This image – the first released from NASA’s James Webb Space Telescope – shows the galaxy cluster SMACS 0723. Some of the galaxies appear smeared or stretched due to a phenomenon called gravitational lensing. This effect can help scientists map the presence of dark matter in the universe. Credits: NASA, ESA, CSA, and STScI https://www.nasa.gov/webbfirstimages
Could one of the biggest puzzles in astrophysics be solved by reworking
Albert Einstein’s theory of gravity? A new study co-authored by NASA scientists
says not yet.
The universe is expanding at an accelerating rate, and scientists don’t
know why. This phenomenon seems to contradict everything researchers understand
about gravity’s effect on the cosmos: It’s as if you threw an apple in the air
and it continued upward, faster and faster. The cause of the acceleration,
dubbed dark energy, remains a mystery.
A new study from the international Dark Energy Survey, using the Victor M.
Blanco 4-meter Telescope in Chile, marks the latest effort to determine whether
this is all simply a misunderstanding: that expectations for how gravity works
at the scale of the entire universe are flawed or incomplete. This potential
misunderstanding might help scientists explain dark energy. But the study – one
of the most precise tests yet of Albert Einstein’s theory of gravity at cosmic
scales – finds that the current understanding still appears to be correct.
The results, authored by a group of scientists that includes some from
NASA’s Jet Propulsion Laboratory, were presented Wednesday, Aug. 23, at the
International Conference on Particle Physics and Cosmology (COSMO'22) in Rio de
Janeiro. The work helps set the stage for two upcoming space telescopes that
will probe our understanding of gravity with even higher precision than the new
study and perhaps finally solve the mystery.
More than a century ago, Albert Einstein developed his Theory of General
Relativity to describe gravity, and so far it
has accurately predicted everything from the orbit of Mercury to the existence
of black holes. But if this theory can’t explain dark energy, some scientists
have argued, then maybe they need to modify some of its equations or add new
components.
To find out if that’s the case, members of the Dark Energy Survey looked
for evidence that gravity’s strength has varied throughout the universe’s
history or over cosmic distances. A positive finding would indicate that
Einstein’s theory is incomplete, which might help explain the universe’s
accelerating expansion. They also examined data from other telescopes in
addition to Blanco, including the ESA (European Space Agency) Planck satellite, and reached the same conclusion.
The study finds Einstein’s theory still works. So no explanation for dark
energy yet. But this research will feed into two upcoming missions: ESA’s Euclid mission, slated for launch no
earlier than 2023, which has contributions from NASA; and NASA’s Nancy Grace Roman Space Telescope, targeted for launch no later than May 2027. Both telescopes will search
for changes in the strength of gravity over time or distance.
Blurred Vision
How do scientists know what happened in the universe’s past? By looking at
distant objects. A light-year is a measure of the distance light can travel in
a year (about 6 trillion miles, or about 9.5 trillion kilometers). That means
an object one light-year away appears to us as it was one year ago, when the
light first left the object. And galaxies billions of light-years away appear
to us as they did billions of years ago. The new study looked at galaxies stretching
back about 5 billion years in the past. Euclid will peer 8 billion years into
the past, and Roman will look back 11 billion years.
The galaxies themselves don’t reveal the strength of gravity, but how they look when viewed from Earth does. Most matter in our universe is dark matter, which does not emit, reflect, or otherwise interact with light. While scientists don’t know what it’s made of, they know it’s there, because its gravity gives it away: Large reservoirs of dark matter in our universe warp space itself. As light travels through space, it encounters these portions of warped space, causing images of distant galaxies to appear curved or smeared. This was on display in one of first images released from NASA’s James Webb Space Telescope.
This video explains the phenomenon called gravitational lensing, which can
cause images of galaxies to appear warped or smeared. This distortion is caused
by gravity, and scientists can use the effect to detect dark matter, which does
not emit or reflect light. Credits: NASA’s Goddard Space Flight Center
Dark Energy Survey scientists search galaxy images for more subtle
distortions due to dark matter bending space, an effect called weak
gravitational lensing. The strength of gravity determines the size and
distribution of dark matter structures, and the size and distribution in turn
determine how warped those galaxies appear to us. That’s how images can reveal
the strength of gravity at different distances from Earth and distant times
throughout the universe’s history. The group has now measured the shapes of
over 100 million galaxies, and so far, the observations match what’s predicted
by Einstein’s theory.
“There is still room to challenge Einstein’s theory of gravity, as measurements gets more and more precise,” said study co-author Agnès Ferté, who conducted the research as a postdoctoral researcher at JPL. “But we still have so much to do before we’re ready for Euclid and Roman. So it’s essential we continue to collaborate with scientists around the world on this problem as we’ve done with the Dark Energy Survey.”
Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
Source: NASA
Scientists Help Probe Dark Energy by Testing Gravity | NASA
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