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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. A telescope that uses mirrors to focus light
aphelion
Reflector
MOONS: most geologically active
Red Giant Branch Star
2. When the Moon entirely blocks the Sun.
Synchrotron Rotation
Spectral Lines
Total Eclipse
Grand design spirals
3. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Synchrotron Rotation
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.
Light Gathering Power
Black Hole
4. 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)
Spectroscopic Parallax
meteoriod
Coldest surface
general star population
5. A collection of galaxies like the one the Milky Way belongs to
If it is in a denser medium - such as glass - it will move slower
Photometry
Poor Cluster
Europa (Jupiters moon)
6. When one side of a body always faces the planet it revolves around
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.
Electromagnetic Radiation: Radio
Supernova (You can be my supernova girl)
synchronous rotation
7. The displacement of spectral lines to redder colors caused by the expansion of the universe.
Eyepiece Lens
Triple Alpha rocess
Bulge
cosmological red shift
8. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
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
accretion disk
MOONS: most geologically active
Nucleus
9. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
Yes - frozen at the poles- remains protected from the suns rays
isotropic
tectonics of Mars
Interstellar Extinction
10. The family of radiant energy that includes light as a subset
Electromagnetic Radiation
Astronomical Unit
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
Molecular Clouds
11. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
blazar
density parameter
self-propagating star formation
Colestial Pole
12. Distance from sun to nucleus- 8 kiloparsecs (26000 LY) - diameter of Milky way- 150000 LY - length for sun to orbit once around milky way- 250 million years
Kuiper belt
contrast northern lowlands and the southern highlands of mars...
Radio Galaxy
Milky way Galaxy
13. Mercury and venus
Filament
belt
aurora
fewest moons
14. A star fusing hydrogen to helium in it's core
Jovian Planets
Main Sequence Stars
highlands
opposition
15. The Big Bang was not an explosion of matter into empty space - like the explosion of a bomb. Instead - it was an emergence of space and time filled with pure energy where before none of this was present. The point from which is emerged is called the
The Big Bang Theory
Electromagnetic Radiation: Visible Light
AGN
planetesimal
16. 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:
Drake equation
Sunspots
meteor shower
Photosphere
17. A word meaning 'the same in all directions.'
Electromagnetic Radiation: X-Ray
isotropic
Annular Eclipse
great dark spots
18. A fusion process in which protons build together to form helium
conjunction
Proton-proton chain
density
dark matter
19. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
greatest elongation
Turn off Point
force
Self-Propogating Star Formation
20. The crust of a meteorite caused by its entry into Earth's atmosphere
Synodic Day
Callisto (Jupiter)
fusion crust
blazar
21. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
Make up of the jovian planets
least dense
disk
Make up of the jovian planets
22. Any class of objects with a uniform luminosity used to determine distance.
cosmic fireball
radiation dominated universe
standard candle
Make up of the terrestrial planets
23. A star that erratically and explosively brightens and dims
Nova
Ground State
thinnest atmosphere
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
24. A quantity measuring the stability of the Earth's atmosphere
Liquid metallic hydrogen
SETI
Flocculent spirals
Seeing
25. When a planet lines up with the sun inthe sky
conjunction
Parallax
semimajor axis
meteor shower
26. The dark - relativley smooth areas on the moon; Latin for sea
Maria
belt
Superior planets
Void
27. All wavelengths of light emitted by a blackbody.
Electromagnetic Radiation: X-Ray
Spectroscopy
Blackbody Curve
CCD
28. The point directly overhead.
Zenith
Gamma ray bursts
supermassive black hole
Self-Propogating Star Formation
29. Either Io -Europa - Ganymede - or Callisto
Kuiper belt
Galilean satellite
Electromagnetic Radiation: Microwave
Colestial Pole
30. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
greatest elongation
Penumbra
Electromagnetic Radiation: X-Ray
31. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
Electromagnetic Radiation
acceleration
reflection star clusters
Radiative Diffusion
32. The 'edge' of the universe. Light beyond this has not reached us yet.
Ole Roemer
Drake equation
partile horizon
Corona
33. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Gamma ray bursts
terrestrial planet
Titus-Bode Law
jovian
34. When one side of a body always faces the planet it revolves around
synchronous rotation
density
dark energy
Emission Spectrum
35. Radiation given off by electrons accelerating in a magnetic field
Quasar
difference between maria and highlands of the moon.
H2 Regions
Synchrotron Rotation
36. Is space infinitely large?
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37. The force of attraction between any two objects having mass
gravity
radiation pressure
accretion disk
How is winding dilemma solved?
38. The distance between a lens and its focal plane
Galilean satellite
Focal Length
Coldest surface
Annular Eclipse
39. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
quasar
Degeneracy
quarks
most moons
40. The shadow behind the Earth or Moon where the Sun is partially obscured.
Red Giant
Penumbra
fusion crust
Big Bang
41. Jupiter - Saturn - Uranus - Neptune
Occam's razor
Jovian Planets
Main Sequence
Cepheid Variable
42. The rotation period of the Earth measured relative to the Sun.
Neutron Star
Rich vs poor clusters
Thermonuclear Fusion
Synodic Day
43. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Hydrostatic Equilibrium
homogeneous
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Electromagnetic Radiation
44. A crystalline patter found in iron meteorites
highlands
widmanstatten pattern
Astronomical Unit
cosmological red shift
45. The science of measuring light energy by wavelength.
slowest rotation
roche limit
Hyashi track
Spectroscopy
46. The oldest grouping of stars - found in the galaxy halo
Seyfert galaxy
acceleration
Globular Cluster
matter dominated universe
47. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Nebula
aphelion
nova
Pulsar
48. Jupiter
Rich Cluster
Hipparchus
Largest diameter
Open - flat - and closed.
49. The mass of an object divided by its volume
Supercluster
Magnification
density
Superior planets
50. The act of removing an electron from an atom.
Poor Cluster
Cepheid Variable
Turn off Point
Ionization
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