Stellar Evolution. Solar Composition Most stars in space have this composition: 74% hydrogen, 26%...
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Transcript of Stellar Evolution. Solar Composition Most stars in space have this composition: 74% hydrogen, 26%...
Stellar Evolution
Solar CompositionSolar CompositionMost stars in space have this composition:74% hydrogen, 26% heliumFusion is the energy maker of the sun
Star FormationStar FormationAll stars begin as a stellar/solar nebula (cloud of
gas and Dust) it is theorized the gas and dust formed as a result of another star’s collapse.
A Protostar (new star) is formed from a nebula
that collapses due to the force of gravity. After
the nebula collapses fusion reactions begin and a
new star is formed
The life cycle of this star has already been determined due to the amount of mass it began with.
Star Life Cycle: You need to memorize!
DRAW & LABEL
Life Cycle of a StarLife Cycle of a Star Protostar turns into a medium size star Medium sized star becomes a red giant with all of its
matter squeezed together.
It could do two things depending on its original mass Red Giant with low mass becomes a white dwarf (shines
with a white hot light) it then becomes a black dwarf (dead star)
OR If the Red Giant was very massive it can become a
supernova and blow up, its core can become a neutron star (gives off pulses of energy) or a Black hole
Black HolesBlack Holes Begin as stars with mass 10x greater than our sun and have
a short life span due to this mass After the supernova explosion the core that remains is so
massive that (without fusion to support it) the core is swallowed by its own gravity.. It literally gets sucked inward on itself.
Not even light can escape it, it swallows energy and matter like a vacuum cleaner
Most are found due to their companion star, gases from the companion are pulled into the black hole and they give off a burst of x-rays before the matter falls into the black hole.
There are new theories on black holes: hole to new universe, they form new stars, different dimension…
Hertzsprung-Russell diagramHertzsprung-Russell diagramDon’t copy any of this… watch the video for an explanationhttps://www.youtube.com/watch?v=UIoA1P30HrM
The properties of mass, luminosity, temperature, color and diameter are closely related
Each star has specific characteristics related to each of the properties
90% of all stars fall along main sequence
Basic Properties of StarsBasic Properties of Stars
1. Apparent Magnitude: Brightness as it appears on Earth
2. Absolute Magnitude: Amount of light a star actually gives off
3. Luminosity: is the actual energy output on the surface of a star per second, measured in watts
Positions and Distances of StarsPositions and Distances of Stars
Distance is measured in light years (distance light travels in 1 year = 6 trillion miles)
To account for the motion of the Earth when viewing the stars, the apparent shift in position of the star is called parallax
TelescopesTelescopes Refracting: first type, lenses brought visible light top a focus Reflecting: mirrors bring visible light to a focus
All telescope goals are to bring radiation (wavelengths human eye can not detect) to a focus
There are x-ray, infrared, ultraviolet, and gamma ray telescopes that only detect those parts of the electromagnetic spectrum
Interferometry: process of linking separate telescopes together so they act as one. Very detailed!
Space based telescopes: Hubble, Ultraviolet Spectroscopic Explorer, Chandra X-Ray Observatory, Compton Gamma Ray Observatory
Spectra: Draw a picture of each Spectrum: Visible light arranged according to wavelength. Used
to find out the elements stars are composed of.
Continuous: can be caused by a glowing gas or liquid, color band lengths indicate amountof element present
Emission: bright lines at certain wavelengths indicate the element present
Absorption: caused by different chemical elements being absorbed, dark lines indicate element present
Groups of StarsGroups of Stars There are 88 constellations that were named by ancient
people They appear to move around the poles They can be seen only during certain times of the year. They are not gravitationally bound together
BinariesBinaries Two stars that are gravitationally bound together Orbit a common center of mass Most appear as a single star
Novas Nova is a star that increases in brightness in a few hours