Apophis

By Evan Finnes

On Friday the 13th, of April 2029 an asteroid approximately 330 meters in diameter will transverse the Earth’s orbit, coming nearer to the Earth than any other known asteroid in recorded history. Apophis was discovered in 2004 and after six months of optical and radar observations it was concluded that this asteroid will pass within 35700 km of the Earth, which is an altitude less than that of our satellites in geocentric orbit. Apophis will once again return on 2036, and astronomers say that if the asteroid’s center of mass passes through a small gravitational keyhole in the Earth’s atmosphere in 2029, Apophis’2 2036 orbit could be redirected into the Earth. Astronomers currently rank this asteroid has having little chance of impact, and is 0 on the Torino Scale.

The Torino scale is a scale from 0 to 10 that indicates the threat level of Near Earth Objects (NEO). A zero indicates that there is either no threat of impact, or that the object is too small to penetrate the atmosphere. A ten indicates that the object is likely to impact catastrophically. A NEO is assigned an integer value on the 0 to 10 scale based on impact probability and its kinetic energy. On December 23, 2004, Apophis had been given 1 in 233 chance of impact and a 2 on the Torino scale (Apophis is the first asteroid to have a value larger than 1 on the Torino scale). Later that day the odds of impact were increased to 1 in 64 with a 4 on the Torino scale. By 2006 the chance of impact has been reduced to 1 in 45,000 with a zero on the Torino scale.

In April 2008, a thirteen year old from Germany calculated the chances of collision to be 1 in 450 by factoring changes in the Asteroid’s orbit due to collisions with one or more geosynchronous satellites. To eliminate rumors that NASA and the ESA confirmed these calculations, NASA released a statement saying that the angle of approach relative to Earths equator, and the relatively small size of the satellites leave little or no chance of a satellite-asteroid collision.

Even though NASA has placed a low probability of impact, the threat is real enough that NASA plans on somehow deflecting the asteroid away from the tiny keyhole to prevent a future impact scenario. Some of these plans include nuking the asteroid, painting one half of it white, or by tugging it away using the gravitational pull of a probe. Nuking the asteroid has basically been ruled out because that may just result in showering us with several asteroid segments instead of one large one. Painting half of the asteroid white would result in the painted half of the asteroid reflecting more photons and thus pushing the asteroid in the desired direction, but this solution is impractical. Even if a good plan is developed it will do little good without precise and accurate details and calculations of the asteroid.

In 2008 the Planetary Society developed a $50,000 competition for the best mission designed to track the asteroid, and perform trajectory calculations for a year with an unmanned probe. The goal of the competition is to help Earth’s governments decide whether or not the probe should be deflected. The Planetary Society received 37 entries from 20 countries. The winning entry was designed by an Atlanta based company called Spaceworks Engineering. This plan called ‘foresight’ is planned to launch in 2012, after 5 months of travel it will rendezvous with Apophis, orbit it for one month while taking measurements with a multi-spectral imager. Once the orbiting phase is complete, the probe will follow Apophis around the sun for 10 months while it takes careful measurements of the asteroids orbit.

On Friday the 13th, in April of 2029, Apophis will be observable with the naked eye as it passes over the Earth at a distance of approximately 1/10 that of the moon. If you happen to be watching as the large asteroid come closer to the Earth than any other large asteroid in human history, remember one thing: even though calculus is perfect, the people who use it are not.

Kepler to Launch Soon

By Bellatrix

The Kepler Spacecraft is one step closer to launch. The Kepler spacecraft is set to launch in March of 2009, and its now packed up and ready to ship off to Cape Canaveral.

The launch of the Kepler Spacecraft will be an exciting one for planet hunters. It is named for the Dutch astronomer/mathematician Johannes Kepler who back in the 1500s derived some very important empirical laws describing planetary orbits. This spacecraft will be the most advanced piece of technology in the ever-growing arsenal used to detect exosolar planets. Kepler will monitor more than 100,000 stars simultaneously for signatures of planets of all sizes and orbital distances including earth sized planets. It will have the ability to detect rocky planets like Earth and ones that are located in the habitable zone of a star. For those unaware, the habitable zone is the area surrounding a star where the temperature i.e. distance from the star is such that life is possible. So in our solar system the habitable zone is more or less where Earth is and out to Mar’s orbit. So Kepler is not only expected to be the first to measure a Earth sized planet around a similar star but hopefully it should be able to tell us if they are rare or common, and thus whether possible life is rare or common.

