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Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. Population 1 with higher metals and contain many young stars in star clusters. Distribution of stars is everywhere in disk (arms only have 5% more stars)
High Velocity Stars
general star population
MOONS: most geologically active
Cosmic Microwave Background (CMB)
2. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Photometry
Make up of the terrestrial planets
mapping the structure of Milky Way disk
zone
3. A continuous spectrum of light missing energy at a few wave lengths.
disk
Absorption Spectrum
Ionization
We don't know. It might be but does not have to be.
4. The crust of a meteorite caused by its entry into Earth's atmosphere
Proton-proton chain
evidence of water on mars
evidence of water on mars
fusion crust
5. A small chunk of rock in space
meteoriod
Dwarf planets
Seeing
Rich Cluster
6. Approximate speed of light in a vacuum
cosmological principle
300000 KM/sec
Chromosphere
radiant
7. Ganymede and Titan
MOONS: larger than mercury
Electromagnetic Radiation: Microwave
Halo
Main Sequence Stars
8. What causes the zones and belts on jupiter and saturn?
Cepheid variables
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
White Dwarf
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
9. Possible Fates of the Universe
Electromagnetic Radiation: Radio
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
Turn off Point
Vernal Equinox
10. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Annular Eclipse
density parameter
Oort cloud
Main Sequence
11. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Filament
We don't know. It might be but does not have to be.
Electromagnetic Radiation
Nebula
12. An object that may remain after a star explodes
Red Giant
Sidereal Day
Neutron Star
general star population
13. 100 nm 10 nm
Photometry
Electromagnetic Radiation: Ultraviolet Light
Proton-proton chain
Kirchhoff's Law
14. The elementary building blocks from which protons and neutrons are formed.
quarks
Population 1 vs Population 2 stars
most moons
Make up of the terrestrial planets
15. The rock that makes up the lunar maria
Meridian
comet
Plague
mare basalt
16. Hot cells of gas that rise and fall in the hotosphere
Positive - Converge - Greater than 1
Granules
Coldest surface
Light: travels like a wave - detected like a particle
17. 100 nm 10 nm
Halo
radio galaxy
MOONS: most geologically active
Electromagnetic Radiation: Ultraviolet Light
18. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
dark energy
Hydrostatic Equilibrium
opposition
dark energy
19. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
evidence of water on mars
Seyfert galaxy
Electromagnetic Radiation
Cassegrain Focus
20. A star that blows itself apart
Supernova (You can be my supernova girl)
Summer Solstice
Magnification
epicycle
21. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
deferent
Plague
difference between maria and highlands of the moon.
22. A star that is burning hydrogen to helium in a shell surrounding it's core
Grand design spirals
Red Giant Branch Star
High Velocity Stars
force
23. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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24. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Ganymede (Jupiter)
Primary Mirror
Asymptotic giant Branch Star
Focal Length
25. What Ole Roemer used to measure the speed of light in a vacuum
Eclipses of the Moons of Jupiter
force
Flat - Flat
Dark matter candidates
26. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Sa spiral galaxy
great red spot
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
standard candle
27. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Asymptotic giant Branch Star
Open - flat - and closed.
Europa (Jupiters moon)
epicycle
28. The study of the universe as a whole.
Kuiper belt
cosmology
Granules
Penumbra
29. N=are*Fp(Ne)(Fl)(Fi)(Fc)(L) N: number of civilizations possible to communicate with are*: rate solar-like stars are created Fp: fraction of stars with planets Ne: number of planets like ours Fl: fraction of planets with life Fi: intelligent life Fc:
Hydrostatic Equilibrium
Radio Galaxy
The Big Bang Theory
Drake equation
30. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Differential Rotation
Light Curve
smallest diameter
The Local Group
31. A bridge of material held in position above the solar surface. They can remain for hours even days
belt
zone
jovian
Prominence
32. The movement of the Earth's crustal plates riding on top of the mantle.
Energy Level
synchrotron radiation
cosmology
plate tectonics
33. The lowest energy of an atom.
MOONS: roundest shape
Ground State
Sc spiral galaxy
Parallax
34. The Greek philosopher responsible for making the stellar magnitude scale.
Eyepiece Lens
Seeing
Red Giant
Hipparchus
35. The rock that makes up the lunar maria
Molecular Clouds
mare basalt
Gamma ray bursts
great red spot
36. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Make up of the terrestrial planets
neutrino
quasar
Ionization
37. The rotation period of the Earth measured relative to the stars.
OB Associations
Sidereal Day
molecular clouds
most moons
38. Venus
OB Associations
dark matter
Roundest orbit
disk
39. A prominence seen against the disk of the sun
opposition
Pixel
Filament
Cassegrain Focus
40. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
Main Sequence
condensation temperature
mapping the structure of Milky Way disk
cosmic singularity
41. When massive objects bend space and time enough to create multiple images of an object located behind them
molecular clouds
Gravitational Lens
Negative - Diverge - Less than 1
Electron
42. The organization of clusters of galaxies into sheets and strings
HII Region
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
Supercluster
Parsec
43. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
shape and color of SPIRAL galaxies
Kirkwood gaps
Population 1 vs Population 2 stars
44. That which is responsible for Jupiter's magnetic field
meteor
Reflector
Liquid metallic hydrogen
Ground State
45. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
aphelion
Dark Nebula
Synchrotron Rotation
Cepheid Variable
46. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
How is winding dilemma solved?
Limb darkening
Largest diameter
47. In what chemical form are jupiters nitrogen - carbon and oxygen?
coma
Ammonia - methane - and water
Electromagnetic Radiation: Infrared
neutrino
48. Jupiter
Spectroscopy
Electromagnetic Radiation: Ultraviolet Light
Grand design spirals
fastest rotation
49. A particle of light.
highlands
Photon
CMB
Enke gap
50. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
Spectroscopic parallax
Sc spiral galaxy
supernova
Terrestrial Planets