Astrophysics

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Last updated 9:57 AM on 6/14/26
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22 Terms

1
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Unit for Gravitational Field Strength

Newton per Kilogram (N/kg)

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Universe

large collection of billions of galaxies

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Galaxy

large collection of billions of stars

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Our Solar System

Milky Way Galaxy

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Explain Variations in Gravitational Field Strength

  • earth's gravitational field strength is different than that on other planets and the moon

  • larger mass → greater gravitational field strength

  • smaller radius → greater gravitational field strength at surface

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Gravitational Force causes:

  • moon to orbit planets

  • planets to orbit the sun

  • artificial satellites to orbit the Earth

  • comets to orbit the Sun

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Differences in Orbits

  • comet: very elliptical

  • planets: elliptical

  • moon: circular

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Orbital Speed Equation

orbital speed = (2 x π x orbital radius)/ time period

v = (2 x π x r)/ T

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Classification of Stars According to Colours

  • star's colour is related to its surface temperature

  • hot stars looks blue, medium stars looks yellow, cooler stars look red.

  • OBAFGKM (hottest to coldest) - Oh Be A Fine Guy, Kiss Me

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Evolution of Stars of Similar Mass to Sun

Nebula → Main Sequence Star → Red Giant → White Dwarf Star

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Process of Evolution of Stars from Nebula to Main Sequence Star

  • nebula is cloud of dust

  • gravity causes cloud to collapse

  • temperature of cloud increases

  • hydrogen atoms in nebula move towards each other due to gravitational force

  • KE store increases, increase temperature

  • nuclear fusion of hydrogen starts

  • becomes main sequence star

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Process of Evolution of Stars from Main Sequence Star to White Dwarf

  • fuses H into He in core

  • outward pressure from fusion balances inward gravitational force — star is stable

  • hydrogen in core runs out

  • core contracts and heats up

  • outer layers expand and cool

  • becomes a red giant

  • helium fuses into heavier elements in core

  • core becomes white dwarf

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Evolution of Stars with Mass Larger than Sun

Main Sequence Star → Red Supergiant → Supernova

Nebula → Neutron Star or Black Hole

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Process of Evolution of Stars with Mass Larger than Sun

  • fusion stops in core of main sequence star

  • core collapses (increases temp in layer surrounding core)

  • restarts fusion in core

  • star contracts, surface temp decreases

  • star becomes red supergiant

  • fusion of heavier elements stops in core

  • star explodes as supernova

  • core collapses to form a neutron star or black hole

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Absolute Magnitude

brightness of star at standard distance

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Hertzsprung-Russel Diagram

A → White Dwarfs

B → Main Sequence

C → Giants

D → Supergiants

<p>A → White Dwarfs</p><p>B → Main Sequence</p><p>C → Giants</p><p>D → Supergiants</p>
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Big Bang Theory

  • expansion (of space)

  • continuing (expansion)

  • from very hot/dense start

  • from a point

  • origin of Universe

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Evidence Supporting Big Bang Theory

  • Red-Shift

  • Cosmic Microwave Background (CMB) Radiation

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Red-Shift of Galaxies

  • change in frequency or wavelength of radiation

  • wavelength increased/ frequency decreased

  • as star moves away (from us)

  • big bang has expanding universe

  • with galaxies moving away (from each other)

  • further the galaxy is (from Earth), the greater the red-shift;

  • larger redshift means faster movement of galaxies

  • the further away, the faster the galaxy moves away

  • galaxies moving apart from each other implies expansion from a single point or since the Big Bang;

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CMB Radiation

  • radiation that comes from all over the sky

  • the Big Bang theory has a initial explosion

  • that releases radiation

  • CMBR appears to be the same in all directions / is everywhere

  • (which) implies all parts of the Universe were in contact a long time ago

  • wavelength has increased (as the universe has expanded);

  • Universe was (significantly) hotter long ago;

  • Doppler Effect

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Relationship between Change in Wavelength and Reference Wavelength

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Red-Shift in Light Received from Galaxies at Different Distances

  • light shifted to red end of specctrum

  • light waves stretched so wavelength increases

  • black lines move to red end