a. Jets of gas
Event horizon
Accretion disk
b. they are related because a black hole exceeds the speed of light so everything around it, including light, is sucked in.
c. we really don't see the black hole, what we see is the matter being sucked into it.
d. a characteristic radius associated with all masses.
Friday, October 10, 2008
Wednesday, October 1, 2008
sun spots
Sunspots can be as large as 50,000 miles in diameter.
They were first recorded around 28BC in ancient China.
Sunspot's magnetic field is about 2,500 times stronger than earth's.
They occur in pairs with magnetic fields pointing in opposite directions.
Sunspots are about the same size as Earth.
Sunspots are dark because they are much cooler than the rest of the sun.
Sunspots cause the northern lights.
Sunspots cause solar flares.
Sunspots are plotted on a butterfly diagram.
Sunspots can last from days to weeks.
Sunspots don't only form on our sun.
The Maunder Minimum of the late 17th century caused a little ice age.
The safest way to view sunspots is by way of projection.
Royal Observatory of Belgium and the National Oceanic and Atmospheric Administration keeps track of sunspots.
Two official numbers of sunspots are recorded because of the two places they are recorded.
Spectroscopes and spectrohelioscopes are used to observe sunspots.
Land based solar telescopes and satellites observe sunspots.
Sunspots can be seen with the naked eye. (but it's not safe!!)
Sunspots can be seen with a basic telescope.
It is believed that the ancient Greeks understood that sunspots existed, but not what they were.
Johann Goldsmid, Galileo Galilei, Christopher Schiener, and Thomas Herriot are all accredited for finding sunspots.
They were first recorded around 28BC in ancient China.
Sunspot's magnetic field is about 2,500 times stronger than earth's.
They occur in pairs with magnetic fields pointing in opposite directions.
Sunspots are about the same size as Earth.
Sunspots are dark because they are much cooler than the rest of the sun.
Sunspots cause the northern lights.
Sunspots cause solar flares.
Sunspots are plotted on a butterfly diagram.
Sunspots can last from days to weeks.
Sunspots don't only form on our sun.
The Maunder Minimum of the late 17th century caused a little ice age.
The safest way to view sunspots is by way of projection.
Royal Observatory of Belgium and the National Oceanic and Atmospheric Administration keeps track of sunspots.
Two official numbers of sunspots are recorded because of the two places they are recorded.
Spectroscopes and spectrohelioscopes are used to observe sunspots.
Land based solar telescopes and satellites observe sunspots.
Sunspots can be seen with the naked eye. (but it's not safe!!)
Sunspots can be seen with a basic telescope.
It is believed that the ancient Greeks understood that sunspots existed, but not what they were.
Johann Goldsmid, Galileo Galilei, Christopher Schiener, and Thomas Herriot are all accredited for finding sunspots.
Thursday, September 25, 2008
The Very Large Array
c) how old the light coming into the telescope is, in light years or light minutes
a) The Very Large Array can detect all forms of light.
b)
c)
d) it uses 27 antennas that admit radio waves
a) The Very Large Array can detect all forms of light.
b)
c)
d) it uses 27 antennas that admit radio waves
Friday, September 19, 2008
Part A-
5: interactions- 36
10: interactions- 66
15: interactions- 272
20: interactions- 276
25: interactions- 346
as the number increases the interactions increase as well, the relationship is exponential because of the leaps in the numbers.
Part B-
5: interactions- 25
10: interactions- 113
15: interactions- 203
20: interactions- 403
25: interactions- 620
the numbers are more linear. They are more accurate because there are more test subjects.
Part C-
1.5ev- 828nm- sent-15 detected- 12
1.8ev- 690nm- sent-15 detected- 12
2.0ev- 621nm- sent-15 detected- 14
2.3ev- 540nm- sent-15 detected- 12
2.5ev- 297nm- sent-15 detected- 13
It's wavelength goes down and the number detected stays almost the same
Part D-
2.2eV- 565nm- H- sent- 15 detected- 8
2.2eV- 565nm- O- sent- 15 detected- 13
2.2eV- 565nm- Mg- sent- 15 detected- 11
2.2eV- 565nm- Na- sent- 15 detected- 11
2.2eV- 565nm- Ca- sent- 15 detected- 10
With all of the gases it stays about the same but with O there is a higher amount detected and with H there is fewer. I don't think you will get the same patterens because the numbers seem to vary a lot.
5: interactions- 36
10: interactions- 66
15: interactions- 272
20: interactions- 276
25: interactions- 346
as the number increases the interactions increase as well, the relationship is exponential because of the leaps in the numbers.
