-
The Great Red Spot of Jupiter has been observed since
the 1600s.
-
**The basic energy source in the interior of the Sun is the nuclear energy derived from the fusion of
hydrogen into helium
-
**Which of the following is a problem inherent to individual radio telescopes?
poor angular resolution
-
The temperature of the solar photosphere is about
5,800 K.
-
The Zeeman effect describes what changes in spectral lines?
Line splitting due to intense magnetic fields
-
In general, the Jovian planets differ from the terrestrial planets in several important features. Which of the following is not one of these features?
(less dense, more massive, longer rotation periods, considerably larger in size)
longer rotation periods
-
What is the average length of time from one time of sunspot maximum on the Sun until the next time of sunspot maximum?
11 years
-
**Two forms of electromagnetic radiation that penetrate Earth's atmosphere are
Visible light and radio waves
-
Where are the main belt asteroids generally found in the solar system?
Between the orbits of Mars and Jupiter
-
The light from the visible surface of the Sun comes from which atmospheric layer?
Photosphere
-
What natural barrier tries to prevent two protons from combining?
Electromagnetic repulsion
-
Asteroids associated with the Lagrange points in the orbit of Jupiter are called
Trojan asteroids
-
The dark appearance of sunspots indicates that they are ______ the surrounding surface of the Sun.
cooler than
-
**The four giant moons of Jupiter were discovered by
Galileo
-
The only satellite in the solar system known to have a dense atmosphere is _________. It is one of the satellites of Saturn
Titan
-
Which of the following properties is constant for all types of electromagnetic waves?
speed
-
**Which of the following is a problem inherent to individual radio telescopes?
They have poor angular resolution.
-
**Which kind of process, as a net result, supplies the energy of our Sun?
Hydrogen atoms are converted to helium through fusion.
-
Observation of the shift of a star's spectrum toward the red or the blue enables us to determine the star’s
radial velocity.
-
Name the second most abundant element in the Sun.
Helium
-
Which of the following is one of the many contributions Galileo Galilei made to astronomy?
He used a telescope to observe the heavens, thereby reinforcing the notion of heliocentricity.
-
**Where are asteroids generally found in the solar system?
Between the orbits of Mars and Jupiter
-
If you view a hot star through a cool cloud of gas, what sort of spectrum are you likely to see?
Absorption
-
**The temperature of the solar photosphere is about
5,800 K.
-
Adaptive optics are used to correct what problem?
Atmospheric turbulence
-
**The amount of light reflected by a planet or other object is its
albedo
-
**The Zeeman effect describes what changes in spectral lines?
Line splitting due to intense magnetic fields
-
How was Uranus discovered?
By accident, by an astronomer who was conducting a sky survey
-
Suppose you are at the Tropic of Cancer, which has a latitude of 23.5°. The altitude of the north celestial pole as seen from your position is:
- 23.5°
- (same number - the altitude of the north celestial pole is always the same as your latitude)
-
The planet that rotates on its axis with a period almost identical to that of the Earth is
Mars
-
Suppose you see the Moon in the sky one evening. The next evening, it will have moved
to the east
-
In 1928 the International Astronomical Union divided the entire sky into ______ officially recognized constellations.
88
-
**What is the primary ingredient in the Earth's atmosphere?
Nitrogen
-
Which of these is LEAST important to an astronomer for observing stars?
magnifying power
-
The absolute magnitude of a star is defined to be the apparent magnitude that the star would have if it were at a standard distance of ______ parsec(s).
10
-
The apparent magnitude of the Sun is about
-27
-
Which of the following would be considered to be a correct spectral type and luminosity class for our Sun?
G2V
-
A parsec is defined as the distance to an object which has a parallax of _____ second(s) of arc.
1
-
A fifth-magnitude star is times brighter than a fifteenth-magnitude star.
10,000
-
If you view a typical star with a spectrograph, what type of spectrum are you likely to observe?
Absorption
-
The luminosity of a star is a unique measure of its
total energy output
-
Which of these is the greatest distance?
1 parsec
-
All F-type stars have approximately the same
temperature
-
The absolute magnitude of the Sun is about
+5
-
**The spectrum of a typical gaseous nebula illuminated by an early B-type star is
an emission spectrum.
-
An eighth-magnitude star is times brighter than a tenth-magnitude star.
6 3/10
-
A telescope of large aperture is better than one of small aperture because of
greater resolving power
-
Which two ingredients are needed to make an emission nebula?
Hot stars and interstellar gas
-
Stars which are just forming (protostars) radiate most of their energy and are most commonly detected in
infrared
-
**What is NOT thought to be approximately the same for each star in a cluster?
mass
-
**What inevitably forces a star like the Sun to evolve away from the main sequence?
It builds up a core of helium
-
**What is the most important physical characteristic in determining the time that a given star spends on the main sequence?
Mass
-
**A galactic cluster is young if
it has an H-R diagram that resembles a complete main sequence.
-
The H-R diagram is a plot of
luminosity versus spectral type.
-
Another term for luminosity
absolute magnitude
-
Spectral type is based on...
temperature
-
**What inevitably forces a star like the Sun to evolve away from being a main sequence star?
It builds up a core of helium
-
Which of the following definitely does NOT agree with present theories of stellar evolution?
- [the misconception that] more massive stars evolve more slowly than the less massive stars
- (Actually, the bigger the star, the more rapidly they evolve.)
-
**A galactic cluster is young if
it has an H-R diagram that resembles a complete main sequence.
-
**What is the most important physical characteristic in determining the time that a given star spends on the main sequence?
Mass
-
**The spectrum of a typical gaseous nebula illuminated by a B-type star is
an emission spectrum
-
Which of the following are not intrinsic type variable stars?
Eclipsing binaries
-
If we know only the period for a Cepheid variable star, we can estimate its
absolute magnitude
-
A binary system cannot be seen as an eclipsing system if
its orbital plane is perpendicular to the line of sight.
-
Spectroscopic studies of Cepheids show that their changes in brightness are correlated with changes in
size
-
The masses of stars other than the Sun would be unknown without the study of
binary stars
-
The distances to the nearby galaxies like M33 in Triangulum are based primarily on observations of the periods of the which can be seen in these nearer galaxies.
Cepheid variable stars
-
**Stars which are just forming (protostars) radiate most of their energy and are most commonly detected in
infrared
-
The variable star delta Cephei is a classic example of a/an
classical Cepheid
-
The type of intrinsic variable stars known as stars have periods ranging from a few hours to one day and are often found in globular clusters. They are sometimes referred to as cluster variables. They are often used to estimate distances to globular clusters.
RR Lyrae
|
|