SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
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 amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Resolving Power
3 reasons we orbit satellites to observe universe
critical density
fusion crust
2. The science of measuring light energy by wavelength.
Steady State Theory (Leads to Olber's Paradox)
Spectroscopy
Sunspots
Flare
3. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Negative - Diverge - Less than 1
Halo
Globular Cluster
asteroid
4. Possible Fates of the Universe
Hubble law
density parameter
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
Occam's razor
5. Ganymede and Titan
MOONS: larger than mercury
standard candle
Objective Lens
Umbra
6. In what chemical form are jupiters nitrogen - carbon and oxygen?
Grand design spirals
Ammonia - methane - and water
fewest moons
jovian
7. The location around an atom where an electron resides.
White Dwarf
Energy Level
Bulge
Cepheid Variable
8. A two-filter measure of the color - and hence temperature - of a star.
Hydrostatic Equilibrium
Color Index
density waves
Open - flat - and closed.
9. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
Black Hole
Dark Nebula
Population 1 vs Population 2 stars
MOONS: thickest atmosphere
10. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
Photon
thinnest atmosphere
Nebula
AGN
11. The part of the Milky way that has on-going star formation
Disk
Dwarf planets
Galilean satellite
Ammonia - methane - and water
12. What do we think the actual fate of the universe will be and why do we think this?
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.
quasar
Europa (Jupiters moon)
The Big Bang Theory
13. VENUS
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
Light-Year
Blackbody
Sidereal Day
14. A very dense - highly populated cluster of galaxies
fewest moons
Rich Cluster
Photon
rotation curve=winding dilemma?
15. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
Flare
greehouse effects
Dark Matter
Halo
16. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
mapping the structure of Milky Way disk
Precession
era of recombination
Ganymede (Jupiter)
17. That which is responsible for Jupiter's magnetic field
Thermal Equilibrium
comet
Synchrotron Rotation
Liquid metallic hydrogen
18. When one side of a body always faces the planet it revolves around
synchronous rotation
Thickest atmosphere
Inverse Square Law
AGN
19. Half of the longest diameter across an ellipse
semimajor axis
least dense
Primary Mirror
rotation curve=winding dilemma?
20. A large and bright but cool star.
reflection star clusters
most moons
smallest diameter
Red Giant
21. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
gravity
Light Curve
OB Associations
Flat - Remain Parallel - Exactly 1
22. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
tectonics of Earth
retrograde motion
E=mc2
Prominence
23. A representation of the changes in color and brightness of an evolving protostar.
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
We don't know. It might be but does not have to be.
Hyashi track
Gamma-ray Burst
24. The number of protons in an atom.
Flat - Flat
Degeneracy
jovian
Atomic Number
25. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
Nebula
Make up of the terrestrial planets
radiation pressure
Zenith
26. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
Hubble law
Blackbody
Dark Nebula
Astronomical Unit
27. A small round distribution of gas surrounding a dying star
Oort Cloud
Olber's paradox
interstellar dust
Planetary Nebula
28. The mass of an object divided by its volume
density
meteor shower
cosmic fireball
Flat - Flat
29. Infinitely long -> 10 cm
reflection star clusters
Electromagnetic Radiation: Radio
E=mc2
Main Sequence Stars
30. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
Sunspot cycle
critical density
HII Region
Electromagnetic Radiation
31. The rotation period of the Earth measured relative to the Sun.
matter dominated universe
solar nebula
Limb darkening
Synodic Day
32. A quantity measuring the stability of the Earth's atmosphere
semimajor axis
Ionization
Seeing
Atomic Number
33. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Big Crunch
dark matter
Thermal Equilibrium
Poor Cluster
34. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
fewest moons
radio galaxy
Continuous Spectrum
thinnest atmosphere
35. Venus
tectonics of Venus
Thickest atmosphere
tectonics of Mars
Kirkwood gaps
36. A plot of star absolute magnitude verses spectral type.
Photon
Summer Solstice
belt
H-are Diagram
37. The rock that makes up the lunar highlands
Limb darkening
anorthosite
Spectral Lines
protostar
38. Dark areas on the sun that are cooler than the surrounding photosphere
Shepherd satellite
Limb darkening
Sunspots
The Local Group
39. A star without enough mass to begin hydrogen fusion
Chromosphere
plate tectonics
fastest rotation
Brown dwarf
40. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
thinnest atmosphere
Absorption Spectrum
bulge
A family of radiant energy- includes light
41. The distance between a lens and its focal plane
Focal Length
Photosphere
Kirkwood gaps
Hydrostatic Equilibrium
42. The entity responsible for spiral arms in grand-design spiral galaxies
Density Wave
Terrestrial Planets
cosmic fireball
Light: travels like a wave - detected like a particle
43. The location of a supermassive black hole
Zenith
Nucleus
Ecliptic
Synchrotron Rotation
44. A planet orbiting about a distant star
radiation pressure
Cosmic Microwave Background (CMB)
Extrasolar Planet
synchrotron radiation
45. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Halo
Photon
Color Index
Occam's razor
46. Jupiter
conjunction
most moons
Secondary Mirror
Objective Lens
47. An element of a highly efficient - two-dimensional electronic light detector
Pixel
Titus-Bode Law
cosmic fireball
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
48. Why does the earth have few craters while the moon has many?
Gamma ray bursts
epicycle
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Cassini division
49. Mercury
Nucleus
aurora
Halo
thinnest atmosphere
50. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
Seyfert galaxy
Io (jupiters moon)
most moons
Brown dwarf