Webb telescope confirms the universe is expanding at an unexpected rate

Spiral galaxy NGC 628, located 32 million light-years away from Earth, is seen in an undated image from the James Webb Space Telescope. NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team/Handout via REUTERS/File Photo
Fresh corroboration of the perplexing observation that the
universe is expanding more rapidly than expected has scientists pondering the
cause - perhaps some unknown factor involving the mysterious cosmic
components of dark
energy and dark
matter.
Two years of data from NASA's James
Webb Space Telescope have now validated the Hubble Space Telescope's
earlier finding that the rate of the universe's expansion is faster - by about
8% - than would be expected based on what astrophysicists know of the initial
conditions in the cosmos and its evolution over
billions of years. The discrepancy is called the Hubble Tension.
The observations by Webb, the most
capable space telescope ever deployed, appear to rule out the notion
that the data from its forerunner Hubble was somehow flawed due to instrument
error.
"This is the largest sample of Webb Telescope data -
its first two years in space - and it confirms the puzzling finding from the
Hubble Space Telescope that we have been wrestling with for a decade - the
universe is now expanding faster than our best theories can explain," said
astrophysicist Adam Riess of Johns Hopkins University in Maryland, lead author
of the study published on Monday in the Astrophysical Journal.
"Yes, it appears there is something missing in our
understanding of the universe," added Riess, a 2011 Nobel laureate in
physics for the co-discovery of the universe's accelerating expansion.
"Our understanding of the universe contains a lot of ignorance about two
elements - dark matter and dark energy - and these make up 96% of the universe,
so this is no small matter."
"The Webb results can be interpreted to suggest there
may be a need to revise our model of the universe, although it is very
difficult to pinpoint what this is at the moment," said Siyang Li, a Johns
Hopkins doctoral student in astronomy and astrophysics and a study co-author.
Dark matter, thought to comprise about 27% of the universe,
is a hypothesized form of matter that is invisible but is inferred to exist
based on its gravitational effects on ordinary matter - stars, planets, moons,
all the stuff on Earth - which accounts for roughly 5% of the universe.
Dark energy, believed to comprise approximately 69% of the
universe, is a hypothesized form of energy permeating vast swathes of space
that counteracts gravity and drives the universe's accelerating expansion.
"There are many hypotheses that involve dark matter,
dark energy, dark radiation - for example, neutrinos (a
type of ghostly subatomic particle) - or gravity itself having some exotic
properties as possible explanations," Riess said.
The researchers employed three different methods to measure
a specific telltale metric - distances from Earth to galaxies where a type of
pulsating star called Cepheids has been documented. The Webb and Hubble
measurements were in harmony.
The universe's expansion rate, a figure called the Hubble
constant, is measured in kilometres per second per megaparsec, a distance equal
to 3.26 million light-years. A light-year is the distance light travels in a
year, 5.9 trillion miles (9.5 trillion km).
Under the standard model of cosmology - basically, the
conventional wisdom concerning the universe - the value of the Hubble constant
should be about 67-68. The Hubble and Webb data give a value averaging about
73, with a range of about 70-76.
The Big Bang event 13-14 billion years ago initiated the
universe, and it has been expanding ever since. Scientists in 1998 disclosed
that this expansion was actually accelerating, with dark energy as the
hypothesized reason.
The new study looked at Webb's data covering about a third of
Hubble's full slate of relevant galaxies. The researchers in 2023 announced
that earlier interim Webb data validated the Hubble findings.
"We need more data to better characterize this clue.
Exactly what size is it (the discrepancy)? Is the mismatch at the lower end -
4-5% - or the higher end - 10-12% - of what the current data allows? Over what
range of cosmic time is it present? These will further inform ideas,"
Riess said.
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