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What are the three main components of the universe?
What were the three major components of the solar nebula?
What are the three components to form a galaxy?
What percentage of the total mass-energy density does normal matter account for?
What is the purely observational evidence used to infer the existence of Dark Matter?
Approximately what proportion of the universe's total mass-energy budget is attributed to Dark Energy?
What cosmological function is attributed to Dark Energy in contrast to Dark Matter?
What particles constitute normal matter, often referred to scientifically as baryonic matter?
What role does Dark Matter play in the formation and maintenance of cosmic structures?
Which large-scale mapping technique helps refine models of structure formation related to Dark Matter?
What is the standard cosmological model that incorporates Normal Matter, Dark Matter, and Dark Energy called?
What two opposing forces determine the ultimate fate and destiny of the universe?
Why is Dark Matter completely invisible to conventional telescopes despite its abundance?
What percentage of the solar nebula's total mass was composed of primordial hydrogen ($ ext{H}$) and helium ($ ext{He}$)?
What characteristic defines refractory solids like rock and metal?
What materials condensed exclusively in the hot inner portion of the protoplanetary disk?
Where is the frost line generally located in relation to the orbits of modern planets?
Which group of compounds is classified as volatile ices in the solar nebula context?
What was the definitive sorting mechanism that separated the three primary material classes in the nebula?
What provided the necessary mass boost for the cores of Jupiter and Saturn to rapidly accrete hydrogen and helium gas?
How were the hydrogen compounds necessary for Earth's oceans and early atmosphere primarily delivered?
What fate befell Uranus and Neptune compared to Jupiter and Saturn regarding gas accretion?
Relative to the gas content, how is the material composition of the inner solar system described?
What are the three primary, massive structural components used to define a galaxy's appearance and dynamics?
Which structural component of a galaxy is primarily characterized by ongoing star formation and the presence of significant cold gas and dust?
How is the motion of stars within the central bulge typically described, contrasting with the orderly rotation seen in the disk?
What substance almost entirely constitutes the Dark Matter Halo, preventing it from interacting with the electromagnetic force?
Which component accounts for the vast majority (often 80% to 90% or more) of a galaxy's total gravitational influence?
Relative to the stars in the galactic disk, what is generally true about the age of the stellar population found in the central bulge?
By what means is the existence and extent of the Dark Matter Halo primarily inferred by astronomers?
What dictates the orbital speed of stars within the galactic disk as they circle the center?
In the analogy comparing galaxy components to layers of an archaeological dig, which structure represents the deepest, oldest layer?
What is a likely structural consequence observed in a galaxy that has experienced a major merger event involving two spirals?