Echo of the Universe
Nobel
Prizes in Astrophysics & Cosmology - Part 7
(A Twelve Part Series)
John Mather & George Smoot
Cosmology
is a science which has only a few observable facts to work with. The discovery
of the cosmic microwave background radiation added one — the present radiation
temperature of the universe. This, however, was a significant increase in our
knowledge since it requires a cosmology with a source for the radiation at an
early epoch and is a new probe of that epoch.
- Robert W Wilson
Temperature map of the CMB measured
by the Planck
spacecraft
The Nobel Prize is
equated with the pinnacle of human achievement in both popular perception and
professional esteem. Since it was first awarded in 1901, the annual
Nobel Prize for Physics has gone to major contributions in Astrophysics and Cosmology
related fields only on eleven occasions. The first six awards (1967, 1974,
1978, 1983, 1993, 2002) were the subjects of earlier articles (see here 1,2,3,4,5,6).
The next was in 2006, shared by John C Mather and George F Smoot for their momentous
discoveries related to the Cosmic Microwave Background (CMB) Radiation, the afterglow of the Universe.
What is
CMB
The Cosmic Microwave
Background is a faint, nearly uniform glow of microwave
radiation that fills the entire universe. It’s the thermal
remnant of the hot, dense state of the early universe about 380,000
years after the Big Bang, when electrons and protons combined to form neutral
atoms (a moment called recombination). At that time, light could
travel freely for the first time — and that light has redshifted over billions
of years into microwaves that we detect today.
Discovery
- In 1964, Arno Penzias and
Robert Wilson accidentally detected a persistent microwave signal
with a radio antenna at Bell Labs (see article on their Nobel Prize winning
discovery here).
- They couldn’t explain the noise; it
was isotropic (same in all directions) and corresponded to a
temperature of about 3 K.
- Simultaneously, theoretical work
by Robert Dicke, Jim Peebles, and others predicted such a
background as a relic of the Big Bang.
- Penzias and Wilson’s observation
provided strong evidence for the Big Bang theory and earned them
the Nobel Prize in Physics (1978).
Follow-up Work
Over decades, more precise
measurements beginning with COBE (Cosmic Background Explorer) have mapped the
CMB in great detail:
COBE (1989–1993)
COBE is
the ‘Cosmic Background Explorer’ satellite, a NASA probe launched in 1989 to
study the properties and distribution of the CMB. It
- Detected the blackbody
spectrum of the CMB with high precision, and
- Found tiny temperature fluctuations
(anisotropies).
Graph of CMB spectrum around its peak in the microwave frequency range, a near perfect fit
Work of John Mather and
George Smoot
They were awarded the 2006 Nobel
Prize in Physics “for their discovery of the blackbody form and
anisotropy of the cosmic microwave background radiation.” Their work
was based on results from NASA’s COBE (Cosmic Background Explorer)
probe, launched in 1989.
Scientific Background
The Cosmic Microwave
Background (CMB) is relic radiation from the epoch of recombination
(~380,000 years after the Big Bang) when photons decoupled from matter.
Theoretical prediction
(1940s–1960s):
- Universe should contain residual
radiation.
- Spectrum should be thermal (‘Planckian’).
- Tiny fluctuations (~10⁻⁵ level) should
exist as seeds of structure formation.
Before COBE:
- CMB was detected in 1964.
- Temperature was measured to be ~2.7 K.
- But precision was insufficient to:
- Confirm exact blackbody shape.
- Detect primordial anisotropies.
COBE changed all that.
Blackbody Spectrum with FIRAS, the Far Infrared Absolute Spectrophotometer
An artist’s view of FIRAS
Scientific Question: Is the CMB exactly a blackbody spectrum?
A blackbody spectrum
follows Planck’s law:
Any deviation from this would
indicate:
- Energy injection after recombination
- Exotic early-universe physics
FIRAS compared:
- Radiation from the sky, and
- Radiation from a precisely controlled
onboard blackbody calibrator
It measured the frequency
range: 1–95 cm⁻¹ (≈30–3000 GHz)
Result:
- Temperature: T=2.725±0.002 K
- Spectrum matches Planck curve to better
than 1 part in 10⁵
This is the most
perfect blackbody spectrum ever measured in nature.
