293
have proved to be false positives
but, after three years of analysis,
the program had identified 1,284
exoplanets, with more than 3,000
stars left to examine. The statistics
for the exoplanets in the Kepler field
are striking—most stars are part
of a planetary system. This means
that the number of planets in the
universe is likely to exceed the
number of stars.
The amount of dimming during
a transit gives an indication of how
big an exoplanet might be, but the
study of an exoplanet’s size and
characteristics is still in its early
stages. The light reflected from
a planet is about 10 billion times
fainter than the star it orbits.
Astronomers are waiting for the
James Webb Space Telescope in
2018 and the European Extremely
Large Telescope in 2024 to image
this light directly and analyze the
chemistry of exoplanets. Until then,
they have to speculate using very
little data: an approximate mass
of the planet, its radius, the orbital
distance, and the temperature
of the star. This tells them what
the planet is probably made of
and allows them to conjecture
what the surface conditions are
likely to be.
Hot and super Jupiters
The exoplanets discovered so far
have added a host of weird worlds
to the neat family portrait that is
the sun’s planetary system. For
THE TRIUMPH OF TECHNOLOGY
example, 51 Pegasi b was the first
of many “hot Jupiters.” These have
a mass similar to Jupiter’s and a
large size that shows that they are
mostly made of gas. 51 Pegasi b is
half as massive as Jupiter, but is
slightly larger. This gas giant orbits
its sunlike star every four days.
That means it is much closer to
its star than Mercury is to the sun.
Such proximity means it is tidally
locked to the star—one side always
faces the scorching stellar surface,
and the other always faces away.
Many hot Jupiters have been found.
They have confounded scientists,
who are trying to understand how
gas planets can exist so close to
a star without evaporating. Some
exoplanets are dozens of times
more massive than Jupiter, and
are known as “super-Jupiters.” ❯❯
We were not expecting
to find a planet with a
4-day [orbital] period. No
one was expecting this.
Michel Mayor
The “super-Jupiter” Kappa
Andromedae b, shown here in an
artist’s render, has a mass of 13 times
Jupiter’s. It glows a reddish color, and
may yet be reclassed as a brown dwarf.