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Showing posts with the label galaxy

Choosing Planets

Let's turn our imagination to the edge and do something different today. We can call it a thought experiment, a childish game, a daydream, science fiction, pure fantasy, or whatever we want, but let's move the boundaries far away from Earth, far away from our solar system, even farther from our galaxy, and do something wild.

Let's choose a planet.

Or, to be more precise, let's select one in the vastness of the cosmos and move away from this Earth and start new life. Of course, in daydreams we are allowed to do this just because the imagination is what our species differs from others on Earth.

Ok, to begin this little endeavor, we need a little astronomy to start with. What we know for sure is that our galaxy alone contains more than 200 billion stars, the majority of them not so different from our Sun, and by using a basic statistical study based on the planet finder's microlensing technique, there are approximately 100 billion planets orbiting them. Perhaps more. Multiply that by a factor of billions of galaxies in our universe, and you'll get that there are far more Earth twins out there than living people on Earth. There are planets for everybody's taste. So let's start with the planet's basic properties.

Choosing the World

It has to be huge, much bigger than Earth, maybe twice as big in size or even more, to harbor as many people as Earth today and still have plenty of room for many more. To be something like in Canada's distant regions today with only up to a thousand people per square kilometer. However, its composition must be radically different than Earth's, as, in my imagination, it has to maintain gravity more or less like the third rock from the Sun. After all, I don't like to move there and look ridiculously dysfunctional when it comes to, say, simple walking. So fewer heavy elements inside, please, and let it be around the famous, well-known number of 9.81. More or less. So no radical changes when gravity is in question, but I would choose the one with radically fewer water layers than we are familiar with within here. Don't get me wrong, I do like water, and I would like to have plenty of it all over the place, but with no oceans or large seas. Rivers are ok in any variety, lakes too, and small seas are also fine, but please no oceans. Nobody needs that. Hey, it's my planet; if you like oceans, find your own, or don't move anywhere; there are lots of oceans here.

Basically, there must be one giant continent in Norway's style with lots of rivers and lakes and small seas with large bays and calm weather. One rotation cycle could be a little longer than Earth's, but not so much over 30 hours. You can't get rid of old habits that easily. Like Earth, it needs to have a slightly tilted rotation axis to provide longer seasons and temperature changes over the year, with a revolution over the main star similar to the one in Mars or approximately twice as long as Earth's. Earth-like atmosphere and its greenhouse effect would provide a temperature range over the year to be a little milder compared to our native planet, maybe no less than -10°C in harsh winters and no higher than +30°C in summers. A tilted axis and position within the habitable zone of the mother star would also provide no big differences between the planet's equator and pole regions. What else? Oh yes, it has to be protected with both a strong magnetic field and a couple of perfectly positioned giant outer planets from both radiation and looney asteroids and comets. It could also be part of a binary star system, where the second star could also provide additional protection when it comes to violent cataclysmic events in the neighborhood. Last and surely not least, it has to be green all over the place. Extremely suitable for cultivation of various kinds of anything possible. The geography of the planet could be variable with both long valleys and mountains, just like in our home yard.

Humanoids by Star Trek "design"

Do you like my paradise so far? In a way, it was not hard to set the basic astronomical properties of the star system and planet itself. However, a bigger challenge comes with defining the demographics of the planet. You might not like it anymore after I continue and say that I would like the planet to be colonized without any domesticated intelligent species. Why? First of all, it wouldn't be right to find a desirable planet along with at least one dominating intelligent species already evolved there. It would be like colonizing the Americas and killing or putting the population into reservations. We've been there. It's just wrong. Secondly, and probably even more important, is that I would like to share it with other intelligent species. Preferably humanoids. Not mandatory, though. That way neither would be in a position to set a flag and say, "This is mine; everybody else is not looking like me; go away". Basically, in my vision, everyone intelligent who would like to come and build a house is welcome at any time as long as they sign some sort of "sharing" agreement. Something similar to the Antarctic Treaty System we are having here on Earth. Basically, the colonization idea would be comparable to the Earth back in dinosaur time, when all the aliens missed the opportunity to colonize it when no domestic intelligent species existed to claim it for itself. Or they didn't miss it at all, and we are actually them and have never been native to this planet.

