Top 10 Ways the Universe Could Kill Us! July 24, 2009
Posted by kfarley in Asteroid, Astronomy, Cosmology.Tags: Asteroid, blackholes, Gamma Ray Burst, neutron star
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Asteroid Impact
Asteroids and other near-Earth objects (NEOs) come near the Earth more frequently than one would guess. Question: Why don’t we ever hear of these objects hitting the Earth? Answer: Because they don’t. More often than not our atmosphere causes great friction on these solar bodies causing them to burn up. This happens before the asteroids can go through our atmosphere and hit the Earth. Our atmosphere can be a good friend to us – protecting us from solar debris that could potentially hit Earth and end civilization as we know it. If an asteroid were to make it through our atmosphere it becomes classified as a meteor. It is theorized that a large meteor hit the Earth about 65 million years ago wiping out the dinosaurs. According to NASA, a meteor about 1/5 that size will hit the Earth about once or twice every million years. If Earth did get hit by an asteroid of that caliber we would most likely not survive. I haven’t heard of an asteroid that size hitting the Earth in quite some time, maybe we’re overdue. With ≈6.7 billion people in the world your chance of seeing the Earth hit by that size meteor is…well, you do the math. To learn more information on NEOs check out NASA’s FAQs.

Illustration of an asteroid that could have wiped out the dinosaurs.
Solar Flare
A solar flare is a huge explosion of energy in the Sun’s atmosphere. Think of it like a giant spike of light and heat that suddenly rises off the surface of the Sun. The rays emitted (mainly X-rays and UV rays) from this explosion are strong enough to disrupt radio communication on Earth! The flares can influence the surface of Earth by having an effect on our weather. Just outside our atmosphere, the flares can present radiation hazards to spacecraft and astronauts. The solar flares can also produce streams of highly energetic particles in our atmosphere. These highly energetic particles help in the production of the beautiful aurora borealis! On the other hand, the radiation from solar flares also pose incredible complications that could arise during manned missions to Mars, the Moon, or other space travel. Satellites’ orbital paths can also be disrupted by the solar flares. Kind of a catch-22, amazing Northern lights produced but also possible space travel limit. Hmm…

Aurora borealis co-created by solar flares.
Supernova
Ever had someone shine a flashlight in your eyes? Not very nice, huh? Think of shining a light in your eyes a billion times brighter! A supernova is just that – an exploding star billions of times brighter that our Sun. After the core of a star collapses it emits great energy as a flash of growing intensity before fading back out of sight. If a supernova was close enough and aimed toward our solar system, it could wipe out our atmosphere. Our planet would overheat from UV rays causing mass extinction. It’s messy too. The supernova will throw large clouds of dust and gas into space that could exceed 10 times the mass of our Sun. We should be thankful for supernovae in a way. It is hypothesized supernovae created the heavier elements such as gold, iron, and uranium found here on Earth.

Supernova.
Gamma Ray Burst
Gamma ray bursts (GRBs) are flashes of gamma rays that last from fractions of a second to almost an hour. They normally last a few seconds and usually come from outside our galaxy. They are the most luminous (electromagnetic) events that occur in the universe. GRBs often have an afterglow affect as longer wavelengths travel from the blast. The blast from a GRB in our galaxy would definitely cause mass extinction from the intense rays that would encompass our planet. It is hypothesized such an event caused the mass planetary extinction on Earth about 444 million years ago. A GRB depleted the ozone layer leaving our planet helpless to direct UV rays that heated and kill organisms until food chains were depleted.
P.S. Gamma rays gave the Hulk his powers (I think that is fictional though).