Cosmological
Significance
This ruled out many
alternative cosmological models (e.g., steady-state variants).
It confirmed that the early universe was in thermal equilibrium.
The energy density of CMB:
ργ=aT4
where a is
the radiation constant.
The FIRAS study provided direct
evidence of hot Big Bang.
Detection
of Anisotropies through DMR (Differential Microwave
Radiometers)
Gorge Smoot led this
experiment.
Scientific Question
Are there primordial
fluctuations in the CMB?
Theoretical prediction: ΔT∼10−5 and density fluctuations
of the same order.
These tiny fluctuations
would later grow via gravitational instability into galaxies and clusters.
Observational Results
(1992)
COBE detected ΔT≈30μK
After subtracting dipole
anisotropy due to Earth’s motion ~3.3 mK and foreground emission, they did
indeed reveal the primordial anisotropies just as expected.
John C Mather (1946 - ) – A
Biographical Sketch
John Cromwell Mather was
born on 7 August 1946, in Roanoke, Virginia, USA. Raised in a family that
valued education and intellectual curiosity, Mather developed an early
fascination with science. He earned his B S in physics from Swarthmore College
(1968) and went on to complete his Ph D in physics at the University of
California, Berkeley (1974).
His doctoral work focused on
precision measurements in experimental cosmology—skills that would later prove
decisive in one of the most important discoveries in modern astrophysics.
Mather’s name is permanently
linked with the study of the cosmic microwave background (CMB) — the
faint afterglow of the Big Bang.
In the 1970s and 1980s, he
became the Project Scientist for NASA’s COBE (Cosmic Background
Explorer) mission. Launched in 1989, COBE carried three key instruments:
- FIRAS (Far Infrared Absolute Spectrophotometer) –
led by Mather
- DMR (Differential Microwave
Radiometers) – associated with George Smoot
- DIRBE (Diffuse Infrared Background
Experiment)
Mather’s instrument, FIRAS,
made an extraordinarily precise measurement of the CMB spectrum and showed that
it is an almost perfect blackbody radiation curve at a temperature of
about 2.725 K.
This result was monumental
because:
- It confirmed a central prediction of the
Big Bang theory.
- It ruled out alternative steady-state
cosmological models.
- It established that the early universe
had once been in a hot, dense, thermal equilibrium state.
For this achievement, Mather
shared the 2006 Nobel Prize in Physics with George F Smoot.
The Nobel citation specifically
recognized the discovery of the blackbody form and anisotropy of the cosmic
microwave background radiation.
Mather’s contribution
specifically concerned the blackbody spectrum confirmation, often
described as one of the most precise measurements ever made in physics.
Leadership in Space
Astronomy
After COBE, Mather continued
to play a central role in space-based astronomy. He became Senior Project
Scientist for NASA’s flagship infrared observatory, later to become the James
Webb Space Telescope (JWST). Mather was one of the earliest scientific
advocates for this and helped guide the mission for decades, through technical
and political challenges. The telescope’s extraordinary success stands as testimony
to his enduring legacy.
Mather is known for:
- Exceptional experimental precision
- Strong collaborative leadership
- Long-term commitment to major scientific
missions
- Ability to bridge theoretical cosmology
and instrumentation
His work transformed
cosmology from a speculative discipline into a precision science.
Honors and
Recognition
Beyond the Nobel Prize,
Mather has received:
- The NASA Distinguished Service Medal
- The Shaw Prize in Astronomy
- Membership in the U.S. National Academy
of Sciences
He remains a leading voice
in cosmology and space science.
Legacy
Mather’s confirmation of the
CMB’s perfect blackbody spectrum is often compared to a “Rosetta Stone” for
cosmology. It provided the thermodynamic fingerprint of the Big Bang and
cemented modern cosmology on firm experimental foundations.
George F Smoot (1945 – 2025)
– A Biographical Sketch
Early Life and
Education
George Fitzgerald Smoot III
was born on 20 February 1945, in Yukon, Florida, USA. He studied mathematics
and physics at the Massachusetts Institute of Technology (MIT), earning his
undergraduate degree in 1966. He then completed his Ph D at MIT in 1970,
working on experimental particle physics.
