213
See also: The properties of sunspots 129 ■ The Homestake experiment 252–53 ■
Exoplanets 288–95
I
n 1960, American physicist
Robert Leighton made
observations with a camera
that he had devised, which led to
the discovery that the sun is “ringing
like a bell,” as he put it. Working
with Robert Noyes and George
Simons, Leighton picked up
perturbations of the sun’s surface
using Doppler shift solar cameras.
These cameras detected tiny
shifts in the frequency of the sun’s
absorption spectra as its outer layer
moved toward or away from Earth.
Five-minute oscillations
The complex patterns of vibrations,
with an average period of five
minutes (known as “5-minute
oscillations”), were at first thought
to be a surface phenomenon. Then
in 1970, Roger Ulrich explained
them as trapped acoustic waves
bouncing within the sun from one
side to the other, causing the star’s
surface to wobble as it resonated.
Today, these waves allow
scientists to investigate the interior
of the sun, in much the same way
that acoustic earthquake waves
reveal the inner composition
and structure of Earth. Known as
helioseismology, this process is often
compared to trying to build a piano
by studying the sounds it makes
when it falls down a flight of stairs,
but it has produced a model of the
sun’s interior processes. The model
places tight constraints on the
amount of helium in the star’s core,
which has important consequences
for models of the early universe. ■
NEW WINDOWS ON THE UNIVERSE
THE SUN RINGS
LIKE A BELL
THE SUN’S VIBRATIONS
IN CONTEXT
KEY ASTRONOMER
Robert Leighton (1919 –1997)
BEFORE
1954 Canadian astronomer
Harry Hemley Plaskett observes
the sun’s oscillation effect.
AFTER
1970 American physicist
Roger Ulrich proposes that the
oscillations are from acoustic
waves in the solar interior.
1970s Helioseismology opens
up a new way of investigating
the interior of the sun.
1995 The solar observatory
satellite SOHO is launched.
1997 The SOHO team discover
“jet streams” of plasma in the
convective zone.
1990–2000s Hundreds of
thousands of the sun’s
vibrational modes are identified.
2009 The Kepler satellite
measures oscillations in
sunlike stars to describe
conditions on exoplanets.
With his very inquisitive
mind, every funny effect
that you’d see in nature
he’d try to explain.
Gerry Neugebauer
Physicist and colleague
of Robert Leighton