HDF Index
Summary Of Key Findings From The Hubble Deep Field
Press Release downloaded from
STScI HDF Key Findings
Overview
The Hubble Space Telescope spent 10 days in December 1995
observing a single tiny patch of sky near the Big Dipper. These
observations resulted in the deepest image of the sky, called the
Hubble Deep Field (HDF), revealing galaxies fainter than had ever
been seen before. The striking full-color image of the distant
universe was unveiled at the American Astronomical Society
Meeting in January 1996, and for the last year has been the
subject of intense study worldwide. Here is an overview of the
current findings.
Small Galaxies in the Early Universe
The HDF is apparently dominated by galaxies smaller than the
typical giant galaxies in the present universe (this was also
inferred from the earlier Hubble Medium-Deep Survey). The HDF
shows that galaxies stay small even at faint magnitudes. In
theory the angular diameters of galaxies should stop decreasing
significantly beyond 8 billion light years (redshift of 1). For a
closed universe, galaxies even get bigger at high redshifts.
Open Versus Closed Universe
Open universe models work best for matching both the number of
galaxies and their colors (used to asses stellar populations) in
the HDF. Alternatively, closed universe models with an enhanced
population of dwarf galaxies at redshifts between 0.5 and 2 might
work as well. These dwarfs at moderate redshifts would either
have to merge to become part of bright galaxies seen today or
fade away so that they are no longer visible in the local
universe. There are difficulties with both possibilities, but
neither is firmly ruled out.
Disturbed Galaxies
A surprisingly large fraction of galaxies show disturbed or
peculiar morphologies, even among the brighter galaxies in the
HDF (whose sizes and numbers are reasonably consistent with the
quiescent evolution of galaxies). Nevertheless, it is not clear how
much of this is due to real evolution and how much is due to the
fact that ultraviolet light from distant galaxies tends to
highlight the peculiarities of even normal galaxies.
Stellar Baby Boom
Star formation in galaxies peaked at between 7 and 9 billion
years ago (redshift of 1 and 2). This is based on colors and
redshift surveys which provide an estimate of the total stellar
output of galaxies at redshifts greater than 2.5 (very few
galaxies were known above redshifts of 1 prior to the HDF).
In Search of Hidden Stars
Much of the star formation in the universe may be taking place
in dusty galaxies. Calculations based only on optical
measurements may be missing much of the starbirth action. (This
claim is disputed and has yet to be published.)
Missing Mass -- Still Missing
The HDF results rule out low-mass, hydrogen-burning stars as a
major source of dark matter in the Milky Way, because there are
only a handful of red stars in the HDF field.
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