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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 lens in a telescope used to determine the magnification
quasar
Steady State Theory (Leads to Olber's Paradox)
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
Eyepiece Lens
2. An entity that is likely in the nucleus of most - if not all - galaxies.
Light Gathering Power
Emission Spectrum
supermassive black hole
Zenith
3. Then the Sun moves from north to south across the celestial equator (about September 23)
Thermonuclear Fusion
OB Associations
Autumnal Equinox
Filament
4. The normal eastward movement of a planet against the background of hte distant stars.
Density Wave
anorthosite
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
direct motion
5. A faint - remarkably uniform distribution of radiation in space
Cosmic Microwave Background
3 reasons we orbit satellites to observe universe
Cassini division
Trojan asteroids
6. An empirical scheme for predictin ghe orbital distances of planets
evidence of water on mars
Ground State
Titus-Bode Law
differential rotation
7. The 'edge' of the universe. Light beyond this has not reached us yet.
Olber's paradox
partile horizon
Galilean satellite
Globular Cluster
8. 1 mm 1μm
Trojan asteroids
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.
Kuiper belt
Electromagnetic Radiation: Infrared
9. The point in its orbit where a planet is farthest from the sun
aphelion
Dwarf planets
direct motion
Radiative Diffusion
10. When massive objects bend space and time enough to create multiple images of an object located behind them
Photometry
The Big Bang Theory
Yes - frozen at the poles- remains protected from the suns rays
Gravitational Lens
11. 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)
planetary nebula
Hubble law
meteoriod
Cosmological Principle
12. A planet that is farther from the sun than the Earth is
Make up of the terrestrial planets
Superior planets
Gamma ray bursts
Maria
13. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
rotation curve=winding dilemma?
Jupiters red spot
Electromagnetic Radiation: Infrared
synchrotron radiation
14. A large and bright but cool star.
Red Giant
Titus-Bode Law
difference between maria and highlands of the moon.
Electromagnetic Radiation: Radio
15. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Grand design spirals
retrograde motion
Callisto (Jupiter)
Thickest atmosphere
16. The rock that makes up the lunar highlands
anorthosite
Ecliptic
Nebula
Jovian Planets
17. 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.
mapping the structure of Milky Way disk
Cepheid Variable
White Dwarf
Supernova (You can be my supernova girl)
18. 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.
Eyepiece Lens
Zenith
Population 1 vs Population 2 stars
Instability strip
19. Venus (retrograde)
meteorite
Zenith
slowest rotation
radiation pressure
20. The act of removing an electron from an atom.
molecular clouds
Electromagnetic Radiation: X-Ray
Ionization
Meridian
21. The process that powers the sun and hydrogen bombs
anorthosite
Thermonuclear Fusion
Grand design spirals
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.
22. 10^2 nm 10^7 nm
Electromagnetic Radiation: Gamma Ray
fastest rotation
radiation dominated universe
Supernova (You can be my supernova girl)
23. The area behind a lens where images are resolved
Focal Plane
Flat - Flat
open star clusters
most eccentric orbit
24. The fusion process that turns three helium nuclei into a carbon nucleus
fewest moons
cosmic fireball
Triple Alpha rocess
protostar
25. Any change in the speed or direction of an object's motion
Pixel
solar nebula
Jovian Planets
acceleration
26. Originially thought to be stars emitting radio radiation but are now concluded to be nuclei of distant galaxies (same as radio galaxies aka emit streams of material)
White Dwarf
greatest elongation
Emission Spectrum
quasar
27. An object that may remain after a star explodes
meteor
coma
Neutron Star
Pixel
28. The relation that tells how light dims with distance.
nucleus
Inverse Square Law
Electromagnetic Radiation
E=mc2
29. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
rotation curve = dark matter?
density waves
Quasar
Emission Spectrum
30. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
density waves
highlands
Gamma ray bursts
Callisto (Jupiter)
31. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
bulge
How is winding dilemma solved?
Particle Horizon
Spectroscopic parallax
32. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
Astronomical Unit
cosmological principle
acceleration
radio galaxy
33. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
conjunction
3 reasons we orbit satellites to observe universe
interstellar dust
Kirkwood gaps
34. Venus
Flat - Remain Parallel - Exactly 1
Roundest orbit
AGN
Light Gathering Power
35. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
CMB
Eyepiece Lens
Molecular Clouds
nova
36. When the Sun is farthest south of the celestial equator (About December 22)
partile horizon
Eyepiece Lens
Io (jupiters moon)
Winter Solstice
37. The point in its orbit where a planet is farthest from the sun
Plague
Photometry
aphelion
Absorption Spectrum
38. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Synchrotron Rotation
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Seyfert galaxy
slowest rotation
39. A location on an H-are Diagram where evolving stars pulsate
Instability strip
Thermal Equilibrium
Heliocentric
terrestrial planet
40. What Ole Roemer used to measure the speed of light in a vacuum
Radiative Diffusion
Eclipses of the Moons of Jupiter
coma
condensation temperature
41. The equation that describes how matter equates with energy
E=mc2
Horizontal Branch Star
Electromagnetic Radiation: X-Ray
bulge
42. The oldest grouping of stars - found in the galaxy halo
Light Gathering Power
Dark Nebula
Eyepiece Lens
Globular Cluster
43. The 'edge' of the universe. Light beyond this has not reached us yet.
Seyfert galaxy
partile horizon
Oort Cloud
Autumnal Equinox
44. A push or a pull
Spectroscopic Parallax
Electromagnetic Radiation: Ultraviolet Light
Sunspots
force
45. The dark - relativley smooth areas on the moon; Latin for sea
Maria
Radio Galaxy
Coldest surface
Sa spiral galaxy
46. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Ole Roemer
Zenith
interstellar dust
cosmic fireball
47. What causes the zones and belts on jupiter and saturn?
Penumbra
High Velocity Stars
conjunction
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
48. The seasonal shifting of a nearby star's position relative to more distant objects.
Rich vs poor clusters
Photosphere
Parallax
meteorite
49. An element of a highly efficient - two-dimensional electronic light detector
Pixel
epicycle
mapping the structure of Milky Way disk
Dwarf planets
50. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
The Big Bang Theory
anorthosite
synchrotron radiation
great dark spots