Define it!
True or False?
Nuclear
Measures
Stars
Grab Bag
100

The process by which two or more small nuclei fuse to make a bigger nucleus

Nuclear fusion
#1a SG

100

The earth’s solar system belongs in the Milky Way, which belongs to the Local Group, which belongs to the Virgo Cluster.

True
#23 SG

100

What is true about the starting mass and ending mass of both nuclear fusion (in the sun) and nuclear fission (in a nuclear power plant) processes?

The starting mass is larger than the ending mass
(mass is converted into energy in both processes)
#7 SG

100

The term for the distance light could travel along a straight line in one year.

Light year
#1f SG

100

What part of the sun do we see?

The photosphere
#4 SG

100

The term for a large ensemble of stars, all interacting through the gravitational force and orbiting around a common center.

Galaxy
#1g SG

200

The process by which a large nucleus is split into smaller nuclei

Nuclear fission
#1b SG

200

The crab nebula was most likely formed by a pulsating variable.

False
(it was most likely formed by a supernova, which is an exploding star; supernovas leave behind a cloud of bright gases – called a nebula)
#18 SG

200

Why is nuclear fusion considered a better option for energy production than nuclear fission?

There are no radioactive byproducts, there is no chance of meltdown, and the starting materials are cheap
#9 SG

200

Why are Cepheid variables so important for measuring long distances in the universe?

They seem to have a relationship between their period & their magnitude
(this allows them to be used in the apparent magnitude method for measuring long distances in the universe)
#20 SG

200

Name the four regions of the sun from the inside to the outside.

The core, the radiation zone, the convection zone, and the photosphere
#2 SG

200

What type of galaxy is the Milky Way?

A spiral galaxy
#21b SG

300

The amount of isotope necessary to sustain a chain reaction

Critical mass
#1c SG

300

Of the two methods for measuring the distance from earth to a star (parallax and apparent magnitude methods), the parallax method is the most accurate.

True
#19a SG

300

Why is it impossible for a nuclear power plant to have a nuclear explosion?

A power plant does not have significantly more than the critical mass of the large nucleus that is breaking apart
#8 SG

300

Why do most astronomers believe the universe is expanding?

The light from nearly every galaxy experiences a red shift before it reaches the earth
(and the red shift increases the farther the galaxy is from the earth)
#24 SG

300

How does the sun get its power, and in which region of the sun does this process occur?

The sun gets its power from nuclear fusion that occurs in the core.
#3 SG

300

What are the four basic types of galaxies?

Spiral, lenticular, elliptical, and irregular
#21a SG

400

The brightness of a star, corrected for distance, on a scale of -8 to +19. The smaller the number, the brighter the star.

Absolute magnitude
#1d SG

400

Of the two methods for measuring the distance from earth to a star (parallax and apparent magnitude methods), the apparent magnitude method can be used to measure long distances.

True
#19b SG

400

Why can’t we use nuclear fusion to produce energy yet?

We cannot master the technology to make it economically feasible.
#10 SG

400

If the universe is expanding, does the geometry of the expansion matter?

Yes
(the geometry makes a great deal of difference)
#25a SG

400

What similarity exists between novas, supernovas, and pulsating variables?

They are all variable star types
(their brightness changes radically with time)
#16 SG

400

Stars group together to form ______, which group together to form _____, which group together to form ______, some of which group together to form ______.
(Fill in using: clusters, galaxies, superclusters, and groups)

Stars group together to form galaxies, which group together to form groups, which group together to form clusters, some of which group together to form superclusters.
#22 SG

500

The brightness of a star as seen in the night sky. The smaller the number, the brighter the star.

Apparent magnitude
#1e SG

500

A supergiant star is at:
Magnitude -7
Spectral Letter F
(Confirm this star type on the H-R Diagram on page 421.)

True
#11c SG

500

Two 4He nuclei collide and turn into a 7Be nucleus and one neutron. Is this nuclear fusion or nuclear fission?

Nuclear fusion
(Since two small nuclei became a bigger nucleus plus a neutron)
#6 SG

500

Why does the geometry of the expansion of the universe matter?

It is the basis to develop theories about the universe’s formation
(the theories depend on the assumed geometry)
#25b SG

500

What is the big difference between novas, supernovas, and pulsating variables?

Lifetime
(pulsating stars last a long time, supernovas exist very briefly, and novas are somewhere in between)
#17 SG

500

Put these stars in order by increasing size – red giant, main sequence, supergiant, and white dwarf.
(hint: pay attention to the names; also see page 408)

White dwarf, main sequence, red giant, and supergiant
#13 SG

600

This type of star is at:
Magnitude -1
Spectral Letter K
(Find this star type on the H-R Diagram on page 421.)

Red giant
#11a SG

600

A supergiant star is at:
Magnitude 0
Spectral Letter B
(Confirm this star type on the H-R Diagram on page 421.)

False
(This is a main sequence star, like our sun.)
#11b SG

600

A 251Cf nucleus is bombarded with a neutron. It breaks down into a 124Sn nucleus, a 120Cd nucleus, and 7 neutrons. Is this nuclear fission or nuclear fusion?

Nuclear fission
(Since a large nucleus split into two smaller nuclei and a few neutrons)
#5 SG

600

To classify a star, find it on the H-R Diagram on page 421. Its measures are:
Magnitude 11
Spectral Letter B

White dwarf
#11d SG

600

Of these stars – red giant, main sequence, supergiant, and white dwarf – which is most like our sun? Which is coolest in temperature?

Most like our sun = main sequence
Coolest = red giant
 #12 & 15 SG

600

Put these stars in order by increasing brightness – red giant, main sequence, supergiant, and white dwarf.
(hint: the smaller the magnitude, the brighter the star; also see the H-R Diagram on page 421)

White dwarf, main sequence, red giant, and supergiant
#14 SG