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UMD ASTR101 Final Exam Review/UMD ASTR101 Final Exam Review

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UMD ASTR101 Final Exam Review/UMD ASTR101 Final Exam Review

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ASTRO 101 Final Exam Review
Extraterrestrial Life
 life on earth centers itself around carbon
o Crucial:
 held together by strong nuclear force
 most common form is a chain
 it can form chains with other elements
 carbon-carbon chain has a strong backbone
 very large and stable
 DNA contains billion of atoms, yet the arrangement holds 4
o Silicon is a dead end bc it is too simple
 Meteorites contain amino acids strings of carbon atoms with nitrogen, oxygen,
hydrogen
 Terrestrial Life:
o We define terrestrial life as series of processes by which material are
taken in and used for metabolism, respiration, and reproduction with the
possibility of change - the potential for mutations to occur.
o large molecules and complex chemistry
o life on earth originated in water
 water provides protection from UV light
 oldest fossils were aquatic life forms (3.5 billion years)
 Requirements for Habitability:
o A source of nutrients from which to build cells0
o Energy to fuel activities: sunlight, chem reactions, heat from Earth
o Liquid Water: transports nutrients into cells, waste out
Habitable zone - the orbital region around a star in which an Earth-like planet can
possess liquid water on its surface and possibly support life. Liquid water is essential to
all life on Earth
 Miller-Urey Experiment: found that Earth’s “primitive” atmosphere did NOT
contain O2
 Black Smoker: geothermal vent seen on ocean floor
o microbes that are found in these mineral enriched environments are
ancient on the evolutionary scale
o **Could be similar on Europa**

Early Models for the Arrangement of Stars
 Herschel’s Model:
o Milky Way galaxy is disk shaped (CORRECT)
o Our Sun is at the center of the galaxy (INCORRECT)
 Shapley’s Model: observed globular star clusters
o we are not at the center of the galaxy bc he viewed globular clusters!!
 if we were at the center of the galaxy, we would see the same
number of stars in all directions
o came after stellar parallax

,Milky Way Galaxy
 Structure: Spiral galaxy
o spiral arms blend into a thin disk that contains more than 100 billion stars
o center of the disk; find a bright central bulge, supermassive black hole
o surrounding the disk is a vast, spherical halo, which contains globular star
clusters
o disk=100,000 LY in diameter
o sun=28,000 LY from center
 Galactic disk is filled with interstellar gas and dust→ known as the interstellar
medium
o obscures our view when we try to peer directly in it
 21 CM RADIATION: when the hydrogen atoms in hydrogen gas have a slight
change in energy, they emit a wavelength of radio energy. The wavelength they
emit is 21.1 cm. The slight change in the energy in a hydrogen atom occurs
when the electron moving around the proton flips from a parallel spin to an anti-
parallel spin in order to be in a lower energy state. Remember that all atoms
prefer to be in the lowest energy state as possible. hyperfine transition**
o If proton and electron are spinning the same direction, they’re in a spins
aligned state
 slightly greater energy
o If protons and electrons are spinning in opposite directions, they’re in a
spins opposite state
 slightly less energy
o When it changes from spins aligned to spins opposite, it is called a
hyperfine transition
 hyperfine transitions release low energy, long wavelength photon!
 21cm = radio photon
o 21cm radiation is used by astronomers to see further into the Universe
 The interstellar medium (gas and dust) does not block 21cm
radiation (RADIO WAVES!!!)
 Center of our galaxy:
o infrared image of galactic center: we find a lot of red giants
o The galactic center is a turbulent place
 gas flung outward from the galaxy’s center about 10 million years
ago (from doppler shift)
 Synchrotron emission (electrons and strong mag field)
 There are 4 million solar masses within 10AU from each other…
 ***Supermassive black hole***


Mysterious Spiral Nebulae
 Messier catalogued nebulae so that he wouldn’t confuse them with comets
o star forming regions
o planetary nebulae = dying stars
o star clusters

, o spirals
 Herschel and Lord Rosse made detailed sketches of spirals

Cepheid Variable Stars change in Brightness Regularly
 not eclipses - variable stage of stars’ evolution
 Henrietta Leavitt identified cepheid variables in the Magellanic Clouds
 brightest ones had the longest periods of variation
 if all are at the same approx distance, the brightest ones must be more luminous

Edwin Hubble used Mt. Wilson 100’’ Telescope
 Hubble saw Cepheid variables in the Andromeda spiral nebula
 Plotted light curves - found periods
 Used the P/L relation to estimate distance
 2.5 million LY away, so this is distance to Andromeda spiral
Hubble’s contributions:
 Discovered that Andromeda spiral nebula is a galaxy
o used cepheid variables to determine distance
o 2 million LY beyond Milky Way’s boundaries
 Developed the classification system for galaxies
o based on visual appearance
o spirals, ellipticals, irregulars
o observed spectra of galaxies
 Redshift/Distance Correlation:
o angular size of a galaxy decreases with increasing red-shift
 Hubble’s Law: V = H x d
o V = velocity of recession measured from redshift, spectrum
o H = Hubble’s constant, 20-40 km/sec/MLY
o d = distance in MLY (10^6 LY)
o Law explained:
 most distant galaxies have greatest redshifts
 these galaxies are moving away at huge velocities
 explained as the “expansion of space”
 galaxies at greater distance have more of this expanding space
between us and them
 produces greater redshift
 ***Observational basis for space expansion model***

Types of Galaxies
 Elliptical: round to oval subclasses
 Spiral: bright centers w/ thin disk made by visible spiral arms or dust
o Barred Spirals: visible extension across center
 Irregular: some appear distributed
 Orbits of Disk Stars
o stars in the disk orbit in a circular path
o arises from its gravitational attraction toward the galactic center; bobbing
arises from localized pull of gravity within the disk

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