Kepler is currently at the Ball Aerospace & Technology Corporation in Colorado, ready to leave for Florida. It hasp assed all its environmental tests and its pre-ship review. It will be launched atop a Delta 2 rocket and sent into an earth trailing solar orbit. It will be a solar orbit as opposed to the usual earth orbit so that earth will not obstruct its view of the stars since it will need considerably long exposure time to see such small planets. The telescope will be pointed at Cygnus, which is outside the elliptic of the solar system, which will prevent sunlight from obstructing the view of outside stars. Looking at Cygnus will also keep objects form the Kuiper Belt and asteroid belt from obstructing the starlight. The telescope will have a 1.4-meter mirror on it, the largest of any space based telescopes yet.

So with any hope the mission will launch as scheduled on March 5th. It has already been delayed several times due to budget issues (it was originally scheduled to launch in 2006 and is costing an estimated $467 million dollars). NASA other original mission to hopefully find earth-sized planets, the Terrestrial Planet Finder, was cancelled due to budget issues. But I think that this is one area in astronomy right now that has the most public support, so the most chance to receive funding. The general public may not be so concerned with something like WMAP (a spacecraft used to study the cosmic microwave background radiation) but the general public knows about finding other planets, about finding life outside of here; that is something easy to understand and still very exciting. So hopefully if Kepler is successful it will not only renew some lost passion for astronomy by the general public but also generate funding for future projects.

Could life exist on Super-Earths?

By Evan Finnes

The search for extraterrestrial life within our solar system has mainly been focused on Mars, and there has been speculation that some the moons of the outer solar system may also be a good place to look for life. Outside of our solar system, planet hunters and astrobiologists have been searching for Earth-like planets to help answer one of mankind’s most profound questions, “are we alone?” To date, no such planets have been discovered, so a team of scientists have now set their sights on a relatively abundant group of extrasolar planets known as “super-Earths”.

The term “super-Earth” is slightly misleading because the only thing that these planets have in common with the Earth is the fact that they are terrestrial. A super-Earth is typically classified as a terrestrial planet with a mass of 5 to 10 Earth masses. Thus far, Super Earths have not been found within the habitable zone of their host star, with orbits much too far or much too close to sustain life as we know it. The super-Earths with orbits far from their host star are the places that astrobiologists now believe could harbor some form of life.

It is estimated that one-third of all solar systems contain super-Earths, and some scientists believe that it may be possible to find some that have liquid water either on the surface, or below a thick layer of ice. This water could theoretically exist on a super-Earth if one of three conditions were met. 1) If the planet had a thick enough atmosphere it may be possible that enough solar radiation could be by greenhouse gases to prevent water from completely freezing. 2) If the planet was massive enough or young enough, there may still be enough primordial heat available to sustain some amount of liquid water.

Currently, the best technique for discovering super-Earths is by using gravitational microlensing. This phenomena occurs when an object in the foreground has enough mass, its gravitational field will bend the incoming light of a much more distant object. This results in the magnification of the distant object, no matter how faint it may seem.

It is not unfathomable to predict that an extrasolar super-Earth outside of its host stars habitable zone could contain water, at least as ice. Much of the ice in our own solar system is located outside of the habitable zone. There is no super-Earth in our solar system, but there are icy bodies that could contain liquid oceans. It is hypothesized that Jupiter’s moon, Europa, may have enough heat due to tidal flexing to permit a liquid ocean.

Traveling amongst the stars and exploring extrasolar planets is unfortunately not in the near future, but we can test hypothesis such as this one by exploring the planets within our solar system, and isn’t it about time we send a probe to Europa?

OUU Podcast #5: Something from Nothing

By Aridian PR
Our Undiscovered Universe Podcasts

LISTEN NOW:

[audio:http://ourundiscovereduniverse.com/podcast/OUUpodcast_01052009.mp3]

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OUU Podcast #5: Something from nothing

Welcome to the fifth in a series of podcasts that explore Null Physics as presented in the book, Our Undiscovered Universe, written by Scientist and Engineer, Terence Witt.

The topic of discussion today is “Something from nothing”, discussing various cosmology theories like the big bang and how they compare to the theory presented using Null Physics.

Also in Episode 5:

  • How does science address new ideas?
  • What role does the Big Bang play when scientists are looking for an alternative theory?
  • How did Null Physics evolve to the theory it is today?
  • What is the difference between a steady state universe of null or zero, and the theory that one began as zero then exploded with a bang?
  • Also available on iTunes! Search “Null Physics” and Subscribe Now!