题目材料
In addition to conventional galaxies, the universe
contains very dim galaxies that until recently went
unnoticed by astronomers. Possibly as numerous
as conventional galaxies, these galaxies have the
same general shape and even the same
approximate number of stars as a common type of
conventional galaxy, the spiral, but tend to be much
larger. Because these galaxies' mass is spread out
over larger areas, they have far fewer stars per unit
volume than do conventional galaxies. Apparently
these low-surface-brightness galaxies, as they are
called, take much longer than conventional galaxies
to condense their primordial gas and convert it to
stars-that is, they evolve much more slowly.
These galaxies may constitute an answer to the
long-standing puzzle of the missing baryonic mass
in the universe. Baryons-subatomic particles that
are generally protons or neutrons-are the source .
of stellar, and therefore galactic, luminosity, and so
their numbers can be estimated based on how
luminous galaxies are. However, the amount of
helium in the universe, as measured by
spectroscopy, suggests that there are far more
baryons in the universe than estimates based on
galactic luminosity indicate. Astronomers have long
speculated that the missing baryonic mass might
eventually be discovered in intergalactic space or as
some large population of galaxies that are
difficult to detect.
The author mentions the fact that baryons are the
source of stars' luminosity primarily in order to explain
- Ahow astronomers determine that some galaxies
contain fewer stars per unit volume than do
others
- Bhow astronomers are able to calculate the total
luminosity of a galaxy
- Cwhy astronomers can use galactic luminosity to
estimate baryonic mass
- Dwhy astronomers' estimates of baryonic mass
based on galactic luminosity are more reliable
than those based on spectroscopic studies of
helium
- Ehow astronomers know bright galaxies contain
more baryons than do dim galaxies
显示答案
正确答案: C