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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. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
terrestrial planet
Absorption Spectrum
Red Giant
deferent
2. Ganymede and Titan
cosmology
MOONS: larger than mercury
Halo
Planetary Nebula
3. The layer of the sun just above the photosphere
epicycle
radio lobe
Penumbra
Chromosphere
4. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
shape and color of SPIRAL galaxies
cosmic singularity
Inverse Square Law
Sunspot cycle
5. The sinking of denser elements to the center of a young molten planet
tectonics of Earth
dark energy
Autumnal Equinox
chemical differentiation
6. Hot cells of gas that rise and fall in the hotosphere
Black Hole
Synchrotron Rotation
Granules
least dense
7. The part of the Milky way that has on-going star formation
Reflector
Disk
scarp
Electromagnetic Radiation: Visible Light
8. The entity from which the whole universe is postulated to have come from.
cosmic singularity
Population 1 vs Population 2 stars
Dwarf planets
Quasar
9. The point in its orbit where a planet is farthest from the sun
synchrotron radiation
density parameter
Apollo asteroids
aphelion
10. 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)
Synodic Day
nucleus
H2 Regions
Disk
11. An element of a highly efficient - two-dimensional electronic light detector
Pixel
Galilean satellite
homogeneous
Limb darkening
12. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Black Hole
Colestial Pole
matter dominated universe
epicycle
13. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Cosmic Microwave Background
Main Sequence
tectonics of Earth
Electromagnetic Radiation: Infrared
14. What is the universe expanding into?
most eccentric orbit
Metals
partile horizon
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
15. A small round distribution of gas surrounding a dying star
Nebula
We don't know. It might be but does not have to be.
Planetary Nebula
differential rotation
16. A galaxy sending out a stream of material from its nucleus
Extrasolar Planet
Chandrasekhar Limit
Radio Galaxy
Dark Nebula
17. 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
Pulsar
High Velocity Stars
fewest moons
conjunction
18. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
highlands
meteor shower
quarks
Sa spiral galaxy
19. The law that describes the blackbody curve - and let to quantum mechanics.
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20. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
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
Plague
Colestial Pole
Neutron Star
21. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Negative - Diverge - Less than 1
Halo
Blackbody
Energy Level
22. 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
terrestrial planet
Oort cloud
Milky way Galaxy
Kuiper belt
23. Venus
Parsec
Roundest orbit
The Big Bang Theory resolves Olber's Paradox
Umbra
24. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
opposition
accretion
Autumnal Equinox
Dark Nebula
25. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Precession
meteoriod
Spectroscopic Parallax
Shepherd satellite
26. 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
rotation curve=winding dilemma?
Flat - Flat
reflection star clusters
Halo
27. The part of the Milky way that has on-going star formation
Largest diameter
Prominence
Disk
Nucleus
28. The process of acquiring material
accretion
Flat - Remain Parallel - Exactly 1
isotropic
great dark spots
29. A planet that is closer to the sun than the earth
Red Giant Branch Star
Photon
aurora
inferior planets
30. 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.
Enke gap
Jovian Planets
Population 1 vs Population 2 stars
asteroid
31. A distance measure determined by the shifting of a star against the background sky every 6 months.
Parsec
Flat - Flat
Drake equation
Reflector
32. In what chemical form are jupiters nitrogen - carbon and oxygen?
If it is in a denser medium - such as glass - it will move slower
Electron
Ammonia - methane - and water
Electromagnetic Radiation: Ultraviolet Light
33. The measure of a variable star's apparent magnitude as it brightens and dims with time
Light Curve
epicycle
Sunspots
meteor shower
34. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Milky way Galaxy
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
supermassive black hole
molecular clouds
35. The entity responsible for spiral arms in grand-design spiral galaxies
Supernova (You can be my supernova girl)
Density Wave
great dark spots
coma
36. VENUS
radiation pressure
Bok Globule
cosmic fireball
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
37. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
zone
CNO Cycle
MOONS: most geologically active
Seeing
38. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Seyfert galaxy
mass
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
cosmic singularity
39. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
Nebula
Degeneracy
Parallax
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.
40. A phenomenon seen when the Earth passes through the orbit of a burned out comet
accretion
general star population
meteor shower
inferior planets
41. The light produced when particles from the sun collide with atmospheric molecules
Olber's paradox
aurora
Seeing
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.
42. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
belt
Pixel
rotation curve=winding dilemma?
Emission Spectrum
43. How did Earth come to have an oxygen rich atmosphere?
Resolving Power
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.
Halo
Black Hole
44. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
dark energy
mass
Oort Cloud
density waves
45. The rotation period of the Earth measured relative to the stars.
force
Spectral Lines
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Sidereal Day
46. 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
isotropic
self-propagating star formation
Enke gap
47. A star that erratically and explosively brightens and dims
Halo
fusion crust
Rich vs poor clusters
Nova
48. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Emission Spectrum
Flat - Flat
Sa spiral galaxy
accretion
49. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
density
standard candle
Meridian
Seyfert galaxy
50. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Bulge
slowest rotation
Rich Cluster
The Local Group