Part B-
5: interactions- 25
10: interactions- 113
15: interactions- 203
20: interactions- 403
25: interactions- 620
the numbers are more linear. They are more accurate because there are more test subjects.
Part C-
1.5ev- 828nm- sent-15 detected- 12
1.8ev- 690nm- sent-15 detected- 12
2.0ev- 621nm- sent-15 detected- 14
2.3ev- 540nm- sent-15 detected- 12
2.5ev- 297nm- sent-15 detected- 13
It's wavelength goes down and the number detected stays almost the same
Part D-
2.2eV- 565nm- H- sent- 15 detected- 8
2.2eV- 565nm- O- sent- 15 detected- 13
2.2eV- 565nm- Mg- sent- 15 detected- 11
2.2eV- 565nm- Na- sent- 15 detected- 11
2.2eV- 565nm- Ca- sent- 15 detected- 10
With all of the gases it stays about the same but with O there is a higher amount detected and with H there is fewer. I don't think you will get the same patterens because the numbers seem to vary a lot.
Notes on Stellar Spectra
1.Absorption spectra
2. closer, because the distance they are from us make them seem to move more than the further ones
3. brightness
4. the middle radiates to the rest of the star
5. intensity is how bright it looks
magnitude is how bright it really is
2. closer, because the distance they are from us make them seem to move more than the further ones
3. brightness
4. the middle radiates to the rest of the star
5. intensity is how bright it looks
magnitude is how bright it really is
annie cannon
one task would like to spend my whole life doing is working with people. I just want to make a difference in at least one person's life. at this moment i really don't know what i want to do with my life.
Wednesday, September 17, 2008
speed of light
Distance between the hot spots 10cm
Wavelength 20cm
Wavelength .2m
Frequency of the microwave 2500000000m
EQUATION c=λ*f .2*2500000000=c
Your calculated speed of light 500,000,000m/s
Wavelength 20cm
Wavelength .2m
Frequency of the microwave 2500000000m
EQUATION c=λ*f .2*2500000000=c
Your calculated speed of light 500,000,000m/s
Thursday, September 11, 2008
Electromagnetic Radiation
With out a cell phone, something that uses electromagnetic radiation, my life would be very different. not only would I not be able to call my friends (or my mom when I needed a ride) I would also be unorganized because I wouldn't have the calender in it (which i use a lot). Telling time would also be a hassle because I don't own a watch, and my phone has a built in clock =3.
Wednesday, September 10, 2008
Blog 3
a. That the rotation is fairly quick
b. It lost energy between going to mars and coming back
c. The five slices are from five different points of mars that the wave hit.
b. It lost energy between going to mars and coming back
c. The five slices are from five different points of mars that the wave hit.
Tuesday, September 9, 2008
Tunguska explosion
I think the Tunguska explosion was caused by some sort of nuclear blast. Some reasons for this are:
- No meteorite was found (perhaps it exploded into untraceable pieces)
- The trees have a similar blast pattern as Hiroshima
- There were some mutation in people and animals
- There is radiation damage in the area
- No meteorite was found (perhaps it exploded into untraceable pieces)
- The trees have a similar blast pattern as Hiroshima
- There were some mutation in people and animals
- There is radiation damage in the area
Wednesday, September 3, 2008
scaling solar system
1. earth would be located 0.967 meters away
mercury would be 0.374 meters away
that's how far the planets are if Pluto was 175 miles away from the sun
2. .72 years old
the planets have diffrent orbit speeds
3. 75.6
JUPITER
if you are too heavy you will get squished because the gravity pushing on you will be too much
mercury would be 0.374 meters away
that's how far the planets are if Pluto was 175 miles away from the sun
2. .72 years old
the planets have diffrent orbit speeds
3. 75.6
JUPITER
if you are too heavy you will get squished because the gravity pushing on you will be too much
Tuesday, September 2, 2008
Sunday, August 31, 2008
stars in the night sky
Constellation Name # of Stars I Saw
1. Ursa major- 7
2. Ursa minor- 14
3. Cassiopeia- 16
average x 100 = 1233.3
i don't think every one in the class will have around the same number because around us there are different light sources and we also vary on our seeing abilities.
1. Ursa major- 7
2. Ursa minor- 14
3. Cassiopeia- 16
average x 100 = 1233.3
i don't think every one in the class will have around the same number because around us there are different light sources and we also vary on our seeing abilities.
Wednesday, August 27, 2008
astronomers
Aristotle (384-322BCE)

