Ahhh, tis Thursday and time for another installment of Schopenhauer Was Right. However, in its stead I want to very briefly address an epistemological concern I’ve been chewing on lately:  The abandoned treatment of essential purpose(s) in scientific method manifest in the treatment of supermassive black holes.

For the record, I must distinguish what I mean by essential purpose.  For example, it may be rightfully said that supermassive black holes cause the formation of spiral galaxies.  If may also be said that spiral galaxies cause the formation of supermassive black holes.  Neither of these statements address the essential purposes of supermassive black holes as vital constituents of spiral galaxies.  To be essential is to be purposeful – to be vital to the constitution of an existing whole.

In his book, Our Undiscovered Universe: Introducing Null Physics, Terence Witt outlines a cosmology based on his theory Null physics. His Null cosmology accounts for the purposes of supermassive black holes observed at the center of spiral galaxies. Indeed, by asking the question “Why are supermassive black holes at the center of spiral galaxies”, Mr. Witt reminds all of us that the universe is not superfluous in essence or purpose. Are there nonessential physical laws? Are there excesses of gravitational forces or electromagnetic currents upsetting the balance of our universe?

Terence Witt represents the general will of a number of thinkers who remain unsatisfied with the direction science has chosen in forsaking the essential purposes of things in order simply describe what things do and what they may do. We are reasonably confident in our understanding of black holes i.e. how they interact with matter and light. Additionally, we must similarly seek to understand the essential purpose of supermassive black holes. Or are we to believe supermassive black holes have no purpose in relation to the stellar and planetary swirl of a spiral galaxy?

Saturn’s sixth largest moon, Enceladus, was discovered in 1789 by British Astronomer William Herschel. With a low albedo and close proximity to Saturn, Enceladus is difficult to observe. Because of this difficulty little was known about this moon until the Voyager flybys in the 1980’s. Voyager 1 discovered that Enceladus is located in the densest part of Saturn’s E Ring, and Voyager 2 discovered that Enceladus has diverse and relatively complicated surface features.

The Voyager missions generated a number of questions about the small moon: “Is there a connection between Enceladus and Saturn’s E-ring?” “What is causing the tectonic activity which is deforming Enceladus’s surface?” The recent Cassini mission was able to answer these questions, along with generation new discoveries and new questions.

To answer the first question, Cassini discovered that Enceladus is the fourth known body in the solar system with active volcanism. The other three are Earth, Jupiter’s moon Io, and Neptune’s moon Triton. This volcanism causes icy jets, plumes of water vapor, and other materials to be shot into the atmosphere. It is this cryovolcanism which was determined to be the cause of Saturn’s E Ring. Just recently Cassini photographed the volcanic southern pole. These pictures revealed a geological feature scientists are calling “tiger stripes”. These tiger stripes are 300 meter deep fractures and are surrounded by chunks of ice, and are the source of Enceladus’s volcanism.

Cassini also discovered the cause of the tectonic activity. Enceladus, like many other moons is traped in orbital resonances, this causes tidal heating on the moons interior. Like thought to exist on Jupiter’s moon Europa, this could also cause Enceladus to have a subsurface liquid ocean. Because of the volcanic activity a subsurface ocean on Enceladus is though to be only tens of meters beneath the surface, where the oceans on Europa are thought to be 100 kilometers beneath the surface.

Does Enceladus have a subsurface ocean? If it does, is this another place to look for signs of life? With many more Enceladus flybys to come, we may yet find out if there is a subsurface ocean, but we will certainly have to wait for the right mission if we want to determine if life exists.

It has been nearly three months now since GLAST was launched, NASA’s Gamma-ray Large Area Telescope. The telescope isn’t fully functional right now, but according to NASA’s website the telescope is up and running and so far passing all of the checks the engineers are laying out.

