Binary Star Systems Trivia Quiz

Answer: Two stars which orbit a common center of gravity

In a binary system, two stars orbit each other due to a common gravitational center, which is dependent on the mass on the stars.

When two stars appear close together in the sky, the situation is known as an "optical double". This means that although the stars are aligned along the same line of sight, they may be at completely different distances from us. This occurs in constellations; however, two stars in the same constellation can also be part of a binary system.

Answer: Gravitational

Photometric binaries are also called eclipsing binaries.

Answer: Telescope

Candidate visual binaries are viewed and studied with a telescope, normally over decades, and even over centuries. Using photographs, an astronomer can determine whether it is a visual binary or an optical double by studying the orbital path of the stars.

Answer: True

This is true. When it was discovered in 1844 by the German astronomer Bessel, the Sirius system was classed as an astrometric binary, because the companion star, Sirius B, was too faint to be seen.
Bessel, who was also a mathematician, determined by calculations that Sirius B existed after observing that the proper of Sirius A (the main star) followed a wavy path in the sky, rather than a uniform path.

Sirius can now be studied as a visual binary because, with improving technology and therefore improved telescopes, Sirius B was able to be seen, although not for 20 years after Bessel had correctly predicted its existence.

Answer: Doppler

The Doppler effect (also called Doppler shift) was named after the Austrian mathematician and physicist Christian Doppler, the man who discovered it. The effect is due to the frequencies of waves changing for an observer relative to the source of the waves.

You can experience it for yourself using sound waves, by listening as vehicles drive past you. The effect is especially evident if the vehicle has a siren.

Answer: True

By observing the variation in luminosity (brightness), a graph can be drawn (plotting the variation against time) which shows periodic troughs.
The deepest troughs occur when the faint companion star blocks some light of the brighter star. The shallow troughs occur when the fainter star is behind the other, and therefore indicates the luminosity of the brighter star.
Using the deep troughs, it can be worked out what fraction of the brighter star is obscured.

From this, it is possible to work out the ratio of the areas of the two stars. Since area is proportional to the square of the radius, this can be used to work out the ratio of the two radii. Using the speeds of the stars obtained from Doppler measurements, the actual radii can be worked out.

Eclipsing binaries are actually a subclass of spectroscopic binaries, although they are normally regarded as a separate category.

Answer: Mizar (Zeta Ursae Majoris)

Mizar is the second star from the end of the Big Dipper's handle, and is known as Vasistha in Indian astronomy. Mizar A was the first spectroscopic binary to be discovered, by Edward Pickering in 1889.

Answer: Mass (prop) radius, and Mass (prop) lum^4

The answer is Mass (prop) radius, and Mass (prop) luminosity^4. To better illustrate these relationships, here are two examples.

If a star was 2 times the mass of the Sun, the radius would be 2 times that of the Sun, and the luminosity would be 2^4 i.e. 16 times that of the Sun.

If another star had 0.2 times the mass of the Sun, the radius would be 0.2 times that of the Sun, and the luminosity would be 0.2^4 i.e. 0.0016 times that of the Sun.

As demonstrated by these examples, you can see that a relatively small difference in mass gives a relatively large difference in luminosity.

Answer: White dwarf

White dwarfs are composed of what is called electron-degenerate matter. This means that the matter is compressed so far that each electron shell is full starting from the inwards and coming out. The matter is supported by electron-degeneracy pressure and withstands further compression. These stars are very dense; they are approximately the size of the Earth, but have approximately the mass of the Sun.

When a star in a binary pair is a white dwarf, mass from the larger star is transferred to and accumulates on the surface. Eventually this mass heats up and explodes brightly. The mass is scattered into space. This is called a nova. Novae can reoccur.

Supernovae occur in the same way, however the difference is that when the mass on the white dwarf exceeds the mass that electron-degeneracy pressure can support (approx. 1.4 solar masses, called the Chandrasekhar limit), the carbon core of the white dwarf collapses and heats up, reaching the temperature for carbon fusion, the carbon burns explosively, and the star matter is ejected into space. This is the death of the star.

Answer: Yes

The answer is yes. The term "binary system" is not used exclusively for star systems, but also for planets, asteroids, and galaxies which rotate around a common center of gravity.

However, this is not a trick question; even in star binaries, the companion can be a black hole. An example of this is Cygnus X-1.

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