Astronomy and Physics Fundamentals Flashcards

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Comprehensive flashcards based on lecture notes covering the Big Bang Theory, galaxy and star classification, Kepler's and Newton's laws, and astronomical constants and conversions.

Last updated 5:50 PM on 5/16/26
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30 Terms

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Big Bang Theory

A theory that posits the universe originated from a dense, hot state and has expanded over time.

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Evidence for Big Bang Theory

Includes cosmic microwave background radiation, redshift of galaxies, and the abundance of light elements.

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Cosmic microwave background radiation

A remnant thermal radiation from the early universe that provide clues about its origins.

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Spiral galaxy

A galaxy characterized by a flat disk structure with spiral arms, a central bulge, and is rich in gas and dust.

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Elliptical galaxy

A galaxy that lacks a spiral structure and possesses older star populations with less gas and dust.

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Actual size

Refers to the true dimensions of an object.

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Scaled size

A proportional representation of an object's actual dimensions.

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Kepler’s First Law

The law stating that planets move in elliptical orbits around the sun, with the sun at one focus.

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Kepler’s Second Law

The law stating that a line segment joining a planet and the sun sweeps out equal areas during equal intervals of time.

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Kepler’s Third Law

The law stating that the square of a planet's orbital period is proportional to the cube of the semi-major axis of its orbit.

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Newton’s Law of Gravitation

States that every mass attracts every other mass with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.

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Formula for gravitational force

F=GM1M2r2F = G\frac{M_1 M_2}{r^2}

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Gravitational constant (GG)

6.67×1011N(m2/kg2)6.67 \times 10^{-11} \, \text{N(m}^2/\text{kg}^2)

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Star classification by temperature

Classified into types O, B, A, F, G, K, and M.

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Star classification by brightness

Classified as main-sequence, giants, supergiants, and white dwarfs.

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Criteria for galaxy classification

Morphology, size, brightness, color, and spectral properties.

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1 degree in minutes

1degree=60minutes (’)1 \, \text{degree} = 60 \, \text{minutes (')}

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1 degree in seconds

1degree=3600seconds (”)1 \, \text{degree} = 3600 \, \text{seconds ('')}

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Formula for the mass of an orbiting body

M=r3×4π2GT2M = \frac{r^3 \times 4\pi^2}{GT^2}

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Radius of Earth's orbit

1.496×108km1.496 \times 10^8 \, \text{km}

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Formula for energy in terms of frequency

E=hvE = h \cdot v

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Planck’s constant (hh)

6.63×1034J×s6.63 \times 10^{-34} \, \text{J} \times \text{s}

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Speed of light (cc)

3.0×108m/s3.0 \times 10^8 \, \text{m/s}

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Wave relationship formula

c=λvc = \lambda \cdot v where λ\lambda is the wavelength and vv is the frequency.

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Light-year

1light-year=9.48×1012km1 \, \text{light-year} = 9.48 \times 10^{12} \, \text{km}

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Angstroms to meters conversion

1A˚=1010m1 \, \text{Å} = 10^{-10} \, \text{m}

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Nanometers to meters conversion

1nm=109m1 \, \text{nm} = 10^{-9} \, \text{m}

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Inches to centimeters conversion

1inch=2.54cm1 \, \text{inch} = 2.54 \, \text{cm}

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Miles to kilometers conversion

1mile=1.609km1 \, \text{mile} = 1.609 \, \text{km}

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Miles to feet conversion

1mile=5280feet1 \, \text{mile} = 5280 \, \text{feet}