planets like
beyond our planetary neighborhood? Could
their landscapes resemble our own? Or
could they hold mysteries beyond our
modern comprehension? On exploring the
topic of mysterious exoplanets, TRAPPIST-
1 is certainly the right place to start.
TRAPPIST-1 is a planetary system located
at a distance of 39 light years (in miles)
from the Sun, within the constellation
Aquarius [1]. The planetary system consists
of at least seven planets (Figure 1), which
orbit about an ultra-cool red dwarf star that
is 12 times less massive than the Sun, and
slightly larger than Jupiter [1]. This system
is of importance in the exoplanet field,
because of its central dwarf star. Planets that
orbit about ultra-cool red dwarfs tend to
have similar planetary characteristics to
earth in several different aspects. The
discovery of seven temperate terrestrial
planets is a significant discovery because
this is the greatest number of planets
detected in any system. Three of these
newly discovered planets are considered to
lie within the habitable zone of the star.
Timeline
Although the central TRAPPIST-1 star
was discovered in 1999 during the Two
Micron All Sky Survey(2MASS) [2], the
detection of a planetary system is a
relatively recent development. In May of
2016, Michael Gillon and his team at the
University of Liege in Belgium published
findings of three Earth-sized planets
orbiting the star. They used the method of
transit photometry, with the Transiting
Planets and Planetesimals Small Telescope
(TRAPPIST) at the La Silla Observatory
in Chile[3]. On June 6th, the first transit of
the planet TRAPPIST-1d was detected!
Not long after, on October 11th, the first
Figure 1 Trappist-1 exoplanetary system NASA/JPL-Caltech image.
transit of planet 1h was observed as well.
Almost a year later, on August 31st 2017,
exciting news broke! A scientific paper
reported Ultraviolet observations, which led
to the suggestion that the outer planets
might host water.
Following these discoveries,
multiple series of scientific papers have
been published on the planets. These new
papers outlined the more recently
discovered characteristics of the system. At
this point, a record-breaking total of seven
planets had been observed. All these seven
planets were discovered using the transit
method, during which the recorded
brightness of a host star is observed for
periodic dips suggesting an orbiting body
(Figure 2). Following these discoveries, the
next course of action called for
investigations into the atmospheric
conditions of the planets, as well as their
habitability and likelihood of liquid water.
Now let us journey far beyond our bounds
on earth, and dive into the most notable
properties of the TRAPPIST-1 planetary
system! The innermost planet,
TRAPPIST-1b, is a rocky planet sharing
some characteristics of our solar systems
very own planet Venus as its atmosphere
is incredibly hot and thick. TRAPPIST 1-
b’s size is comparable to that of Earth,
although its atmosphere has a much
greater reach, and its density is relatively
low. TRAPPIST-1c is the third largest
planet of the system, and it is also the most
massive. Similar to planet 1b in
atmosphere and composition, the most
intriguing fact about this planet is the
proximity of its orbit around the host star,
which causes a year on this planet to last a
mere 58 hours! TRAPPIST-1d is the
smallest planet and falls into the inner
edge of the habitable zone of the red dwarf
star, although recent studies conducted by
the University of Washington suggest it to
be uninhabitable and Venus like [4].
TRAPPIST-1e is a relatively Earth like
exoplanet, with a comparable size, mass,
temperature, and, stellar flux to that of
Earth. Out of all of the planets in the
system, TRAPPIST-1e has the most
potential to be a habitable ocean planet,
and for this fact has been deemed the most
Figure 2 - Spitzer Space Telescope transit data of
TRAPPIST-1. Credit: ESO/M. Gillon et al.TRAPPIST-1
worthy of further study (Figure 3). Further
out into the habitable zone, TRAPPIST-1f is
a partially rocky planet theorized to host
liquid water oceans on its surface under the
right atmospheric conditions. TRAPPIST-1g
is thought to be just barely within, or just
barely outside of the habitable zone, and is
also thought to be a likely candidate to host
some form of water. The last and outermost
planet of the system is TRAPPIST-1h.
Although not significantly smaller than
earth, it has a relatively low density which
suggests the presence of water, and or ice.
At its orbital distance from its host star, this
planet is within the frost line, the point at
which common planetary compounds are
thought to freeze [5]. Regardless of whether
or not the planets of the TRAPPIST-1
system prove to be habitable to human life,
they are surely the first of their kind to be
discovered, and promise to be a hub for
fascinating future research!
Figure 3 "Planet hop from TRAPPIST-1e - Voted best 'hab zone'
vacation within 12 parsecs of Earth" NASA Exoplanets Exploration
Program's Exoplanet Travel Bureau poster
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J. Davy; Liebert, James; Williams, Rik J. (2000). "New
Neighbors from 2MASS: Activity and Kinematics at the
Bottom of the Main Sequence". The Astronomical Journal.
120 (2): 1085–1095. arXiv:astro-ph/0004361.
Bibcode:2000AJ....120.1085G.doi:10.1086/301456.
[3] Gillon, M., Jehin, E., Lederer, S. et al. Temperate Earth-
sized planets transiting a nearby ultracool dwarf star.
Nature 533, 221–224 (2016).
https://doi.org/10.1038/nature17448
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