Want to catch the moon sliding past the planets, Mars, Jupiter and Venus this week? Click here for a chart.
Tonight … come to know Delta Cephei, a famous variable star in the constellation Cepheus. With clock-like precision, this star doubles in brightness, fades to a minimum and then doubles in brightness again every 5.36 days. You can notice this brightness change with the eye alone, and can see it best by contrasting this star with two nearby stars.
The constellation Cepheus requires a dark sky to be seen. But if you can spot this constellation, you might be able to find Delta Cephei, the famous variable star. You’ll find it high in your northern sky on November and December evenings. The pattern of stars in Cepheus resembles a stick house, the kind we all drew as children. The variable star – Delta Cephei – is located near the bottom corner of the house pattern.
Cepheid variable stars are a class of stars named in honor of Delta Cephei. They are known as pulsating variables. The image up above is what astronomers call a “light curve” of a variable star. Each point represents the brightness of the star at a particular time. You can see that the star’s brightness changes in a regular way over a period of days.
The brightness of a Cepheid variable star changes because the star is actually expanding and contracting in size. The radius of a Cepheid variable star changes by several million kilometers (30%) as the star expands and shrinks. There is a very precise relationship between a Cepheid variable’s luminosity, or true brightness, and pulsation period. The greater the intrinsic brightness of the star, the longer the period. For that reason, these variable stars serve as standard candles – in other words, their true brightness is known, so astronomers can see how bright they look to measure the distances to the stars – and hence to faraway galaxies.
Now look again at the chart showing the constellations Cepheus the King and Cassiopeia the Queen at the top of this page. In the actual sky, the two stars near Delta Cephei – Epsilon Cephei and Zeta Cephei – mark the low and high ends of Delta Cephei’s brightness scale. At its faintest, the variable star Delta Cephei is as dim as the fainter star, Epsilon Cephei. At its brightest, Delta Cephei matches the brightness of Zeta Cephei.
Cepheid variable stars enabled the astronomer Edwin Hubble to figure out that the Andromeda galaxy lies outside the bounds of our local galaxy, the Milky Way.
Bottom line: Delta Cephei is a famous variable star in the constellation Cepheus. With clock-like precision, this rather faint star doubles in brightness, dims and then doubles in brightness every 5.36 days.