Gamma rays are some of the most powerful and mysterious objects detected in space so far. As their name entails they are short-lived bursts of gamma ray photons, having energies ranging from a thousand electron volts to several billion electron volts. They range in duration from a few tenths of a second to a few minutes. However, this very short duration makes them very hard to detect and gather data on, since by the time a telescope is alerted to a burst and pointed in the right direction the burst will be over.

Gamma ray bursts are not well understood. They weren’t discovered until the 1960’s, and as late as the 1990’s astronomers weren’t even sure if these bursts were coming from the edge of the solar system or the edge of the universe. However, with recent advancement in technologies we’ve been discovering much more about them, giving us clues to their origin. We now know there are two different classifications of gamma ray bursts. Long Duration ones are bursts lasting 2 seconds to a few minutes, short duration ones are shorter than 30 seconds. Astronomers think fundamentally different processes create them. Long bursts are believed to be generated billions of light years away by the death or collapse of very massive stars, or Wolf Rayet stars. Short bursts are less understood, but may be created in very high energy collisions like between two neutron stars or a neutron star and black hole.

GLAST will be able to cover much more of the sky than the current gamma ray satellite, SWIFT. The GLAST team is currently in the process of checking the validity of the burst locations it detects. So far, GLAST has detected 12 bursts, and other telescopes have so far verified four of these bursts. Once all the checks have been performed and the team operations are running smoothly GLAST should start making some great discoveries. It will be able to gather data on a much higher number of bursts and tell us about the area from which they originated. Matching up the bursts with data about the originating area from before the bursts will hopefully tell us more about how they are created, such as if a known super giant star is in the vicinity of the bursts before but not after the burst.

New technology for this purpose is quite exciting. There are so many strange and mysterious things in the Universe we still don’t understand; to have something that may lead to a new discovery in astronomy is thrilling. It will be important to keep an eye on the data coming in once GLAST really gets going.

Can life exist in the harsh conditions of our solar system? Could life evolve and survive under the extreme heat and pressure of Venus, under the icy crust of Mars, or in the oceans of Europa? To find out just how resilient life is, scientists have been looking for answers in some of the most hostile environments on Earth. And in recent years, life has been discovered in the most extreme conditions, previously thought to be uninhabitable. These microorganisms are sometimes called extremophiles.

There are many different classes of extremophiles, which are named according to the environmental conditions in which they thrive. For example, a thermophile is an organism which lives in conditions between 60˚ and 80˚ Celsius. Recently, a thermophile was discovered nearly two miles beneath the Earth’s surface in the Mponeng Gold mine of South Africa. This particular discovery is interesting because these thermophiles are completely devoid of sunlight, surviving on the byproducts of radioactive decay.

Where might we look for extremophiles outside of Earth? Mars is a good place to start. With the recent confirmation of ice in the crust, it is possible that water has trickled deep into the Martian interior, where thermophiles can survive off of radioactive materials like previously discussed. On Earth, we have discovered halophiles, which require high amounts of salt to survive; recently, the Phoenix Lander discovered several different types of salts in the Martian soil, which could be another location to search for life. Other types of extremophiles discovered on Earth may also apply to Mars, such as: xerophiles, hypoliths, and radioresistant extremophiles.

Europa is another great place to look for extremophiles. It is theorized that there is a global ocean beneath Europa’s thick layer of surface ice. Sattelite images of Europa’s surface show a complex system of tectonic activity–places where the ice has broken and liquid water has upwelled to the surface and refrozen. This tectonic activity is likely the result of tidal flexing, due to the gravitational pull of Jupiter. This tidal flexing may also produce hydrothermal vents. Earth’s hydrothermal vents are host to a large amount of biological activity, meaning Europa is a very promising place to look for extremophiles.

There are future plans in the works to search for extremophiles in the Martian crust. Astrobiological missions to Europa, Titan, or elsewhere are probably deep into the future. Given the amount of life discovered in the harshest places on Earth, I will be surprised if we find that our solar system is devoid of life.