Download Extreme Tidal Waves in Binary Star Systems

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

IAU definition of planet wikipedia , lookup

Lyra wikipedia , lookup

Observational astronomy wikipedia , lookup

Cygnus (constellation) wikipedia , lookup

History of astronomy wikipedia , lookup

Hipparcos wikipedia , lookup

International Ultraviolet Explorer wikipedia , lookup

Astronomical unit wikipedia , lookup

Ursa Major wikipedia , lookup

CoRoT wikipedia , lookup

Astrobiology wikipedia , lookup

Lunar theory wikipedia , lookup

Ursa Minor wikipedia , lookup

History of Solar System formation and evolution hypotheses wikipedia , lookup

Future of an expanding universe wikipedia , lookup

Aquarius (constellation) wikipedia , lookup

Orrery wikipedia , lookup

Stellar evolution wikipedia , lookup

Formation and evolution of the Solar System wikipedia , lookup

Definition of planet wikipedia , lookup

Geocentric model wikipedia , lookup

Stellar kinematics wikipedia , lookup

Comparative planetary science wikipedia , lookup

R136a1 wikipedia , lookup

Extraterrestrial skies wikipedia , lookup

Corvus (constellation) wikipedia , lookup

Rare Earth hypothesis wikipedia , lookup

Extraterrestrial life wikipedia , lookup

Planetary habitability wikipedia , lookup

Dialogue Concerning the Two Chief World Systems wikipedia , lookup

Timeline of astronomy wikipedia , lookup

Transcript
Extreme Tidal Waves in Binary Star Systems
Jim Fuller is..
If you have ever been to the beach, you have seen tides at work.
The ocean slowly recedes from the shore, revealing colonies of
sea shells on the sand deposited the water’s wake. A few hours
later, the ocean creeps back, slowly devouring the sand castles
misfortunate enough to stand within its watery grasp. The tides
in the ocean are caused by the gravitational pull of the Moon
(and to a smaller extent, the Sun). As the Earth rotates through
the gravitational field of the Moon, it is stretched by tidal forces,
slightly distorting the Earth into an elliptical shape. The ocean
rises and recedes in order to adjust to the changing shape of its
basin, causing the smooth ebb and flow of daily tides. On Earth,
theses tides are peaceful, predictable, and passive.
Since tides are much stronger in
stars that orbit each other closely,
the tides in compact binary white
dwarfs can be extremely powerful.
For instance, consider the binary
white dwarf system SDSS J0651.
This system is composed of two
white dwarfs slightly larger than
the Earth and nearly as massive as
the Sun, but closer to one another
than the Earth is to the Moon.
Whereas it takes the Moon nearly
a month to orbit around
the Earth, these stars
orbit each other in just
under thirteen minutes.
On Earth, the tides raised
by the Moon are a couple
feet high. In SDSS J0651,
the tides are over 100
miles high.
In star systems like
SDSS J0651, the tides
are not only impressively
large, but they also have
important consequences
The two white dwarfs of J0651 where once like our sun, but they have
for the evolution of the
burned down to become much smaller and more massive. The larger star
stars. One of the effects
is about the size of Neptune and about a quarter of the mass of the sun.
of tides is to synchronize
The other one is half the sun’s mass and only about the size of the earth.
the spin and orbital
A penny made of this white dwarf’s material would weigh about 1,000
periods of the stars, such
pounds on earth. They are closer to each other than the earth is to the
moon and orbit each other at a speed of 70 miles per second, or 180 times that one side of each
faster than the fastest jet on earth. Not only do they make a complete orbit star is always facing its
companion. In the Earthin just 13 minutes, they also exert a mutual gravitational pull so strong
Moon system, tides
that the lower-mass star is deformed by three percent. If the earth bulged
have synchronized the
by the same amount, we would have tides 120 miles high.
Moon with the Earth,
Image: XXXXXXXXXXXXXXXXX.
so we only see the near
side of the Moon. It will
In binary star systems, tides can be much more volatile. Tidal
take another few billion years to
interactions are particularly intense in compact binary white dwarf
synchronize the Earth with the
systems. White dwarfs are the burnt out cores of stars like the
Moon, and once this happens, the
Sun. They are small compared to their living stellar counterparts:
Moon will only be visible from
most white dwarfs are approximately the size of the Earth. Yet
one side of the Earth! However, the
despite their small size, white dwarfs are roughly the same mass
physics of tidal synchronization
as the Sun, meaning that they are about a million times denser
is
poorly
understood,
and
than the water in our ocean, and a billion times denser than the air
astronomers have been unsure
