Among
all the forces of Nature, the gravitational force is the one that has been known
to man for the longest time. One of its fundamental properties -that all bodies
fall with the same acceleration- was recognized by Galileo at the beginning
of the seventeenth century. Towards the end of the same century, Newton established
the universal gravitation law connecting the force responsible of the fall of
bodies to the gravitational force between planets. Finally, Einstein, with the
theory of general relativity, connected the gravitational field with the structure
of space-time. Nevertheless, we dispose of very few elements on properties of
gravitational force in particular in extreme conditions such as during the primordial
explosion or the collision of black holes. Contrarily to what one could believe
the gravitational force is, among the fundamental forces, the less known.
Einsteins theory predicts the existence of gravitational waves which are
perturbations of the gravitational field spreading out in space at the speed
of light, like ripples on the surface of a pond. However, while electromagnetic
radiations (for example visible light) can be absorbed completely by matter,
gravitational waves can travel through space without being absorbed neither
by stars, nor by interstellar matter.
This very low interaction, together with the weakness of the gravitational force
makes the detection of gravitational waves extraordinarly difficult. Actually,
after 30 years of active research, we only have an indirect proof of their existence.
It has not yet been possible to detect gravitational waves directly, this remains
one of the major challenges of experimental physics.

The
gravitational force
Photo
1
Because the
gravitational pull of matter bends the path of light rays, massive astronomical
objects like stars, galaxies and galaxy clusters, may act like lenses, which
can magnify and severely distort the images of objects located behind them,
producing weird pictures as in a hall of mirrors.
In the most extreme case, where the foreground lensing galaxy and the background
object are perfectly lined up, the image of the background galaxy is stretched
into a ring known as Einstein ring.
(ESO-VLT picture of galaxy cluster CL2244-02)
Photo
2
This
quadruple quasar is in fact a gravitational mirage. It shows
4 ghost images of one single object located far beyond the imaging
red galaxy the mass of which is responsible for the four (of which two are
not completely resolved) gravitationally lensed images of the background
quasar.
(ESO-VLT picture of MG0414+0534)
Photo
3
This butterfly-shaped galaxy
is the product of the collision of two smaller galaxies. The central region
of the galaxy contains two active giant black holes put into evidence through
the x-ray emission from the gas swirling around them. The black holes orbit
each other for hundreds of millions of years before they merge to form a single
super-massive black hole sending out during this process intense gravitational
waves. Such mergings of supermassive black holes are clear targets for gravitational
waves detectors.
(Combined Chandra-HST picture of NGC 6240. Credit: X-ray:
NASA/CXC/MPE/S.Komossa et al.; Optical: NASA/STScI/R.P.van der Marel &
J.Gerssen)
©Lionel Bret / LookatSciences