So how would all that sharing look like, and what kind of civilization am I talking about? There are so-called Kardashev scales defining possible civilizations out there, dividing them into Types I, II, and III, and it, by definition, represents a method of measuring a civilization's level of technological advancement based on the amount of usable energy they have at their disposal. All three types are far away from the civilization of humans as we know it today, and all three are suitable as potential residents for my planet. By the way, let's call it in further text "M." Accidentally, although I first thought of my first name's initial, it is titled more accurately according to the planet's classification seen in Gene Roddenberry's Star Trek. Anyway, the point of using high-end civilization in my story is that young civilizations like ours are simply not suitable. Why? Several reasons, actually. First, it seems that a big amount of mutual tolerance is needed for the sharing principle I have in mind. All desirable intelligent species have to be evolutionary mature and unburdened by racial, religious, and any other interspecies differences. Additionally, the population must be technologically advanced. The system on the planet would be as simple as possible; there would be no countries nor any kind of political organization, no governments of any kind, nothing like on the third rock of our solar system. There will be just one institution, planetary-based, with just one treaty where all colonists have to sign, and it should be pretty simple. If you want to live there, you would have to choose the land that is free and yet unoccupied, claim it yours, and the only condition to keep it is to produce zero waste outside of its boundaries. Otherwise, you can do whatever you want with it—create your dream house, build a school, trade market, entertainment facility, anything at all—as long as you play fair in relation to others.

ISS 3D Printer and first 'emailed' socket wrench

There will be no cities, as the technology at everybody's disposal would provide transportation to the most distant part of the planet easily, safely, and fast. I see smaller settlements, though, based on their mutual benefits and relations. There will be no sports, at least not in the form of the ones we know on Earth. It would be extremely unfair to play, for example, basketball involving multiple species with different masculine properties. However, the technology sports would survive, like races or any kind of recreational activities. Advanced technology in everybody's home would provide planetary and interplanetary networks of various communications; there would be no need for many supporting factories except for basic ingredients, as home computers would be equipped with state-of-the-art 3D printers capable of producing both simple tools and complex machines. The same home computer would also be able to use food replicators for creating food and food supplements. I don't like the existing concept of killing other species and using them for food. Cultivation and planting are perfectly ok, and each household would possess its own greenhouse for growing appropriate food, but I expect high-end civilizations in evolutionary terms would solve "the meat" problem, and I am not talking about a vegetarian diet.

Of course, the main star system would be well explored, with several outposts built for several purposes, along with mining outer moons, other planets, and asteroids in search of all necessary ingredients for planetary life, along with a variety of orbital activities for planetary residents, including entertainment.

Unfortunately, choosing a world to move is still just a dream. Reality still resides far in the future. Nevertheless, I wonder if such a world already exists out there in a far, far... You know.

Image ref:
https://3dprint.com/32269/made-in-space-emails-wrench/

Refs:
http://hubblesite.org/newscenter/archive/releases/2012/07/full/
http://en.wikipedia.org/wiki/Antarctic_Treaty_System
http://www.nasa.gov/audience/foreducators/k-4/features/F_Measuring_Gravity_With_Grace.html
http://en.wikipedia.org/wiki/Kardashev_scale
http://en.wikipedia.org/wiki/Class_M_planet
http://www.imdb.com/name/nm0734472/

Solar System Weirdness

Do you know how big our solar system is? I can't be sure, of course, but there's a strong possibility that common knowledge about our planetary neighborhood ends with enumerating most of the planets—one dwarf planet and a couple of named moons, asteroids, and comets. Amazingly, the truth is far, far beyond that, and believe it or not, if we include Oort cloud, the solar system, with us representing its only living residents, is approximately 3 light years in diameter. This is, more or less, equal to 3e+13 kilometers or 30.000.000.000.000 km. The distance is about 100 million times bigger than the distance to the Moon. It is tremendously huge and just about one and a half light years shorter than the distance from our sun to the nearest star!

The layout of the solar system*

So next time when you, through your polluted sky, look up and see the Moon, Venus, Mars, Jupiter, and occasionally some comet tail or shooting star, remember that what you see is just a fraction of all the weirdness of everything that is gravitationally bonded to the Sun and to each other. So let's see what we don't see with our eyes and check out some weird places, some of them not so far away from our own Earth. And just to be clear, the words 'weird' and 'weirdness' I added in the title and throughout the post are here more for theatrical reasons. Surely, the fact is that what's weird to me and you is only natural behavior and property of the physics of the solar system. We are just trying to understand it.

