Thanks to this student blog, over the semester, I have deepened my knowledge of some very useful astronomy concepts. I have learned more about binary systems, black holes, star formation, exoplanets, and many other extremely interesting astronomy concepts.
Astronomy is my major and it is a very important part of my life so doing something i love and getting to express some of my thoughts about it to this big internet community has been a blessing. I loved the fact that I got so many views and I even got comments and or questions on some of my blog posts. I have to say that I liked the questions the most because they were really good questions.
I want to thank everyone for ready this blog and I hope you all will continue to read the blog in the future!
ASTRONOMY IS THE FUTURE!!!!!!!!
This blog is authored by students taking Astro 305, Astronomy and the Community.
Sunday, December 9, 2012
Tuesday, December 4, 2012
Colloquium November 29
On November 29, 2012 the University of
Michigan welcomed Andy Fabian to speak on Black holes and their environments.
Andy Fabian is a professor at the University of Cambridge. He has received many awards through out his career and he has taught around the world.
During his lecture Fabian focused primarily on the way we view black holes. He talked about how the amount of radiation (energy from matter around the black hole) depends on what surrounds the black hole. He gave details about how we view the spectra of the released energy. He said that the radiation that is sent out by black holes is often in the X-ray band because it has such high energy.
Fabian talked about how the energy of a black hole varies if it has a spinning accretion disk or a non spinning accretion disk. He said that spinning accretion disks release 5 times more energy (radiation) than non spinning disks release. He also said that some black hole shoot jets and these jets can go out as far as 5 Mpcs.
Monday, December 3, 2012
Black hole's affected by surrounding matter
Many black holes are affected by matter that is found around them. These objects that affect black holes include orbiting stars, gas, planetary objects, comets, asteroids, and many other celestial object.
When Black holes are affected astronomers can view the effects through X-ray emissions from the luminous black holes. Astronomers, through X-ray emissions, can see the black hole's strong gravitational affects, its gravity redshifts, its gravitational light bending, its delays, and its dragging of inertial frames in the Kerr metric.
The accretion disks that surround black holes include lots of dust that affect the energy outputs of the black holes. These disks can create soft X-ray emission or hard X-ray emission. These accretion disks can surround both spinning and non spinning black holes. However, spinning black holes produce 5 times as much power as non spinning black holes.
When Black holes are affected astronomers can view the effects through X-ray emissions from the luminous black holes. Astronomers, through X-ray emissions, can see the black hole's strong gravitational affects, its gravity redshifts, its gravitational light bending, its delays, and its dragging of inertial frames in the Kerr metric.
The accretion disks that surround black holes include lots of dust that affect the energy outputs of the black holes. These disks can create soft X-ray emission or hard X-ray emission. These accretion disks can surround both spinning and non spinning black holes. However, spinning black holes produce 5 times as much power as non spinning black holes.
End of Term Evaluation
If you've been reading this blog this term, we'd really appreciate it if you could take a minute or two to let us know what you thought.
It really is quick!
It really is quick!
Tuesday, November 27, 2012
Colluqium November 15
On November 15, 2012 the University of Michigan welcomed Dennis Bodewits to speak on comets and asteroids.
Dennis Bodewits is an assistant research scientist in the Astronomy Department at the University of Maryland. "His research emphasizes comets and asteroids, and he is a member of the EPOXI/Deep Impact and Stardust-Next science teams. His observational studies encompass X-ray, UV and visible regions, and makes use of mostly space-born telescopes, such as Swift, Chandra, and XMM-Newton".(http://www.astro.umd.edu/people/dennis.html)
In his speech Bodewits focused on the roles comets and asteroids played in the creation of water on Earth. He had videos and many photos of artistic interpretations of water formation of Earth. Bodewits also gave detailed explanations of the compositions of asteroids and comets.
For more information on comets here is a link: http://www.michastrostudent.blogspot.com/2012/11/comets.html. For more information on asteroids here is a link: http://www.michastrostudent.blogspot.com/2012/11/asteroids.html. For more information on water formation on Earth here is a link: http://www.michastrostudent.blogspot.com/2012/11/the-water-of-earth-contribution-of.html.
Saturday, November 24, 2012
The Water of Earth. The Contribution of Asteroids, Comets, and Meteors
Earth is
a fascinating and amazing planet to study because it has surface
water. Surface water is an extremely valuable resource. It is
arguably the most valuable resource on Earth because it is essential
to all living organisms and it formed over a large amount of time.
Water formed on Earth through a process that lasted millions of
years.
The process that allowed water to form on Earth included;
asteroids, comets, and meteors. Astronomers have many theories about
this process. Some astronomers have different beliefs about the
ratio of comets, meteors, and asteroids that were involved in the
formation of water on Earth. All of the different theories that
involve the different ratios and time scales can all be justified
because no one really knows how water formed on the surface of
the Earth. It is impossible to know because humans had not even been
created when water formed on Earth. However, astronomers know that
asteroids, meteors, and comets played a role in water formation on
the surface of earth because the water had to have come from some
outside source.
Asteroids, comets,
and meteors are very important celestial bodies that have been found
in our solar system. Most importantly asteroids, comets, and
meteors, contributed to water formation on the surface of the Earth.
These celestial bodies, any natural body outside of the solar system,
have been studied for many years and they are all very different from
one another. Their differences make them very interesting.
Asteroids are airless objects, most commonly found in the asteroid
belt. The asteroid belt is located Mars and Jupiter. For more information on asteroids here is a link http://www.michastrostudent.blogspot.com/2012/11/asteroids.html
Comets
are icy objects, most commonly found in the Oort cloud. The Oort
cloud is a spherical cloud located 50,000 AU from the Sun.
For more information on comets here is a link http://www.michastrostudent.blogspot.com/2012/11/comets.html
Meteors are dust to bolder sized particles of debris that are found
in the solar system.
Meteorites that
astronomers have studied on Earth have hydrogen isotope ratios that
help explain how elements like hydrogen and nitrogen got on the
Earth.
The biggest question astronomers are trying to
answer is how volatiles like hydrogen, nitrogen, and carbon first
arrived on Earth. Astronomers mostly believe that these elements
arrived on Earth through collisions with comets and asteroids.
One of the most accepted theories on how water formed on Earth
suggests that during the creation of the solar system Jupiter and
Saturn's orbits were disturbed and that caused comets in the outer
solar system to move inward and later make their way towards Earth. These comets collided with Earth and left ice and other
elements behind. Later when an asteroid collided with the Earth,
the ice was melted and liquid water was then formed on the surface of
the Earth. This process, according to astronomers, happened many
times and it took millions of years.
Friday, November 23, 2012
Comets
Comets are known as “dirty
snowballs,” because they consist of a mixture of ices (both of
water and frozen gases), carbon dioxide, ammonia, methane, and dust.
The core of a comet is solid and it consists of ice and dust.
Comets also
have two tails. The first tail is an ion tail. The ion tail is blue
because it consists of ionized CO+ and it scatters blue light. The
second tail is the dust tail. The dust tail is green and consists of
the dust that is pushed off of the comet and reflects radiation from
other sources. The tails of a comet can reach 160 million kilometer
long.
The average comet
has a mass of 10^14 kg, a diameter of 20 km, a density of 0.6 g/cm^3,
and an albedo of .05.
Comets are
mostly located in the Oort cloud, except for the occasional comets
that streaks through the inner solar system. The Oort cloud holds
millions and millions of comets and the Oort cloud is found much
farther out than the orbit of Pluto. It is generally believed that we
got our water when comets collided with the Earth.
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