Sunday, 1 April 2012
Monday, 26 March 2012
Jupiter and Venus
Friday, 16 March 2012
The Active Sun
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| Figure obtained from: Astronomy Picture of the Day |
The picture above was taken from astronomy
picture of the day. It was posted on March 15th 2012. The pictures
are of the gamma-ray sky and some recent activity that has occurred very close
to home. When one takes a picture of the
sky in the gamma ray region of the electromagnetic spectrum usually the most
exotic and energetic of astrophysical environments can be observed. An example would be like the active galaxies
such as quasars. These are very small galaxies that look like stars and they
are powered by supermassive black holes. Another example that is shown above
would be a dense pulsar. A pulsar is a rapidly rotation neutron star that emits
regular radio waves at rates around one thousand pulses per second. One can see that in the bottom picture the Sun
lights up part of the gamma ray sky. This is due to a massive solar flare that occurred
on March 7th. This is just one of the recent solar eruptions that
have occurred. This solar flare had energies
up to 1 billion times the energy of visible light photons. This is amazing because
on most other days the Sun would not show up in these gamma ray images because they
do not have the massive amounts of energy. The Sun will most likely shine again in the
gamma ray sky in the not so distinct future because we are approaching a
sunspot maximum. This is the period of time when the Sun will increase in
activity. This increase in activity may have effects on Earth. One of the main
effects would be auroras. As well the charged particles that are coming off of
the Sun during this active time may disrupt radio and electrical transmissions.
It will be neat to follow this increase in the Sun’s activity!
Saturday, 10 March 2012
Holy Moon!
Sunday, 4 March 2012
Spiral Galaxy ESO 510-13
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| Figure Obtained from: Astronomy Picture of the Day |
The
picture above was obtained but Astronomy Picture of the Day. It was posted on
March 4th 2012. This shows a
spiral galaxy edge on and it has a distinctive warped appearance. A galaxy is a
collection of millions, billions, or even trillions of stars gas and dust that
are gravitational bound. The material rotates around a center. The center of the galaxy is the location of a
supermassive black hole. Like our Milky Way Galaxy this galaxy is spiral. As well
from the edge on view one can see the dimensions of the galaxy. The length of
the galaxy is enormous compared to the thickness of the galaxy. The dark bands that are shown in the figure
above are where the gas and dust as well as some stars are located. As well there is a large part of the galaxy
that we are not able to see. This is the large amount of dark matter that is
located at the edge of the visible galaxy and it expands out to large distances. This dark matter is what allows deviations in
Kepler’s third law. If the orbit of the stars around the galactic center
follows Kepler’s third law then the further the star is away from the center
the slower it orbits of the stars around the center are. However, this is not
true for galaxies. The speed of rotation increases up until a certain point and
then it stays relatively constant as you move away from the galactic centers.
This change is caused by the sheer amount of dark matter that surrounds the
galaxy. But why is this galaxy warped? It is also important to note that the
disks of galaxies are thin and flat but not solid. It is thought that some
wraps result from interactions or collisions between galaxies. It however, is not completely known, and it is
also thought that our galaxy is thought to have a small warp.
Sunday, 26 February 2012
Sunday, 19 February 2012
Black Hole
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| Picture Obtained from Astronomy Picture of the Day |
This picture was obtained from astronomy picture of the day.
It was from February 24th 2004. It shows that a black hole is able
to rip up a star. Black holes are stellar remnants that are above three solar
masses. A black hole is formed because the neutron degeneracy pressure that
would keep a neutron star a star is overcome and therefore, the star is able to
collapse and become very dense. A black hole is composed of a singularity where
all the mass is held and then there is the event horizon which is the boundary
of the black hole. Once an object passes the event horizon it cannot escape.
The black hole has so much gravity that an object has to excess the speed of light.
This means that light cannot escape it. If there is material near a black hole it can
be pulled into the hole. In this picture the giant black hole pulls on the front of a closely passing star
much more strongly than the back. This is explained by general relativity. This strong tidal force would stretch out a
star and likely cause some of the star’s gasses to fall into the black
hole. This infalling gas emits x-rays
when the gases are heated when they are compressed from falling into the hole.
The picture above is an artist’s illustration of the sequence of destruction of
the star by the black hole. When the star is destroyed most of the stellar
remains would be flung out into the galaxy. This aspect of the destruction does
not make sense to me. I would think that the material would spiral into the
black home because the star is close enough to the hole and the gravity is large
enough to rip the star apart. However,
these event are rare and occur only once every
10000 years the black holes are located at the center of galaxies. Even though I am not sure about all the
processes that are going on but I know that black holes are very powerful
aspects of the universe.
Sunday, 12 February 2012
A Globular Cluster and A Comet
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| Figure Obtained from: Astronomy Picture of the Day |
The picture that
was posted on Astronomy Picture of the day on February 4th 2012 is a
picture of a comet as well as a globular cluster. The comet that is shown in
the picture is called Comet Garradd and it is slowly moving through the constellation
Hercules. Comets are characterized by the tails that they emit when they are
close to a star. The ice on the comet vaporizes and forms and ion tail and the
other tail are a dust tail. The dust tail is caused when the ice melts and
there is nothing to hold the dust in a clump anymore. The tails of the comets
will always point away from the star and the curved tail is the dust tail. The reason that the tails point away from the
star is because they are pushed out by the pressure of the starlight. The other
interesting aspect of this picture is the cluster of stars that can be observed
to the left of the comet. This cluster of stars is known as a globular cluster.
This means that the stars in the clusters are horizontal branch stars, red
giants, and lower mass main sequence stars. A globular cluster will have an
absence of high mass main sequence stars because of the life time of these
stars. Globular clusters are clusters of stars that are gravitationally bounded
to each other. This means that there are very few stars that can escape the
cluster. Globular clusters are also
thought to be older clusters and this can be seen because of the absence of the
high mass main sequence stars. Larger main sequence stars burn bright a die
young and therefore, these stars would have already burnt through the main sequence
and would have turned off the main sequence to become a giant and finish the
post main sequence stellar evolution. This picture is interesting because it allows
one to look at two aspects of the universe.
Sunday, 5 February 2012
Spirit and Opportunity
Sunday, 29 January 2012
Saturday, 21 January 2012
The Witch Head Nebula
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| Picture obtained from: Astronomy Picture of the Day |
This week I will take a closer look at the photograph that was posted on Astronomy Picture of the Day. This picture was posted on January 17th. One can see that this is a nebula and it is located in the constellation Orion. It is called the Witch Head nebula because many people are able to see the silhouette of a witches face. I however, cannot see the head. This nebula is close to 1000 light years away and has a blue appearance for two reasons. One of the reasons is because of Rigel’s blue color. The other reason is because the dust grains reflect blue light. The nebula is made of large amounts or gas and dust and may collapse to form another star or star system. The clouds can collapse under the influence of its own gravitational attraction. This process is known as Jeans instability. The cloud can reach this unstable point in a number of different ways. Stars that are nearby can cause winds that can compress gas and dust in the nebula, a shockwave from a supernova can cause the nebula to collapses and finally the collapse can occur when clouds collided together. When the nebula collapses a star forms. By studying nebulae like this one may be able to better understand the process of star formation.
Friday, 13 January 2012
Aurora
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| Figure obtained from:Astronomy Picture of the Day |
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