-Discovered the solar eclipse
-Said the earth was round
Hipparchus (190-120BCE)

-Measured distance between Earth and moon
-Measured rotation procession or Earth's rotation axis
Ptolemy (87-150)

- created the geocentric theory of the solar system
Copernicus (1473-1543)

-proved the sun was the center of the solar system using math
-in model of planets used elliptical orbits instead of round ones
Brahe (1546-1610)

-accurately cataloged 1000+ stars
-discovered a new star, Cassiopeia
Carl Sagan (1934-1996)

-solved the mysteries of the high temperatures on Venus
-experimented on mariner, viking, voyager, and viking
Galileo (1564-1642)

-verified that Venus goes though moon like phases
-discovered the other side of the moon
-found the four moons of Jupiter
-used tides to prove earth's movement
-discovered sun spots
-updated the telescope
Newton (1643-1727)

-Explained why planets were attracted to the sun
-used calculations to prove the earth's elliptical orbit
Einstein (1879-1955)

-found the equivalent between all matter and energy in the universe (e=mc2)
Hubble (1898-1953)

-devised a classification system for galaxies
Cannon (1863-1941)

-classified 250,000+ stars using the OBAFGKM classification system
Wilson (1936-)

-mapped the visible part of the milky way
S. Chandrasekhar (1910-1995)

-came up with the theory of white dwarfs
Tombaugh (1907-1997)

-discovered Pluto
-discovered a comet, 5 open clusters, a super cluster of galaxies, and a globular cluster
Hawking (1942-)

-proved black holes weren't black
-Unified general relativity theory and quantum theory
Pope Gregory XIII (1502-1585)

-created current calendar consisting of 365 days
Michelson (1852-1931)

-found speed of light
Van Allen (1914-2006)

-Mapped two main radiation belts
Bode (1747-1826)

