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Least massive atomic particle
electron
least massive atom
Hydrogen
measured the speed of light using lanterns atop hills
Galileo
Ole Romer accurate meaurment of the speed of light 1676
used the delay in eclipses of jupiter's moon when the earth is on the opposite side of the sun as jupiter
most energetic light photons
The most energetic light photons is blue visible light
number of wave repetitions passing an observer each second is defined as
Frequency in hertz
energy is released in the form of light when electrons
move from higher orbital energy levels to lower energy levels
Radiation with the shortest wave length
Gamma rays
An ion is....
a charged particle, more electrons than protons or vis a versa
the spectrum of a star can reveal
its chemical composition its surface temp whether or not it is moving away from us how fast it is moving either away or towards us
compared to visible light radio waves have
lower energy and longer wavelength
the doppler effect detects the speed of a star by
measuring the shift in wavelength of a particular spectral line
a sound passing by a source at a constant speed does.... (firetruck)
has a higher pitch when a approaching and a lower pitch as it recedes
different elements have unique spectral lines because
each element has a unique set of electron orbits due to the unique number of protons attracting the electrons
if a hot object is partially blocked by a could of cold gas then we will see
absorption lines
what is the resolving power of a telescope
the ability to distinguish objects close together in the sky
500 light years= how many real years
500
2 stars have equal luminosity one is twice as far away as the other how much brighter/ dimmer is the further one
1/4 as bright as the closer one
if one star is 10 time further away, how much more luminosity must the further one have for them to appear equally as bright to an observer on the earth
100 times brighter
two stars have equal luminosity one is twice as far away as the other, how much brighter/dimmer does the further one appear than the closer one
the further one is 1/4 as bright as the closer
refracting telescopes are not commonly employed because
chromatic aberration large lenses causing sagging in the middle large lenses cause the telescope to be difficult to maneuver
a telescopes spatial resolution is determined by
the objective diameter
Telescope A has a 4 inch objective diameter, telescope B has an 8 inch objective diameter how much more powerful is telescope B?
4 times
professional astronomers use large telescopes because
to gather more light
Intergalactic UV light must be observed with telescopes in space because
UV light is absorbed by the o-zone and does not penetrate to the ground
atmospheric blurring (aka "seeing") effects the quality of an image. Poor seeing makes a telescopes resolution....
worse
large telescopes are typically placed on high mountains/in space because...
the attempt to eliminate atmospheric blurring and to improve seeing.
Why is there no atmosphere on the moon?
Because its low mass is not enough to hang on to its atmosphere at its temperature.
Lunar Rotation
rotates on its axis with the same period as its revolution about the earth
during a single night the moon moves
East to West across the sky
Trans neptunian object
Any object too small to be classified as a planet that orbits the sun at a greater average distance than Neptune.
Asteroid
Rocky bodies smaller than a planet often found between the orbits of Mars and jupiter.
Venus
Planet that can be in the Easter sky at sunrise
Composition of Jupiter
the composition of Jupiter is closest to the composition of the sun
Planets that cant be seen at Opposition
Planets that have a smaller radius than the earth cannot be seen at opposition
Energy produced by the sun
Comes from nuclear fusion, similar to energy produced in a hydrogen bomb
The suns position within the milky way
The sun is located in the disk, slightly more then halfway out from the center
Approximate number of stars in the MIlky Way galaxy
100,000,000,000 one hundred billion
Absorption Nebulae
should appear redder than Reflection nebulae
Extinction
known as the dimming of distant objects in the plane of the milky way
Immanuel Kent
Philosopher of the 18th century who proposed that the milky way was a flattened disk of stars and that spiral nebulae were "island universes" similar to the milky way
Thomas Wright
pictured the milky way as a spherical shell of stars
Herschel
Discovered Uranus
Bessel's first measurement of parallax importance
important for many reasons and connects back to the ancient renaissance astronomers because measurement of parallax is one proof that the earth moves about the sun that was not measurable previously.
Jacobus Kapteyn
the first to use star counts to develop a detailed model with the sun at the center of a disk-like distribution of stars.
Harlow Shapley
Used the positions of globular clusters to deduce that the sun does not lie near the center of the milky way galaxy
Herber Curtis
he was a former director of the Allegheny Observatory
Harlow Shapley Great Debate point
argued that the spiral nebulae usually appear bluer in color than the milky way does
Heber Curtis Great debate point
Argued that bright novae are often seen in andromeda, so there must be many stars in Andromeda
Henrietta Leavitt
showed that cepheid variable stars follow a distinct relationship between dimming and brightening period and peak luminosity.
Edwin Hubble
Resolved the Great Debate by measuring the distances to external galaxies and resolving individual stars in the andromeda galaxy
Age of the universe
14 billion years.
A spiral galaxy
shows substantial rotation, interstellar gas, and interstellar dust
Vesto Slipher
Measured the spectra of external galaxies noting that they were nearly always redshifted
Luminosity
an effective way to estimate the distances to other galaxies
Einstein's theory or relativity
a theory that has been tested experimentally
Sir Arthur Eddington
organized expeditions to verify the gravitational lensing prediction of general relativity by observing stars near the sun during an eclipse
According to special relativity
Time and space are inseparably linked and observers have a perspective on spacetime that is determined by their state of relative motion

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