Illustration of a gamma ray burst hitting a planet like Earth.
Black hole
Black holes are areas in space in which the gravitational field is so incredible that nothing can escape its pull. Not even light can be reflected from this object, hence its name. It is virtually impossible to escape a black hole once its immense gravitational pull has a hold of you. The point of no return at a black hole is called the horizon. It is an area just outside a black hole where the gravitational pull begins. Once you hit the horizon of a black hole your fate is sealed and escape from the black hole is futile. Knowing not even light can escape the pull of the black hole, you would have to travel faster than the speed of light to escape. If you were to see an object being pulled into a black hole (assuming the object can still reflect light), it would become extremely distorted. The gravitational pull is so intense, the part of the object entering the black hole first would stretch out of normal proportions. For example, if you were floating through space with your arms in front of you (Superman-style) and began to be sucked into a black hole, your arms would stretch out incredibly long before the rest of your body. Black holes are also very massive. They can range anywhere from 10 times to a million times the mass of our Sun. Currently, there are no known black holes in our galaxy. This known with the fact our space travel is limited to our Moon, you are probably safe from a black hole fate.

Illustration of what a black hole over the Milky Way might look like.
Death of Sun
The Sun goes through different stages during its life cycle. It’s about halfway through the “main sequence” before it goes into a different star phase. The Sun will most likely turn into a Red Giant star peaking at its highest luminosity. The Sun will then start to burn out as it turns into a small dwarf star. The Sun won’t turn into a Red Giant for another 5 billion years or so. A more immediate problem, as the Sun moves toward the next stage it becomes gradually warmer. It will get really hot. Life on Earth most likely won’t make it to the Red Giant stage. The Earth will warm up to the point where life will not be sustainable. The Sun has slowly been warming up ever since its birth. The Sun used to not be as hot, one of the reasons life didn’t always exist on the Earth. Just as the warmth of the Sun allowed life on Earth, it will also take it away.

The life cycle of our Sun.
Heat Death of Universe
The heat death of the universe occurs as all the stars and other universal matter continues to expand and uses up its energy or “burns out.” It’s like letting a candle burn and not blowing it out. Eventually it’s going to use up the wax and wick until it can’t burn anymore. The universe runs on “free” energy that is not endless. At some point the fuel for the universe will run out cutting of the energy for the cosmic bodies that give us life (namely our Sun). This probably won’t be happening anytime soon. It’s estimated the energy will run out after black holes vanish in about 10100 years (according to Hawking’s radiation). That’s one big candle!

The flame of life.
The Big Rip
Just like how it sounds, all matter of the universe will be ripped apart. We’ve all heard that the universe is expanding. What would happen if the expansion increased at an accelerated rate? If the universe expanded much faster than it is now, all the galaxies, stars, planets, dust, etc. would be ripped apart! Think of it like a twizzlers. If you pull slowly you can stretch out the twizzlers pretty far. If you stretch too fast the twizzlers will just snap in half. This is a possibility for our universe. The hands pulling on our universe is something called dark energy. Dark energy is a hypothetical energy that saturates all our universe. It is theorized it helps our universe expand – at an accelerating pace. This means the expansion is moving at a faster and faster rate as time goes by. Eventually the universe will reach that point where it is pulling to fast, ripping apart everything. What happens when everything is ripped apart and away from each other? No one knows.

The Big Rip.
Cannibal Galaxies
Cannibal galaxies occur when a smaller galaxy is eaten by a larger galaxy! Natural selection at its best. Galaxies are gravitationally bound collections of stars, stellar bodies such as planets, space dust, and other objects. You are probably most familiar with the Milky Way galaxy (you should know this one, we live in it). Scientists can now detect our Milky Way galaxy is currently tearing apart and engulfing the Sagittarius galaxy as you read this! Closer to home than you might have expected. I guess we are saved this time but poor little Sagittarius galaxy…

Larger galaxy engulfing a smaller galaxy. (Swinburne)
Pulsar
When a star collapses on itself a neutron star is left behind. If we were to survive this giant explosion, we would have a new problem of pulsars to deal with. A pulsar is a neutron star that emits rays of electromagnetic radiation. Electromagnetic radiation is rays that vary depending on their frequency and wavelength. Some rays provide us with the visible light we use every day. Other rays below or above the spectra can be very harmful to us. For instance, radio waves (beyond red in the visible spectra) can vibrate the cells in your body heating them up to a deadly temperature while gamma rays (beyond blue in the visible spectra) can stop the function of the cells in your body. Oddly enough, both radio waves and gamma rays are used to treat different ailments.