in our atmosphere. The small size and large mass of white dwarfs
means that they can orbit each other at relatively small distances.
Continued p. 6
5
The enormous
gravitational pull
of Jupiter on Io is
compounded by
that of other nearby
moons—Europa,
Callisto, and
Ganymede. Jupiter
pulls Io toward itself,
while the gravity of
the outer moons pulls
it in the opposite
direction. These tidal
forces alternately
squeeze and stretch
Io’s interior, making
its surface rise and
fall by some 300
ft. This friction
generates enormous
amounts of heat and
pressure, causing
molten material and
gases to rise through
fractures in the
crust and erupt onto
the surface of Io as
volcanoes.
Image: NASA/JPL.
Extreme Tidal Waves
This diagram shows tidally
excited waves ringing inside a
star. Tides excite large scale,
global deformations of the
stars in binary systems such
that they “ring” like bells. The
friction created in the process
contributes to synchronize
and heat the stars. In turn,
the heating may reignite
thermonuclear fusion, which
normally has ceased in white
dwarfs, and cause them to
erupt as novas.
(cont.)
how tidal processes operate in white dwarfs. Since the orbits of
these stars decay until they merge, it is unknown whether the stars
will be able to synchronize before the collision. And what happens
during the collision (it could create a supernova) is dependent on
whether the stars are synchronized.
Image: XXXXXXXXX
Furthermore, the friction created by large tides will induce
substantial heating of the stars. In Jupiter’s moon, Io, tidal forces
scrunch the moon back and forth, causing frictional heating in
its interior. These kinds of tides are similar to the heating of a
racquet ball after it is hit repetitively. Such tidal heating powers
huge volcanoes on Io, and they may create a giant ocean capable
of sustaining life on Europa, another moon of Jupiter. In systems
like J0651, the heating may make the stars shine much brighter
than they otherwise would. In some cases, it may even be powerful
enough to reignite thermonuclear fusion in the white dwarfs.
There are two ways that tides can synchronize (and heat) stars in
compact binary systems. The first is through the force of friction
created as the stars are stretched back and forth, as described above. The second way that tides can affect stars is by exciting large scale
waves that move within the stars. These waves are periodic global deformations of the star, similar to the ringing of a bell. As the stars
orbit one another, they continually “ring” one another, and the friction created by the waves within the stars helps synchronize them
and heat them. My research has shown that this second method is extremely important for white dwarfs, and that it is able to quickly
synchronize systems such as J0651. Furthermore, the heat produced by this ringing can reignite thermonuclear fusion within the stars,
causing them to erupt in a violent outburst called a nova.
In addition to binary white dwarf systems, the effects of tides
have important implications for newly discovered exoplanetary
systems. In many of the recently discovered solar systems
beyond our own, there are planets that orbit their star in a matter
of days, much faster than Mercury orbits our Sun. For these
planets, the tides are strong enough to synchronize the planet
with the star, such that it is permanent day time on one side of
the planet and permanent night time on the other. In some cases,
tides may cause the orbits of the planets to decay until they are
swallowed by their host stars. In other cases, tides may heat
the planet enough to melt it entirely, or cause its atmosphere to
escape into space.
Even in less extreme cases, tides will have a profound impact
on the planetary climate and on the prospects for life on other
planets. Without tidal interactions between the Earth and Moon,
the day would only be a few hours long, and life as we know it
would not be able to exist. We must therefore continue to study
tidal interactions as we search for life beyond Earth. In the
process, we can learn a little more about how tides have affected
life right here at home, and what we can expect as we look into
the future.
–Jim Fuller
Artist’s conception of Kepler-10b, a rocky planet orbiting around
Kepler-10, a near-solar twin some 158 light-years away in the
constellation of Draco. Kepler-10b and its star are twenty times
closer than Mercury is to our sun, and astronomers think they must
be gravitationally tide-locked: just as the moon keeps one face
toward earth, one of Kepler-10b’s sides always faces its star. The
distance between the two bodies is close enough for stellar radiation
to melt rocks at the surface of Kepler-10b, however, tidal heating may
be able to melt the entire core and mantle of the planet as well.
Image: XXXXXXXXXXXXXXXXXXX
6