It had an apparent magnitude of 13.5 from its center.

It also has an apparent magnitude of 5.66 and is about 3,600 light years away.

Being so far from the Sun, it only has an apparent magnitude of 23.

Recently the star has had an apparent magnitude range of about 6.9 to 8.

The star, as seen from Earth, has an apparent magnitude of 13.8.

It comes to opposition in late May at an apparent magnitude of 20.4.

Its apparent magnitude is 4.98, and approximately 839 light years away from Earth.

The system varies in apparent magnitude from 9.6 to 14.

The star system has a combined apparent magnitude of 2.9.

Because of its low apparent magnitude, Kepler-40 cannot be seen with the naked eye.

On average, the asteroid has an apparent magnitude of 9.4.

It has a visual apparent magnitude range of 5.6 to 10.

The apparent magnitude of the Sun from the spacecraft is 16.3.

It is approximately 27.4 million light years from Earth and has an apparent magnitude of 11.82.

It has an apparent magnitude of 10.01 and can be seen with small telescopes.

It was discovered on January 17, 1929, at an apparent magnitude of 11.

It has an apparent magnitude that varies from about 5 to 7.4.

During the 1914 close approach the asteroid reached about apparent magnitude 7.7.

It has apparent magnitude 6.47 and is about 200 light-years away.

In its quiet phase it has an apparent magnitude of about 12.5.

This star has an apparent magnitude of 8.05 when viewed from earth.

About 7.8 light years from the Earth, it has an apparent magnitude of 13.5 and can only be seen with a large telescope.

This variable star changes in apparent magnitude from 4.3 to 5.1 with a period of 7.59 days.

It varies in apparent magnitude from 6.27 to 6.83 over a period of 15.6 hours.

It varies by about 0.2 in apparent magnitude from 0.75 to 0.95.