chapter 30.1: characteristics of stars. at the center of the most violent starburst region in the...
TRANSCRIPT
Chapter 30.1: Characteristics of
Stars
At the center of the most violent starburst region in the local universe lies a cluster of brilliant, massive stars, known to astronomers as Hodge 301 (lower right hand corner of this photo)
Characteristics of Stars A star is a body of gases that gives off
energy in the form of light & heat. Size varies Color varies based on temperature Our sun is an average star
Composition Star composition observed through a spectrometer
Separates light into its individual colors Each color represents a different wavelength Three types of spectra
Emission or bright-line Absorption or dark-line Continuous
Since different elements absorb different wavelengths of light , elements can be determined.
Composition Continued Hydrogen is the most common element. Surface temperature of a star is indicated
by the color Red stars are the coolest and blue are the
hottest (Figure 2 on page 776).
Motion Two kinds of motion associated with
stars: Actual motion --- just like it sounds! Apparent motion --- This is motions visible
to the unaided eye in a dark sky; due to movement of Earth.
Motion Continued
Some stars create circular trails around a central star (Polaris aka the North Star)
Circumpolar: stars that never go below the horizon. (Circling stars).
Different stars become visible during different seasons.
Three actual motions:1. Rotate on an axis2. Revolve around another star3. Move away or toward the Earth.
Distance Distance
Light Year = 9.5x1012km; Distance that light travels in one year.
Astronomical Unit (AU) --A unit of length used to measure distances in solar system.
Stellar Magnitude
Magnitude: a way to measure the brightness of a body in the sky
Apparent magnitude = brightness of a star as it appears to us on Earth
Measure light from star using telescopes Measurement is then assigned a number
Brightest stars have lowest numbers Dimmest stars have highest numbers
Absolute: the true brightness of the object