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 location of a supermassive black hole
AGN
Positive - Converge - Greater than 1
Absorption Spectrum
Nucleus
2. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
conjunction
Dark Nebula
Lagrangian Razor
Void
3. Mercury and venus
HII Region
Resolving Power
Kirchhoff's Law
fewest moons
4. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
Lagrangian Razor
Hubble law
homogeneous
Europa (Jupiters moon)
5. Approximate speed of light in a vacuum
300000 KM/sec
Steady State Theory (Leads to Olber's Paradox)
Ground State
neutrino
6. The location around an atom where an electron resides.
Most dense
acceleration
Convection
Energy Level
7. The rotation of a star or planet at different speeds at its equator and poles
White Dwarf
rotation curve=winding dilemma?
differential rotation
Flat - Flat
8. The law stating that hotter blackbodies look bluer than cooler blackbodies.
9. Jupiter
anorthosite
most moons
Io (jupiters moon)
Asymptotic giant Branch Star
10. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Spectroscopic Parallax
Extrasolar Planet
neutrino
mapping the structure of Milky Way disk
11. Elliptical orbits that come inside orbit of the Earth.
Apollo asteroids
Color Index
mare basalt
Plague
12. The imaginary sphere centered on the Earth that hols the stars.
Celestial Sphere
Cassini division
Stephen-Boltzman Law
Prominence
13. What do we think the actual fate of the universe will be and why do we think this?
Black Hole
Negative - Diverge - Less than 1
Continuous Spectrum
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.
14. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
homogeneous
shape and color of SPIRAL galaxies
molecular clouds
density waves
15. Centered on the sun.
gravity
Cepheid variables
Heliocentric
differential rotation
16. The temp at which a substance in the vacuum of space solidifies
Winter Solstice
condensation temperature
Ammonia - methane - and water
Ionization
17. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
How is winding dilemma solved?
density waves
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
Electromagnetic Radiation: Radio
18. The Greek philosopher responsible for making the stellar magnitude scale.
radiation pressure
Ionization
Hipparchus
Coronal Loop
19. Then the Sun moves from north to south across the celestial equator (about September 23)
accretion
Autumnal Equinox
Synchrotron Rotation
Particle Horizon
20. Electromagnetic Radiation
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.
Oort cloud
A family of radiant energy- includes light
fusion crust
21. A star fusing hydrogen to helium in it's core
Make up of the jovian planets
Main Sequence Stars
Cassini division
Flat - Remain Parallel - Exactly 1
22. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
greehouse effects
Dark Matter
most moons
Blackbody Curve
23. Mercury
greatest elongation
smallest diameter
radio galaxy
shape and color of SPIRAL galaxies
24. Titan
Cassini division
MOONS: thickest atmosphere
Stephen-Boltzman Law
Oort Cloud
25. 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.
Steady State Theory (Leads to Olber's Paradox)
Differential Rotation
Ground State
mapping the structure of Milky Way disk
26. 1 mm 1μm
Electromagnetic Radiation: Infrared
Open - flat - and closed.
blazar
Blackbody Curve
27. Large nebula consisting of very cold gas and dust
Stephen-Boltzman Law
zone
Molecular Clouds
Lagrangian Razor
28. A plot of star absolute magnitude verses spectral type.
Lagrangian Razor
protostar
H-are Diagram
Yes - frozen at the poles- remains protected from the suns rays
29. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Zenith
Red Giant Branch Star
The Big Bang Theory resolves Olber's Paradox
Seyfert galaxy
30. A faint - remarkably uniform distribution of radiation in space
Gamma ray bursts
matter dominated universe
Cosmic Microwave Background
CNO Cycle
31. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Sa spiral galaxy
Yes - frozen at the poles- remains protected from the suns rays
meteor shower
Sunspot cycle
32. The apparent path of the Sun through the stars on the celestial sphere.
Flat - Remain Parallel - Exactly 1
Big Bang
Ecliptic
Quasar
33. The light produced when particles from the sun collide with atmospheric molecules
Occam's razor
Parsec
aurora
How is winding dilemma solved?
34. Approximate speed of light in a vacuum
Globular Cluster
Oort Cloud
300000 KM/sec
evidence of water on mars
35. A measure of the force of gravity on an object
mapping the structure of Milky Way disk
great red spot
weight
Interstellar Extinction
36. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
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.
Enke gap
Black Hole
Parsec
37. Mercury and venus
fewest moons
Kuiper belt
anorthosite
Synodic Day
38. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Liquid metallic hydrogen
self-propagating star formation
Focal Plane
quarks
39. The part of the Milky way that has on-going star formation
Disk
nova
Seeing
density waves
40. A bright area of higher temperature that often proceeds the formation of sunspots.
Plague
scarp
acceleration
Stephen-Boltzman Law
41. The mix of pure photon energy that emerged at the start of the universe.
Main Sequence Stars
Perihelion
cosmic fireball
Ganymede (Jupiter)
42. When material is heated and moves taking the heat energy with it
standard candle
Cassini division
Convection
How is winding dilemma solved?
43. A star that erratically and explosively brightens and dims
Nova
resonance
Stephen-Boltzman Law
Seyfert galaxy
44. A collection of galaxies like the one the Milky Way belongs to
Main Sequence
Geocentric
Poor Cluster
Self-Propogating Star Formation
45. Collections of young - hot stars
Gamma-ray Burst
planetesimal
rotation curve=winding dilemma?
OB Associations
46. The Greek philosopher responsible for making the stellar magnitude scale.
Synodic Day
dark energy
Hipparchus
molecular clouds
47. A bridge of material held in position above the solar surface. They can remain for hours even days
Negative - Diverge - Less than 1
Prominence
Sb spiral galaxy
Umbra
48. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
Titus-Bode Law
Rich vs poor clusters
Flare
Molecular Clouds
49. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Black Hole
Limb darkening
Thermal Equilibrium
Open Cluster
50. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Trojan asteroids
Light Gathering Power
Enke gap
Perihelion