His early research included
work on antimatter and cosmic rays, but he soon shifted toward cosmology —
particularly the experimental study of the early universe.
Pioneer of Cosmic
Structure Measurements
Smoot is best known for his
leadership in detecting tiny temperature fluctuations
(anisotropies) in the cosmic microwave background (CMB), the relic
radiation from the Big Bang.
He played a central role in
NASA’s COBE (Cosmic Background Explorer) satellite mission, launched
in 1989. Smoot led the team responsible for the DMR (Differential Microwave
Radiometers) instrument
While John Mather’s FIRAS
instrument confirmed the CMB’s perfect blackbody spectrum, Smoot’s DMR
instrument made a complementary and equally historic discovery. In 1992, his
team announced the first detection of minute temperature variations in
the CMB — differences of only about one part in 100,000.
These anisotropies were
crucial because:
- They represented the “seeds” of galaxies
and large-scale structure.
- They provided direct evidence that small
density fluctuations existed in the early universe.
- They strongly supported inflationary
cosmology models.
The discovery was famously
described as: “Looking at the face of God.”
Nobel Prize
For these discoveries, Smoot
shared the 2006 Nobel Prize in Physics with John C Mather.
The Nobel citation
recognized:
- The discovery of the blackbody form
(Mather)
- The discovery of anisotropy in the
cosmic microwave background radiation (Smoot)
Together, these findings
transformed cosmology into a precision, data-driven science.
Later Career and
Contributions
After COBE, Smoot continued
his research at the University of California, Berkeley, contributing to
subsequent cosmology missions and large-scale structure studies. He was
involved in:
- Balloon-borne and satellite experiments
refining CMB measurements
- Cosmological data interpretation from
missions like WMAP and Planck
- Theoretical and observational work
related to cosmic inflation
He also became known for
public engagement in science and international collaborations, including
academic positions in Europe and Asia.
Scientific Impact
Smoot’s measurement of CMB
anisotropies:
- Confirmed predictions that tiny
primordial fluctuations would grow under gravity into galaxies and
clusters.
- Provided empirical support for
inflationary cosmology.
- Laid groundwork for later high-precision
missions such as WMAP and Planck.
Today, the CMB anisotropy
map is considered one of the most important images in modern science.
Personality and
Public Role
Smoot is known for:
- Strong experimental leadership
- Ambitious, large-scale scientific
projects
- Effective communication of cosmology to
the public
He has written popular
science books explaining the origin and evolution of the universe, helping
bring cosmology to a wider audience.
Legacy
If Mather gave cosmology its
thermal proof of the Big Bang, Smoot revealed its structure — the tiny ripples
that grew into galaxies, stars, and eventually observers like us.
Epilogue: Follow-up work on
CMB
WMAP (2001–2010)
WMAP is
the ‘Wilkinson Microwave Anisotropy Probe’, a NASA mission that
- Produced detailed, full-sky maps of CMB
temperature variations.
- Allowed precise determination of
cosmological parameters (age of universe, composition, geometry).
WMAP Spacecraft
Planck (2009–2013)
Planck was
a European Space Agency (ESA) space observatory that
- Provided the most detailed CMB survey to
date.
- Measured the temperature and polarization
anisotropies with unprecedented precision.
These anisotropies are the
seeds of large-scale structure — the galaxies and clusters we see today.
Planck Spacecraft
Current Status
The CMB is now one of the
most well-measured observables in cosmology.
It shows that the universe is:
- ~13.8 billion years old
- Flat (in overall geometry)
- Composed of ~5% ordinary matter, ~27%
dark matter, ~68% dark energy
Current work focuses on:
- CMB polarization,
especially B-modes, which could reveal primordial gravitational waves
from inflation.
- Ground-based telescopes (e.g., the
South Pole Telescope, Simons Observatory) and future missions aiming for
even finer measurements.
Why it Matters
The CMB is a snapshot of the early universe — a cornerstone of modern cosmology that underpins our understanding of the origin, composition, and evolution of the cosmos.