In such a way, let's start with the first and probably the oldest mystery of the orbiting laws around the Sun. Back then, in the 19th century, French mathematician Urbain Le Verrier tried to study Mercury's orbital motion around the Sun in order to post an orbital model based on Isaac Newton's laws of motion. It happened almost a century before Einstein's theory of relativity, which is a current, state-of-the-art mathematical model of gravity and orbital physics, but back then, Verrier's model simply failed to match the observations. In short, Mercury refused to spot itself on predicted spots on the skies, and in every orbit, its perihelion (or orbital spot where the planet is closest to the sun) moved away from predicted places by a small amount. Unfortunately, instead of doubting the equations, like many times before and after in the history, Verrier posted a theory of a new planet or a large orbital body 'inside' Mercury's orbit that might be responsible for Mercury's misbehavior. He even proposed the name 'Vulcan' because of it's potentially very hot orbit so near the Sun. This triggered a series of searches for the Vulcan, and until Einstein came up with the theory of relativity (and it's predictions of heavily banded space and time continuum near the heavy objects) that perfectly explained all the observations of one system so close to the massive Sun observed from the distance, many professional and amateur astronomers claimed that they found the Vulcan and spotted its transit over the main star. Perhaps the final dots to the mystery posted SOHO and STEREO solar missions, and neither of them found anything planetoid-ish inside Mercury orbit. Recent calculations go even further and rule out any asteroid, revolving around the Sun inside Mercury's orbit, that is bigger than 6 km in diameter.

Lagrange points *2

The next weirdness of the gravitational three-dimensional geometry of the solar system (and all the other star systems out there) are called Lagrange points. Physics was observed and defined by the great Italian mathematician and astronomer Joseph-Louis Lagrange in the 18th century. He identified five points in the orbital system of two massive bodies from the perspective of a third small mass. In short, if we consider, for example, Sun and Earth, there are three points on the connecting line between the star and the planet (L1, L2, and L3) and two more, L4 and L5, positioned on the top of equilateral triangles where two other vertices are occupied by Sun and Earth. Now, what is special about these places is that small objects positioned in those points would be able to maintain a stable position relative to the large masses. If you check the image to the left, a small rock positioned in point L1 would be able to revolve the sun with the same orbital period as the Earth. The same goes with the other four points. However, the first three points are pretty unstable, and objects positioned there would tend to fall out of orbit due to gravitational potential energy shown on the image as well with red and blue arrows. L4 and L5, on the other hand, are completely different stories, very stable, and while a spaceship parked in the first three points would need to fire engines constantly in order to stay put, the same spaceship in L4 and L5 would be able to shut the engines down and park it there for eternity. Think of it like the 'egg vs. equinox' myth: even though you can balance the egg on short or narrow ends (and not just on equinox), this position is pretty unstable, and even a little vibration would knock the egg out of balance. Similarly, L4/5 points would be like putting the egg in the eggcup. Scientifically speaking within the Earth-Sun system, L1 is very interesting as the point of monitoring the Sun without any orbital interruptions (SOHO is located there), L2 is a great place for orbital telescopes (Planck and James Webb Space Telescope), and L3 is pretty useless as it is always hidden by the Sun and therefore the origin of all science fiction stories with counter-Earth located in that very point, sharing the orbit with us while we would always be unable to see it. Of course, there is no planet on the other side of the sun; otherwise, we would detect it's gravitational influence. However, if some aliens exist on the mission of monitoring humankind, they would pretty much choose this place to hide their mother ship.

Of course, the solar system is crowded with plenty of large orbiting objects, and Lagrange points, i.e., the Sun-Earth system, are not really points per se, and due to gravitational influences of other planets, they vary in position depending on the current positions of other planets in their orbits. Same goes for the Lagrangian system of Earth-Moon with their L4/5 points, for example, suffering additional complications due to influence of the Sun. But still, these points are ideal for some futuristic space cities orbiting the Earth, and some 40 years ago, Carolyn Meinel and Keith Henson founded 'The L5 Society' around the idea of Gerard K. O'Neill to build a colony that would be positioned in tiny orbit around the L5 point in the Earth-Moon system. In addition, there are also plans to use L1 and L2 points in the system to build Lunar elevators with appropriate counterweights and 'cables' with the use of materials that already exist in production today since they don't require a lot of strength in the process.

