First look
The idea, in plain words
The stars look as if they never change. Most of them hardly do. But some grow brighter and fainter, and a few do it so plainly that you can follow it with nothing but your eyes. Astronomers call them variable stars.
Some of them really are changing. A star of this kind swells and shrinks, over and over, like something breathing. As it does, it grows brighter and fainter. Delta Cephei, which you can see without a telescope, takes 5.366 days over each breath. At its brightest it gives about twice the light it does at its faintest.
The most startling is a red giant called Mira. At its brightest it is easy to see. Then it fades until it cannot be seen at all without a telescope, and about 332 days after it last peaked it is back. David Fabricius was the first to notice it, in August 1596. The name Mira means “the wonderful”.
Other stars only seem to change. Algol looks like one star, but it is two, going round each other. Every 2 days and 21 hours the fainter one passes in front of the brighter one and blocks most of its light. For a few hours Algol drops to about a third of its usual brightness. Then it recovers.
Now and then a star does something nobody expected. Late in 2019 Betelgeuse, the orange star at Orion’s shoulder, began to fade. By February 2020 it was down to about a third of its normal brightness, and anyone who knew Orion could see that something was wrong. By April it was back. The star had thrown out a bubble of gas, which cooled into a cloud of dust and hid part of it.
These stars are useful as well as strange. The breathing kind keep such good time that they can be used to measure the distance to other galaxies. As for the Sun, we are lucky. Its light changes by only about one part in a thousand.
Go deeper
That was the idea. The same subject is written again below for readers who want more, each on a page of its own.
Words used here
- Variable star
- A star whose brightness changes, either because it swells and shrinks or because something passes in front of it.
- Cepheid
- A supergiant star that pulses on a steady beat of days or weeks. The longer the beat, the more luminous the star, which makes Cepheids markers of distance.
- Binary star
- Two stars held together by gravity, each going round the other. Three or more together make a multiple star.
- Red giant
- A star near the end of its life that has swollen to many times its old size and cooled to a red glow.
- Apparent magnitude
- How bright a star or planet looks from the Earth, on a scale where smaller numbers mean brighter.
- Luminosity
- The total power a star gives out, in every direction and at every wavelength.
- Standard candle
- Something whose true brightness is known, so that its distance can be worked out from how faint it looks.
Where this comes from
- ESA/Hubble, Hubble image of variable star RS Puppis
- SEDS, Mira (Omicron Ceti)
- Society for Popular Astronomy, Guide to Algol (Beta Persei)
- ESO, Telescope sees surface of dim Betelgeuse
- ESO, Mystery of Betelgeuse’s dip in brightness solved
The words are written for this site. The pictures are drawn by the page from the figures in the lesson, and each one says underneath what it is based on.