There are galaxies that orbit our galaxy that are believed to be filled with a lot of dark matter. Segue 1 is one of about two dozen dwarf galaxies around ours that have light outputs equal to only a few hundred times that of our sun. There are probably untold numbers of other such galaxies around the more visible galaxies. This is a possible explanation for the discrepancy in the predicted mass of the universe and the observed mass. Some theories postulate that 90% of the mass of the universe is composed of this unobservable "dark matter". The existence of these dim dwarf galaxies help explain the discrepancy.
dimmest stars in aquarius
Deneb is the dimmest star in Cygnus.
Gliese 229 is the dimmest star in the constellation Lepus
No, an EO galaxy is not a type of elliptical galaxy. They are a lenticular galaxy.
No, a tadpole galaxy is not a type of peculiar galaxy. It is a barred spiral galaxy.
Yes, a double galaxy is a type of peculiar galaxy.
Yes, a chain galaxy is a type of peculiar galaxy.
Yes. A ring galaxy is a type of peculiar galaxy.
The dimmest star is Orion is HD 37605 with an apparentmagnitude of 8.69
No, a V-Shaped galaxy is not a type of peculiar galaxy.
Yes, a spiderweb galaxy is a type of peculiar galaxy.
The dimmest star in the Phoenix constellation is HD 201626, which has an apparent magnitude of 5.59. It is a yellow-white F-type star located around 235 light-years away from Earth.