The Vela Pulsar. NASA pic.
New Impact on Jupiter July 21, 2009
Posted by jcconwell in Asteroid, Astronomy, planets.Tags: Asteroid, Jupiter, Solar System
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Taken from the article by Nancy Atkinson at Universe Today
Amateur astronomer Anthony Wesley from Canberra, Australia captured an image of Jupiter on July 19 showing a possible new impact site. Anthony’s image shows a new dark spot in the South Polar Region of Jupiter, at approximately 216° longitude in System 2. It looks very similar to the impact marks made on Jupiter when comet Shoemaker-Levy 9 crashed into the gas giant in 1994. (But read the Bad Astronomer’s post that the black spot could also be weather.)
UPDATE (7/20): It has been confirmed this is an impact on Jupiter. Mike Salway shared the news Glenn Orton from JPL has imaged the Jupiter black spot with the NASA Infrared Telescope and he has confirmed it’s an impact.
Tunguska…The Mystery Continues July 17, 2009
Posted by sgoebel in Asteroid, Astronomy.Tags: Asteroid, comet, meteor, NEO, Tunguska
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Shannon Goebel has her blog at: http://mrsgoebel.wordpress.com/
As the saying goes, everyone loves a good mystery and the 1908 Tunguska Event does not disappoint. I have long been fascinated by this story and love to discuss it each year with my Earth Science students. However, just as in my classroom before we can delve into the juicy details and “who-dun-it’s”, we must first explore the history surrounding this event.
When? Where?
It was a quiet morning around seven o’clock on June 30, 1908 (June 17, 1908 according to the Julian Calendar which was in local use at the time) in remote Siberia near the Podkamennaya Tunguska River. The day started just like any other; no one would have predicted that it would forever be recorded and remembered for the unique and literally Earth-shattering event that would take place. One of the first questions that probably comes to your mind, is where exactly is this place? Shown on the map below, the Tunguska River is located in what is known today as the Krasnoyarsk Krai in Russia.
Photo taken from www.science.nasa.gov
What?
- Photo taken by Professor Leonid Kulik on his 1927 expedition to the impact site.
While on their investigation, the crew collected numerous eyewitness testimonies like the one given below by S. Semenov.
“At breakfast time I was sitting by the house at Vanavara Trading Post (65 kilometres/40 miles south of the explosion), facing north. [...] I suddenly saw that directly to the north, over Onkoul’s Tunguska Road, the sky split in two and fire appeared high and wide over the forest (as Semenov showed, about 50 degrees up – expedition note). The split in the sky grew larger, and the entire northern side was covered with fire. At that moment I became so hot that I couldn’t bear it, as if my shirt was on fire; from the northern side, where the fire was, came strong heat. I wanted to tear off my shirt and throw it down, but then the sky shut closed, and a strong thump sounded, and I was thrown a few yards. I lost my senses for a moment, but then my wife ran out and led me to the house. After that such noise came, as if rocks were falling or cannons were firing, the earth shook, and when I was on the ground, I pressed my head down, fearing rocks would smash it. When the sky opened up, hot wind raced between the houses, like from cannons, which left traces in the ground like pathways, and it damaged some crops. Later we saw that many windows were shattered, and in the barn a part of the iron lock snapped.”
Bob Holmes Newspaper article May 18, 2009
Posted by jcconwell in Asteroid, Astronomy, Observatory.Tags: ARI, Asteroid, EIU
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Bob Holmes, who is an adjunct faculty member in the EIU physics department, has a very nice newspaper article about his research with NASA searching for “killer asteroids”. To read the article online go to the http://jg-tc.com
Asteroid 2009 BD81 Removed from Risk List February 11, 2009
Posted by jcconwell in Asteroid, Asteroids, Astronomy.Tags: 2009 BD81, Asteroid, Astronomy
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This in from The Tracking News JPL/NASA has removed asteroid 2009 bd from the risk page, after new observations that have narrowed the impact uncertainty to exclude Earth.
Summary Risk Table for Risk Assessments Updated Today (last checks: NEODyS and JPL at 2358 UTC)
