Variable Stars: What Causes Their Brightness to Vary?

In summary, large stars are called variable stars because they experience frequent outbursts. When they burst, they can create a nebula but still remain as a star. This is due to the different mechanisms that cause variability in different types of variable stars. These include Cepheids, planetary nebula, supernova, neutron stars, black holes, and T-Tauri stars. Variability is also common among stars as they leave the main sequence and enter the giant stage. The length of time for each star's variability depends on its original mass and composition.
  • #1
varsha
56
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i don't get it. really large stars are unstable and there are frequent outbursts. so they are called variable stars. but when they burst they create a nebula and remain as a star right? how is that? shouldn't they turn into a black hole or a nutron star or just a nebula?

or do they just vary in brightness?
 
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  • #2
varsha said:
i don't get it. really large stars are unstable and there are frequent outbursts. so they are called variable stars. but when they burst they create a nebula and remain as a star right? how is that? shouldn't they turn into a black hole or a nutron star or just a nebula?

or do they just vary in brightness?
The trouble with an answer is that there are very many different types of variavle stars, and each usually has a different mechanism going on which causes the variability. One type is Cepheids, which you can read about in the thread below.

Otherwise, search on:
(1) Variable Stars
(2) Planetary Nebula
(3) Supernova
- Type II
- Type I
(4) Supernova Remnant(s)
(5) Neutron Stars
(6) Black holes
(7) T-Tauri Stars
etc., etc.

There are probably others, but these subjects would find you plenty to read. Also, and probably most essential, is to Read about the Main Sequence where you'll find that almost all stars are variable at some point in their lives. Usually (huge caveat) it is when they leave the main sequence and enter the giant stage(s) and pulsate on a regular basis for many years. The time period for each star depends (mainly) on original mass and chemical composition.
 

What are variable stars?

Variable stars are stars that exhibit changes in their brightness over time. These changes can occur over periods of hours, days, or even years.

What causes the brightness of variable stars to vary?

There are several factors that can cause the brightness of variable stars to vary. These include changes in the star's internal structure, pulsations, eclipses by companion stars, and changes in the amount of material being ejected from the star.

How do scientists measure the brightness of variable stars?

Scientists use a unit called magnitude to measure the brightness of variable stars. The lower the magnitude, the brighter the star appears. However, some variable stars can have magnitudes that change by several orders of magnitude, making them incredibly difficult to measure accurately.

What types of variable stars are there?

There are several types of variable stars, including Cepheid variables, RR Lyrae variables, and eclipsing binaries. Each type has its own unique characteristics and can be used for different purposes in astronomical research.

Why do scientists study variable stars?

Studying variable stars can provide valuable information about stellar evolution, the structure and composition of stars, and the properties of the universe. They can also serve as important tools for measuring distances in space and detecting exoplanets.

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