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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 what chemical form are jupiters nitrogen - carbon and oxygen?
Spectroscopy
Thickest atmosphere
Blackbody Curve
Ammonia - methane - and water
2. When the Sun is farthest north of the celestial equator (about June 22)
molecular clouds
Summer Solstice
Coldest surface
Corona
3. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
Inverse Square Law
mass
greehouse effects
Titus-Bode Law
4. Mercury
Thickest atmosphere
Disk
disk
smallest diameter
5. 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
Kuiper belt
Eyepiece Lens
Ecliptic
Spectroscopic parallax
6. A very dense - highly populated cluster of galaxies
tectonics of Mars
Rich Cluster
Absolute Magnitude
planetary nebula
7. Centered on the sun.
Black Hole
Gamma ray bursts
Heliocentric
Big Crunch
8. Earth
Most dense
plate tectonics
Globular Cluster
planetary nebula
9. A star that is in the process of forming. It glows from gravitational contraction
Light: travels like a wave - detected like a particle
Parallax
protostar
Photosphere
10. A measure of the ability of a telescope to see fine detail
neutrino
Spectroscopy
Resolving Power
cosmological principle
11. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
Jupiters red spot
planetesimal
Sc spiral galaxy
Atomic Number
12. 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.
Hubble constant
Heliocentric
nova
slowest rotation
13. The average distance between the Earth and the Sun (=1.5 x10^8km)
nova
coma
cosmological principle
Astronomical Unit
14. The area behind a lens where images are resolved
Limb darkening
greatest elongation
Seyfert galaxy
Focal Plane
15. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
Hydrostatic Equilibrium
Red Giant Branch Star
Photon
Yes - frozen at the poles- remains protected from the suns rays
16. The oldest grouping of stars - found in the galaxy halo
Jovian Planets
Globular Cluster
cosmological principle
Plague
17. An energetic event taking place in the early universe
Convection
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
Gamma-ray Burst
Eyepiece Lens
18. Light scattered through the atmosphere that degrades astronomical images
Light Pollution
Gamma-ray Burst
coma
Jupiters red spot
19. The apparent backward motion of a planet against the background of stars.
Cassegrain Focus
retrograde motion
Dark Nebula
Annular Eclipse
20. A method of finding a star's distance from its absolute magnitude and spectral type or color.
High Velocity Stars
Nova
Spectroscopic Parallax
neutrino
21. The amount an image is enlarged by a telescope
blazar
Magnification
Main Sequence
Ole Roemer
22. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
mare basalt
Europa (Jupiters moon)
meteorite
Corona
23. The rock that makes up the lunar maria
Galilean satellite
mare basalt
SETI
Nebula
24. A star without enough mass to begin hydrogen fusion
Brown dwarf
Apparent Magnitude
Flat - Flat
deferent
25. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Heliocentric
Eclipses of the Moons of Jupiter
Electron
Big Crunch
26. A high-pressure bulge in Neptune's southern hemisphere
synchronous rotation
Yes - frozen at the poles- remains protected from the suns rays
Spectroscopy
great dark spots
27. Half of the longest diameter across an ellipse
Brown dwarf
semimajor axis
plate tectonics
Dark Matter
28. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
reflection star clusters
force
If it is in a denser medium - such as glass - it will move slower
Thermonuclear Fusion
29. Matter that reveals itself only through its gravitational attraction.
Active Optics
Electromagnetic Radiation: Microwave
dark matter
Pixel
30. A term referring to the orbital character of stars near the Sun
Ganymede (Jupiter)
Focal Plane
HII Region
Differential Rotation
31. Ganymede
differential rotation
thinnest atmosphere
gravity
MOONS: largest size
32. Approximate speed of light in a vacuum
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.
most eccentric orbit
300000 KM/sec
great red spot
33. A perfect absorber and radiator of electromagnetic radiation.
Blackbody
Roundest orbit
Ammonia - methane - and water
superclusters
34. The point in its orbit where a planet is nearest the sun
density waves
Perihelion
rotation curve = dark matter?
Thermal Equilibrium
35. Light scattered through the atmosphere that degrades astronomical images
Light Pollution
Main Sequence
Oort cloud
Neutron Star
36. 1 mm 1μm
isotropic
High Velocity Stars
Electromagnetic Radiation: Infrared
rotation curve=winding dilemma?
37. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
radiant
coma
Atomic Number
Dark Nebula
38. The process similar to conduction by which energy moves from the solar core to the convective layer
Ganymede (Jupiter)
Radiative Diffusion
Poor Cluster
Gamma ray bursts
39. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
Supercluster
CCD
Eclipses of the Moons of Jupiter
Convection
40. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Radio Galaxy
greatest elongation
quasar
meteoriod
41. The lens that gathers the light in a refractor
Celestial Sphere
standard candle
Objective Lens
Perihelion
42. Is there water on the moon?
synchrotron radiation
Energy Level
Yes - frozen at the poles- remains protected from the suns rays
Liquid metallic hydrogen
43. Large nebula consisting of very cold gas and dust
disk
Molecular Clouds
most moons
critical density
44. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
epicycle
matter dominated universe
tectonics of Venus
widmanstatten pattern
45. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
cosmological principle
Coronal Loop
shape and color of SPIRAL galaxies
radio galaxy
46. The act of removing an electron from an atom.
Ionization
chondrite
Brown dwarf
protostar
47. A younger cluster of stars - found in the galaxy disk
Open Cluster
Differential Rotation
rotation curve=winding dilemma?
Energy Level
48. Infinitely long -> 10 cm
Cepheid variables
Electromagnetic Radiation: Radio
Planetary Nebula
Photon
49. Poitns of gravitational stability in the orbit of a planet
Parallax
Kuiper belt
Yes - frozen at the poles- remains protected from the suns rays
Lagrangian Razor
50. Large nebula consisting of very cold gas and dust
condensation temperature
Interstellar Extinction
Molecular Clouds
H-are Diagram