See the CRT page for a list of all objects rated recently as risks and our ephemerides page for a list of risk-listed objects under current observation.
The time horizon for JPL is 100 years from today and for NEODyS is usually the year 2090. Beginning Jan. 22nd, both are also posting impact solutions beyond 100 years for a few objects.
For the latest official risk assessments, and for explanations of the terminology, see the JPL NEO Program Sentry and NEODyS CLOMON (backup) risk pages.
| Object | Risk Monitor |
When Noted UTC |
Year | Prob Cum |
PS Cum |
PS Max |
Notes for Today’s Latest Risk | ||
| 2009 BD81 | JPLSentry | 1605 | R E M O V E D | JPL: Risk listing removed at 1549 UTC. | |||||
Bob Holmes mentioned at “Universe Today” February 7, 2009
Posted by jcconwell in Asteroid, Asteroids, Observatory.Tags: 2009 BD81, ARI, Asteroid, EIU, NEO
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Nancy Atkinson of Universe today just did a very nice article on Bob Holmes, our adjunct faculty member in the physics department here at EIU. It tells about his discovery this week of a NEO (see previous article in this blog) and the work at his observatory ARI (Astronomical Research Institute). Just click on the link below to go to the article.
http://www.universetoday.com/2009/02/07/new-potentially-hazardous-asteroid-discovered/
Some visual aids for asteroid 2009 BD81 February 4, 2009
Posted by jcconwell in Asteroid, Asteroids, Astronomy.Tags: 2009 BD81, ARI, Asteroid, Astronomy, NEO
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My thanks to Bob Holmes of ARI for supplying me with his photos of the asteroid. The first picture is a series of timed lapse photos taken with ARI 32″ telescope showing the discovery. You’ll notice it’s a negative image, which is very common for astronomers to work with, since it makes for easier visual identification.
The second image is a from NASA/JPL Risk web page which shows the orbit
Click on the picture to see the orbital motion.
More information may be found at the ARI’s web page about the object at
New Asteroid Discovered 2009 BD81, listed as “Risk” object by NASA February 3, 2009
Posted by jcconwell in Asteroid, Asteroids, Astronomy.Tags: 2009 BD81, ARI, Asteroid, Astronomy, EIU, meteor
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This just in from Robert Holmes of ARI in Charleston and an adjunct faculty member in the physics department of Eastern Illinois University.
Friday night while measuring 2008 EV1, Robert Holmes found another high speed object moving through the same field. It turned out to be an undiscovered “Potentially Hazardous Asteroid”. A few hours later, a teacher from Texas was using Robert Holmes data measuring 2008 EV1 in a class and also found the new object. A student in Bulgaria that is part of ARO education and public outreach also notice the new asteroid. Holmes listed both observers as measurers and co-discovers as well as H. Devore for confirmation follow-up observations of what is now 2009 BD81. This object is a “Risk” object now listed on the NASA/JPL website and has 10 potential impact risks after March 4th 2042. That year it will miss the earth by just 5.5 earth radii. It will make an even closer approach in 2044. At the end of the month this PHA will pass within 7 million kilometers of earth. The object is small at H = 20.2 and a diameter of 0.314 km. This is the 1,015th PHA discovered to date.
For published discovery details see:
http://www.cfa.harvard.edu/mpec/K09/K09C09.html
NASA/JPL risk page: http://neo.jpl.nasa.gov/risk/2009bd81.html
NEO DyS data:
http://newton.dm.unipi.it/cgi-bin/neodys/neoibo?objects:2009BD81;main
Meteor Update. October 14, 2008
Posted by jcconwell in Asteroid, Astronomy.Tags: Asteroid, meteor
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The asteroid that was predicted to hit Earth over the Sudan last week did have a Kodak moment . A weather satellite, METROSAT-8, was lucky enough to catch the fireball (from above!) as it was burning up in the atmosphere. For more information, go the the EUMETSAT site
Update: Impact of Asteroid 2008 TC3 Confirmed! October 8, 2008
Posted by jcconwell in Asteroid, Astronomy.Tags: Asteroid, meteor
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A bright fireball was observed and sonic sensors registered a upper atomsphere explosion in the range of 1000 tons of TNT over northern Sudan. For more information check out the NASA NEO news.






