Astronomy

(Tina Meador) #1

28 ASTRONOMY • JANUARY 2018


One of humanity’s greatest discov-
eries will be the confirmation that
life exists elsewhere in our uni-
verse. We haven’t made this dis-
covery yet, but each year, astrono-
mers move closer to that goal. This
past year was no exception.
In February, a team of planetary
scientists announced — both at a
press conference and in a Nature
article — that it had found seven
Earth-sized planets orbiting a
nearby star. All seven were within
the so-called habitable zone.
Inside this region, the amount of
starlight the exoplanets receive
could lead to ideal temperatures
for liquid water on those worlds’
surfaces. (Though just because
a planet is in the habitable zone
doesn’t mean there’s water.) The
researchers also ran computer
models and estimated that three
of those exoplanets could harbor
water oceans on their surfaces,
provided those worlds also have
Earth-like atmospheres.
To find these seven worlds,
astronomers used several
ground-based telescopes in
addition to the infrared Spitzer
Space Telescope to focus on the
star known as TRAPPIST-1. They
watched as its starlight flickered.
From their hours of data, the
researchers determined the flick-
ering was due to multiple planets
crossing in front of the star, block-
ing a tiny amount of starlight at
each crossing. As of February,
they could confirm six exoplan-
ets in orbit around TRAPPIST-1.
Confirmation of the seventh

world, which orbits farthest from
the star, came in May. And there
could even be more exoplanets in
the system.
From the amount of light each
exoplanet blocked, the astrono-
mers could calculate its diameter.
By analyzing the amount of time
that passed between subsequent
transits of the same exoplanet,
and comparing the six different
inner worlds’ orbits, the scien-
tists could also estimate those
exoplanets’ masses. With diam-
eter and mass, you can calculate
density. The calculations suggest
the six inner worlds are rocky like
Earth, Mars, Venus, and Mercury,
although the numbers are still
highly uncertain. (The seventh
exoplanet’s density has even
greater uncertainty.)
While the exoplanets might be
rocky and Earth-sized, their star is
nothing like the Sun. TRAPPIST-1
holds only 8 percent of the Sun’s
mass and is about 12 percent of
the width of our star. It is also
much cooler, giving off a red glow
instead of our Sun’s yellow-white
light. This planetary system is
also far more condensed than
our solar system. The innermost
planet completes an orbit around
TRAPPIST-1 in 1.5 days, whereas
the most distant one takes 18.8
days. Even though astronomers
haven’t found an exact solar
system analogue, the discovery
of seven likely terrestrial planets
orbiting a star only 40 light-years
away is a good indication that an
Earth twin may be out there.


  • BepiColombo, the European-
    Japanese collaborative mis-
    sion to Mercury, is set to
    launch in October.

  • SpaceX is still hoping for
    crewed missions to start up
    in 2018.

  • NASA’s next space-based
    exoplanet observatory, the
    Transiting Exoplanet Survey
    Satellite (TESS), launches in
    early 2018.

  • The agency’s InSight
    (Interior Exploration using
    Seismic Investigations,
    Geodesy and Heat
    Transp or t) mission to Mar s
    has a launch window begin-
    ning May 5, and a landing
    date of November 26.

  • The X-ray satellite
    Spectrum-Roentgen-
    Gamma (SRG) will launch
    in 2018. This Russian and
    German collaboration proj-
    ect will scan the entire sky
    and is expected to discover
    millions of supermassive
    black holes. — L.K.


Te r r e s t r i a l p l a n e t


plethora


The TRAPPIST-1 system
contains at least
seven planets circling
an M-dwarf star. All
seven appear Earth-
sized and terrestrial
in nature, prompting
astronomers to
wonder whether they
might also host life.
NASA/JPL-CALTECH
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