22 (1) Flashcards
The left-hand edge of the main-sequence band in the H–R diagram is called the ……….. ………… ………….
We use the term …………… to mark the time when a star stops contracting, settles onto the main sequence, and begins to fuse hydrogen in its core.
zero-age main sequence
zero-age
R 2
The lifetime of a star in a particular stage of evolution depends on how much ……….. ………. it has and on how quickly it uses up that …………
nuclear fuel / fuel
In the case of stars, more massive ones use up their fuel much more quickly than stars of low mass.
what determines how hot a star’s central regions get?
It is the mass of the star—the weight of the overlying layers determines how high the pressure in the core must be:
higher mass requires higher pressure to balance it.
Higher pressure, in turn, is produced by higher temperature.
Stars devote an average of ……… of their lives to peacefully fusing hydrogen into helium.)
90%
(Note that red giant stars do not actually look deep red; their colors are more like …………. or …………)
orange / orange-red
The three basic types of clusters astronomers have discovered are ………………..
- globular clusters,
- open clusters, and
- stellar associations.
globular clusters contain only ………………. stars, whereas open clusters and associations contain …………. stars.
very old / young
The most massive globular cluster in our own Galaxy is ………. …………, which is about 16,000 light-years away and contains several million stars
Omega Centauri
Several open clusters are visible to the unaided eye. Most famous among them is the ………….. which appears as a tiny group of …….. stars (some people can see even more than ……….., and the Pleiades is sometimes called the ……….. Sisters).
Pleiades
six / six / Seven
The ……… is another famous open cluster in the constellation of Taurus the bull. To the naked eye, it appears as a V-shaped group of faint stars marking the face of the bull. Telescopes show that …………. actually contains more than 200 stars.
Hyades
An ………… is a group of extremely young stars, typically containing 5 to 50 hot, bright O and B stars scattered over a region of space some 100–500 light-years in diameter.
association
As an example, most of the stars in the constellation Orion form one of the nearest stellar associations.
we indicated that open clusters are younger than globular clusters, and associations are typically even younger.
R 2
we will show how we determine the ages of these star clusters. The key observation is that the stars in these different types of clusters are found in different places in the ………. ……., and we can use their locations in the diagram in combination with theoretical calculations to estimate how long they have lived.
H–R diagram
There are real star clusters that fit this description. The first to be studied (in about 1950) was ……………., which is still associated with the region of gas and dust from which it was born
NGC 2264