UCSB Science Line
Sponge Spicules Nerve Cells Galaxy Abalone Shell Nickel Succinate X-ray Lens Lupine
UCSB Science Line
Home
How it Works
Ask a Question
Search Topics
Webcasts
Our Scientists
Science Links
Contact Information
How do we know the distance that a star is from earth? How is it calculated? Also how do we know how hot stars are? And how do we know that there is plasma on them?
Question Date: 2013-08-20
Answer 1:

Great questions! We can find the distance of stars by using simple trigonometry! Astronomers observe distant stars at one point in the year, and again six months later when the earth is halfway around the Sun. By that time, the star of interest will have appeared to shift slightly when compared to even more distant stars. From this perspective, scientists can determine the (very small) angle between the Earth, the star, and the Sun. Then using simple trigonometry, they can determine the distance to this star. This technique is used in part to map out the shape of our Milky Way galaxy. A link is provided at the end of this answer.

To find the temperature of stars too far away to measure directly, we need to understand the relationship between heat and color. You may notice that, for example, a cool flame burns faint red or orange, but a hot flame burns bright blue. Analogously, scientists often use the color of a star to determine its temperature. They can classify the type of star by its color (and temperature). A red star, for instance, is about 3,500 – 6,000 F (2,000 – 3,500 C) whereas a blue star is about 20,000 – 50,000 F (11,000 – 28,000 C)! In fact, blue stars are classified as some of the hottest (and usually largest) objects in space. From looking at the composition of our Sun along with various other techniques, scientists make guesses as to the composition of other stars in our universe and conclude that, based on these high temperatures, the phase of the materials must be plasma.

click here please


Click Here to return to the search form.

University of California, Santa Barbara Materials Research Laboratory National Science Foundation
This program is co-sponsored by the National Science Foundation and UCSB School-University Partnerships
Copyright © 2020 The Regents of the University of California,
All Rights Reserved.
UCSB Terms of Use