-numerically proved Titus's law
-Discovered the solar eclipse
-Said the earth was round
Hipparchus (190-120BCE)
-Measured distance between Earth and moon
-Measured rotation procession or Earth's rotation axis
Ptolemy (87-150)
- created the geocentric theory of the solar system
Copernicus (1473-1543)
-proved the sun was the center of the solar system using math
-in model of planets used elliptical orbits instead of round ones
Brahe (1546-1610)
-accurately cataloged 1000+ stars
-discovered a new star, Cassiopeia
Carl Sagan (1934-1996)
-solved the mysteries of the high temperatures on Venus
-experimented on mariner, viking, voyager, and viking
Galileo (1564-1642)
-verified that Venus goes though moon like phases
-discovered the other side of the moon
-found the four moons of Jupiter
-used tides to prove earth's movement
-discovered sun spots
-updated the telescope
Newton (1643-1727)
-Explained why planets were attracted to the sun
-used calculations to prove the earth's elliptical orbit
Einstein (1879-1955)
-found the equivalent between all matter and energy in the universe (e=mc2)
Hubble (1898-1953)
-devised a classification system for galaxies
Cannon (1863-1941)
-classified 250,000+ stars using the OBAFGKM classification system
Wilson (1936-)
-mapped the visible part of the milky way
S. Chandrasekhar (1910-1995)
-came up with the theory of white dwarfs
Tombaugh (1907-1997)
-discovered Pluto
-discovered a comet, 5 open clusters, a super cluster of galaxies, and a globular cluster
Hawking (1942-)
-proved black holes weren't black
-Unified general relativity theory and quantum theory
Pope Gregory XIII (1502-1585)
-created current calendar consisting of 365 days
Michelson (1852-1931)
-found speed of light
Van Allen (1914-2006)
-Mapped two main radiation belts
Bode (1747-1826)
-numerically proved Titus's law
Sunday, August 24, 2008
Friday, August 22, 2008
sources
http://space.about.com/od/astronomerbiographies/a/aristotlebio.htm
http://www.astro.cornell.edu/academics/courses/astro201/earth_precess.htm
http://obs.nineplanets.org/psc/theman.html
http://www.planetary.org/about/founders/carl_sagan.html
http://scienceworld.wolfram.com/biography/Copernicus.html
http://www.lucidcafe.com/library/96feb/galileo.html
http://galileo.rice.edu/chron/galileo.html
http://kepler.nasa.gov/johannes.html
http://scienceworld.wolfram.com/biography/Newton.html
http://www.nada.kth.se/~fred/tycho/index.html
http://www.icstars.com/HTML/icstars/graphics/clyde.htm
http://www.hawking.org.uk/text/about/about.html
http://library.thinkquest.org/15418/cgi-bin/pageserv/srv.cgi?Section=timeline&SubSection=timeline&Page=1
http://www.aip.org/history/gap/Michelson/Michelson.html
http://www.astro.cornell.edu/academics/courses/astro201/bodes_law.htm
http://pmi.itmonline.com/netnotes/Big%20Questions%20Net%20Notes/Edwin%20Hubble%20-%20Bio.htm
http://www.myastrologybook.com/Albert-Einstein-history-of-astrology.htm
http://www.wellesley.edu/Astronomy/Annie/
http://nobelprize.org/nobel_prizes/physics/laureates/1983/chandrasekhar-autobio.html
http://nobelprize.org/nobel_prizes/physics/laureates/1978/wilson-autobio.html
http://www.astro.cornell.edu/academics/courses/astro201/earth_precess.htm
http://obs.nineplanets.org/psc/theman.html
http://www.planetary.org/about/founders/carl_sagan.html
http://scienceworld.wolfram.com/biography/Copernicus.html
http://www.lucidcafe.com/library/96feb/galileo.html
http://galileo.rice.edu/chron/galileo.html
http://kepler.nasa.gov/johannes.html
http://scienceworld.wolfram.com/biography/Newton.html
http://www.nada.kth.se/~fred/tycho/index.html
http://www.icstars.com/HTML/icstars/graphics/clyde.htm
http://www.hawking.org.uk/text/about/about.html
http://library.thinkquest.org/15418/cgi-bin/pageserv/srv.cgi?Section=timeline&SubSection=timeline&Page=1
http://www.aip.org/history/gap/Michelson/Michelson.html
http://www.astro.cornell.edu/academics/courses/astro201/bodes_law.htm
http://pmi.itmonline.com/netnotes/Big%20Questions%20Net%20Notes/Edwin%20Hubble%20-%20Bio.htm
http://www.myastrologybook.com/Albert-Einstein-history-of-astrology.htm
http://www.wellesley.edu/Astronomy/Annie/
http://nobelprize.org/nobel_prizes/physics/laureates/1983/chandrasekhar-autobio.html
http://nobelprize.org/nobel_prizes/physics/laureates/1978/wilson-autobio.html
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