137
was also employed by Hubble in
his discovery of the relationship
between the distance and
recessional velocity of galaxies,
leading to confirmation that the
universe is expanding.
Revising the scale
In the 1940s, the German
astronomer Walter Baade was
working at the Mount Wilson
Observatory in California. Baade
made observations of the stars
at the center of the Andromeda
galaxy during the enhanced
viewing conditions afforded
by the wartime blackout. He
distinguished two separate
populations, or groups, of Cepheid
variables that have different
period–luminosity relationships.
This led to a dramatic revision in
the extragalactic distance scale—
for example, the Andromeda
galaxy was found to be double
the distance from the Milky
Way that Hubble had calculated.
Baade announced his findings
at the International Astronomical
Union in 1952. The two groups
of Cepheids became known as
classical and Type II Cepheids,
and started to be used for different
purposes in distance measuring.
Today, classical Cepheids are
used to measure the distance of
galaxies out to about 100 million
light-years—well beyond the
local group of galaxies. Classical
Cepheids have also been used to
clarify many characteristics of
the Milky Way galaxy, such as its
local spiral structure and the sun’s
distance from the plane of the
galaxy. Type II Cepheids have been
used to measure distances to the
galactic center and globular clusters.
THE RISE OF ASTROPHYSICS
The measurement of distances
to Cepheid variables for more
accurate calibration of period–
luminosity relationships is still
considered extremely important,
and it was one of the primary
missions of the Hubble Space
Telescope project when it was
launched in 1990. A better
calibration is crucial, among
other things, to calculate the age
of the universe. Leavitt’s findings
from over a century ago are still
having significant repercussions
in terms of truly understanding
the scale of the cosmos. ■
A simplified version
of the mechanisms that
cause Cepheid variables
to fluctuate in size is
shown here. The pressure
forces inside a star include
gas pressure, maintained
by heat output from the
star’s core, and radiation
pressure. Another
mechanism that may
be involved is a cyclical
change in the opacity
(resistance to the
transmission of radiation)
in gas within the star’s
outer layers.
Pressure forces exceed
gravity. The star begins
to expand.
Pressure and gravity are now
in balance but inertia causes
the star to expand further.
A B
C
With continued expansion,
the pressure forces decrease,
as does the gravity, though
to a lesser extent. Eventually,
gravity exceeds the pressure
from the pressure forces, and
the star stops expanding
and begins to shrink.
As the star contracts, the
pressure forces increase until
they exceed the inward-
pulling gravity. The star
stops shrinking and begins
to expand again, starting
a new pulsation cycle.
Pressure and gravity
are in balance again
but inertia causes the
star to shrink further.
D E
Hubble’s underwhelming
acknowledgment of Leavitt
is an example of the ongoing
denial and lack of professional
and public recognition that
she suffers from, despite her
landmark discovery.
Pangratios Papacosta
Science historian
Gravity Pressure
forces