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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. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
nova
dark matter
Black Hole
Perihelion
2. Clouds of low density gas often found glowing faintly on either side of an AGN.
Flare
Red Giant Branch Star
scarp
radio lobe
3. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Color Index
Autumnal Equinox
Light: travels like a wave - detected like a particle
meteor shower
4. A measure of the ability of a telescope to see fine detail
Make up of the jovian planets
greehouse effects
Resolving Power
Ecliptic
5. The shadow area behind the Earth or Moon where the Sun is completely obscured.
Trojan asteroids
supermassive black hole
Umbra
Blackbody Curve
6. The oldest part of the Milky Way
tectonics of Venus
Photon
Halo
Electromagnetic Radiation
7. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
Triple Alpha rocess
MOONS: roundest shape
Colestial Pole
H2 Regions
8. The mirror that determines the focus configuration of a reflector
aphelion
Gamma ray bursts
Electromagnetic Radiation
Secondary Mirror
9. Orbit in Jupiters orbit
CMB
Trojan asteroids
HII Region
Photosphere
10. The powdered stone fragments that make up the lunar 'soil'
contrast northern lowlands and the southern highlands of mars...
Electromagnetic Radiation
regolith
Jupiters red spot
11. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Photometry
Heliocentric
Sunspot cycle
Radiative Diffusion
12. A fusion process in which protons build together to form helium
quasar
mare basalt
Proton-proton chain
Asymptotic giant Branch Star
13. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Electromagnetic Radiation: Gamma Ray
Photometry
Main Sequence Stars
Thickest atmosphere
14. The north-south line passing directly overhead through the zenith.
Meridian
MOONS: larger than mercury
Particle Horizon
neutrino
15. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
fewest moons
Geocentric
Europa (Jupiters moon)
Rich vs poor clusters
16. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
supernova
Absolute Magnitude
Eyepiece Lens
molecular clouds
17. The imaginary sphere centered on the Earth that hols the stars.
Celestial Sphere
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
MOONS: most geologically active
Cepheid Variable
18. The oldest part of the Milky Way
Halo
Flat - Remain Parallel - Exactly 1
Total Eclipse
rotation curve=winding dilemma?
19. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
radiation pressure
Terrestrial Planets
Spectroscopic Parallax
20. A bright area of higher temperature that often proceeds the formation of sunspots.
Main Sequence Stars
Degeneracy
Synchrotron Rotation
Plague
21. The elementary building blocks from which protons and neutrons are formed.
Degeneracy
disk
A family of radiant energy- includes light
quarks
22. A term referring to the orbital character of stars near the Sun
terrestrial planet
Secondary Mirror
Differential Rotation
meteor
23. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Plague
H2 Regions
Kuiper belt
MOONS: larger than mercury
24. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
Secondary Mirror
Brown dwarf
semimajor axis
25. The mirror that gathers the light in a reflector
meteor
Spectral Lines
most moons
Primary Mirror
26. Then the Sun moves from north to south across the celestial equator (about September 23)
aphelion
jovian
Autumnal Equinox
Steady State Theory (Leads to Olber's Paradox)
27. The temp at which a substance in the vacuum of space solidifies
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
condensation temperature
Chandrasekhar Limit
Differential Rotation
28. What causes the zones and belts on jupiter and saturn?
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
cosmological red shift
Plank's Law
conjunction
29. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Dark Nebula
High Velocity Stars
Io (jupiters moon)
Absolute Magnitude
30. The lowest energy of an atom.
cosmology
Ground State
Europa (Jupiters moon)
Most dense
31. What do we think the actual fate of the universe will be and why do we think this?
Chandrasekhar Limit
partile horizon
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.
chemical differentiation
32. A change in the appearance of the sun at the edge of the solar disk
Limb darkening
synchronous rotation
Spectroscopy
Cosmic Microwave Background (CMB)
33. Ganymede
High Velocity Stars
Particle Horizon
Granules
MOONS: largest size
34. Possible Fates of the Universe
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
Supercluster
chondrite
dark energy
35. Moon in less than the angular diameter of the Sun.
radio galaxy
Parallax
Annular Eclipse
tectonics of Earth
36. The family of radiant energy that includes light as a subset
Negative - Diverge - Less than 1
Blackbody Curve
Electromagnetic Radiation
Sb spiral galaxy
37. What are the three possible geometries of the universe?
Planck time
Dark matter candidates
Open - flat - and closed.
blazar
38. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
Make up of the terrestrial planets
hottest surface
planetary nebula
Ole Roemer
39. Saturn
coma
Cosmic Microwave Background (CMB)
least dense
dark matter
40. The equation that describes how matter equates with energy
Filament
Plank's Law
fastest rotation
E=mc2
41. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
Main Sequence Stars
Dwarf planets
Doppler Shift
Cosmological Principle
42. Sc galaxies
Olber's paradox
Flocculent spirals
dark matter
great red spot
43. A small chunk of rock in space
density waves
meteoriod
Kuiper belt
Ammonia - methane - and water
44. Approximate speed of light in a vacuum
meteor shower
Dwarf planets
300000 KM/sec
MOONS: larger than mercury
45. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Superior planets
Granules
Big Crunch
radio galaxy
46. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
difference between maria and highlands of the moon.
isotropic
Geocentric
synchrotron radiation
47. 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
Horizontal Branch Star
Galilean satellite
density
48. The source of the force that is accelerating the expansion rate of the universe.
condensation temperature
dark energy
Ole Roemer
supermassive black hole
49. Stars fromt he Halo that have drifted into the disk. as earth zooms past them in a faster orbit they appear to be going backward very fast
Degeneracy
Bok Globule
High Velocity Stars
Drake equation
50. A spinning neutron star
Perihelion
regolith
Flat - Remain Parallel - Exactly 1
Pulsar