Sunday, February 19, 2017

Section 6 - Observers from the Great Beyond

Then:


            The deployment and usage of satellites and space probes hadn’t started until a surprisingly long time period of five decades ago. Before then, we did not have access to rockets powerful enough to launch something out of our planet’s atmosphere and into space. That changed after World War II, however, and soon afterwards the Union of Soviet Socialist Republics, more commonly known as the Soviet Union, launched the world’s first ever satellite, dubbed Sputnik I, into space on October 4, 1957. Despite being the first satellite, it did little other than beep periodically, yet the fact that it was a man-made satellite in space that was not the United States’ property was enough to kick our own space program into gear. Not even half a year later, the United States launched the first American satellite, dubbed Explorer I, into space on January 31, 1958 (space exploration 2016). Explorer I was understandably simple in comparison to the satellites and lunar probes that we launch in our current day and age, yet they were far from just useless displays of a country’s ability to launch chunks of metal into the void surrounding our planet.
Despite looking just like the original, the real Sputnik I burned up in the Earth's atmosphere.
            It is impressive just how much information we managed to squeeze out of Sputnik I during its time spent in orbit. Consisting of what equated to a 184-pound metal beach ball armed with a radio transmitter that was only capable of transmitting meaningless “deep beep-beep” sounds back to Earth (Dickson 2001a), we were able to learn about the density of the upper atmosphere solely through the drag that Sputnik I experienced as its orbit slowly decayed. Said drag was caused by Sputnik moving through the ionosphere’s plasma, and it was speculated that the charge required to achieve this drag could be acquired in the area of our atmosphere where the aurora borealis phenomena takes place (Warwick 1959). Alas, Sputnik was only able to help gather “basic” information like this until it burned up and was destroyed during re-entry. Thankfully for the United States, our first satellite was launched with proper sensors and as such was able to relay back to us data more complex than the density of our upper atmosphere. One of the most important discoveries Explorer I would have to be the discovery of the Van Allen radiation belt, and it continued to relay data on it for roughly four months before its batteries finally ran dry. The satellite continued to orbit the Earth until 1970, where it finally re-entered the Earth’s atmosphere (Dickson 2001b). It is interesting how the powerless mass of metal managed to remain in orbit for around 12 years, but I will touch on that later.


Now:


            We have made leaps and bounds in technological advancement in terms of satellites since the days of Sputnik I and Explorer I. As such, I feel that it would not hurt to go over the basics of satellites as they are now. According to Paleo, a satellite is “an airborne autonomous platform that carries a set of sensors to capture information on the surface of the earth, including vegetation, water masses, ice, and the atmosphere” (Paleo 2007). Satellites do more than just examine the Earth from up above, of course. They can also turn their attention to the distant planets and stars, even wandering out into the void to do so. They then technically become interplanetary probes, but seeing as how those are basically a subgenre of satellites I believe it is worth mentioning. Back on track, there are two kinds of sensors found on modern satellites: passive and active. Passive sensors are in charge of capturing the energy that is reflected by or emitted from a certain geographical area and of a certain wavelength; this is what is used to create an image of what is being captured. Active sensors send energy to the surface of the planet and then transmit whatever is bounced back to them. In general, active sensors are superior to passive sensors in terms of reliability; active sensors are not affected too much by weather due to using microwaves, whereas passive sensors are strongly limited by excessive amounts of clouds like those in storms (Paleo 2007).
Informative imagery such as this would be impossible if it were not for weather satellites.
            As for the types of satellites, there are three major ones: space probes, weather and observational satellites, and communications satellites. I already touched on space probes earlier; they function like regular satellites, yet instead of orbiting the Earth they wander the solar system and sometimes beyond to gather information that would normally be impossible to access. Weather and communications satellites share the similar trait of geosynchronous orbits, which in simpler terms means that they orbit in a way so that they are constantly positioned over a specific area of land. This practice is invaluable for weather satellites, for it is how weather channels are able to provide hour-by-hour weather time lapses; it would be a little more than awkward if one of said time lapses started in Michigan and ended in Wisconsin, now would it not? Being geosynchronous benefits communications satellites since it would be problematic if they wandered while transmissions were sent to or received from them. As for how communication satellites work, they have signals sent to them by stations or other locations and then reflect those signals to receiving stations or antennae. In either case, they are relayed to the consumer in the form of television or other form of media (Satellite transmission 2015).


Later:


            Not even a day ago I saw the descent of a satellite through the Earth’s atmosphere get mentioned on television. The satellite had already broken up into several pieces on the way down, with each piece engulfed in flame and leaving a brilliant trail of light and smoke. This is normally the fate met by satellites that outlive their usefulness: falling through the sky in a fireball reminiscent of a shooting star. Given how much surface area of the Earth is either uninhabited land or open ocean, most of the scrap metal that survives the descent ends up landing away from civilization. There are a few unlucky exceptions, however, such as the case of a particular home in the United Kingdom. One day in the July of 2009, an extremely hot, four-pound chunk of metal hurtled through the sky and crashed into a home in the town of West Hull, piercing the roof before stopping in the home’s attic. The owners of the home were assured that it was most likely a piece of a decades-old satellite that somehow survived re-entry, but the damage was done (Ernstein et al., 2012). In the future, we could find ourselves having to launch more satellites, and more satellites means more man-made meteoroids flying through the sky on their gradual but inevitable re-entry into our atmosphere. The odds of one of them hitting something is rather slim, but with more satellites you have more dice rolls and at least one of those rolls will eventually be a “winner”.
Looks harmless now, right? How about when it's traveling as fast as a shotgun blast?
            Abandoned satellites are not only a danger when they re-enter the atmosphere; they pose an equal, if not greater, risk to other satellites and manned space stations while above the atmosphere. Collision with a functioning satellite could very well put the unlucky satellite out of commission, and such damage caused to manned space stations is scary because of both this and the potential loss of life. Such a situation almost occurred in 2009 when the International Space Station was “buzzed” by a chunk of debris. At around five inches in size, it was like a makeshift cannonball travelling at speeds high enough that it would have burned up in the Earth’s atmosphere if and when it dipped lower. Some are able to celebrate the existence of this debris as relics of history, yet this debris is more than capable of killing an astronaut or puncturing a space station if either is in the wrong place at the wrong time (Ernstein et al., 2012). Again, this problem could be exacerbated in the future if and when we launch more satellites into orbit. I cannot help but think of WALL-E in this case; fictitious as it may be, having even a fraction of the movie’s amount of space debris in orbit is very concerning. As a countermeasure, perhaps satellites could be armed with explosives so that once they serve their usefulness, they could be reduced to smaller, easier to burn fragments of metal. This will take a lot of consideration, however, because this also turns something larger than that aforementioned cannonball into what is the equivalent of a field of grapeshot going at a speed that rivals sound through a vacuum until it starts to give in to the Earth’s gravitational pull.


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