Jupiter and inner-solar system asteroids *3

Lastly, and the absolute winner in the weirdness competition of the solar system related to Lagrange points is Jupiter and it's L4 and L5 points, or in this case regions. Due to the nature and stability of the orbits within, Jupiter is using them as a, well, sort of, garbage collector. Believe it or not, these two regions are the home for more than 6,000 asteroids. They all travel around the sun with the same speed as their father, Jupiter. By astronomical convention, these asteroids are named after the Trojan War, and therefore the entire regions are called 'Jupiter Trojans'. Surely, the three largest asteroids in there are conveniently named Agamemnon, Achilles, and Hector, and the region around L4 is called the 'Greek camp', while all the others in L5 belong to the 'Trojan camp'. Other planets also collect junk, dust, and small and big asteroids in their L4/5 points, and even Earth owns one (discovered so far). It is a rock 300-meter-diameter orbiting the Sun along with Earth in L4. There are also space rocks detected in Saturn's moons and their L4/5 points, as well as the dust detected in the moon's. It will be interesting what we will find in the (far) future when we start exploring the solar system for real. Lagrange points will surely be on the top of all lists to explore, study, and use. I am more than positive that lots of L4 and L5 points throughout the solar system will be used for various space lighthouses, radio beacons, and a wide variety of communication devices. Besides the large number of asteroids caught by Lagrange, there is one more group of 1000+ asteroids gravitationally bonded with Jupiter. Their name is Hildian asteroids, and they are in so-called orbital resonance with the solar system's biggest planet. In this case, it means that Hilda's aphelion point (the farthest distance from the elliptical center) is in resonance with the planet, and on every third orbit it is positioned directly opposite from Jupiter. The story with inner system asteroids doesn't end here, and if we travel a little bit inside the Jupiter orbit from Trojans and Hildas, soon enough we would stumble into a famous asteroid belt with more than a million rocks larger than 1 km in diameter. At the beginning of the 19th century, among certain groups of astronomers, including Heinrich Olbers, was very popular so-called Bode's law, stating that each planet in any star system would be approximately twice as far from as the one before. Remarkably, it fits nicely in the solar system with the exception of Neptune and the planet between Mars and Jupiter. Bode initiated a search for the planet to confirm the theory, and when during the years 1801 and 1802 Ceres and Pallas were found in more or less the same orbit, Olbers suggested that they might be remnants of a large planet named Phaeton. The theory flourished in later years, especially after the discovery of other belt's large and small asteroids. Today we know more about asteroids in the belt and their composition and mass (which is around 4% of the mass of the Moon), and the current theory is that Phaeton never existed and that it was more likely that it was never formed due to heavy attraction from nearby giants. Nevertheless, both Vulcan and Phaeton continued to live in the sci-fi realm and also a couple of mythologies.

If we continue our travel toward the outer edges of the system and pass four gas giants, around 30 AU starts another belt full of heavy objects. Actually, astronomers identified two separate sub-systems, one named 'Kuiper belt' and the other 'Scattered disc'. Just like the main 'inner' asteroid belt, they contain many rocky objects and dwarf planets, with Pluto as the most famous one, but also objects composed from methane, ammonia, and water ice. Scattered disk can be described as an elongated subset of the Kuiper belt containing objects with highly eccentric orbits, like short-period comets that orbit the Sun in less than 200 years. The best-known comet from this bucket is no doubt Halley's Comet. Kuiper Belt was discovered only recently, in the late 20th century, and its discovery needs to thank big time to conspiracy theorists and scifi writers. Actually, after the last gas giant Neptune is found by following the lead of the deviations in Uranus orbit that were caused by Neptune, the same lead is pursued further, following similar perturbations in Neptune's orbit. This directly led to the discovery of Pluto, but as soon as it was found that its mass wasn't enough, the search continued further, and many were sure that there was another big planet further away, conveniently named Planet X. In the fiction, its name was 'Nibiru' with connections to 'ancient astronauts' theorists who gave it an orbit of 3600 years with a pure doomsday scenario, as once in a while it crosses with Earth's orbit and creates a living hell and pretty much the end of life as we know it. Of course, this was just another nonsense and pseudo-science, but eventually, and most thankfully to astronomer and unofficial father of 'Kuiper Belt', Mike Brown, who discovered lots of small trans-Neptunian objects beyond Pluto, we today know a great deal about Kuiper Belt, and in this regard, I will just quote Mike Brown: 'Eris (the biggest TNO along with Pluto so far), and Pluto and all of the rest of them have only a trivial impact on our solar system. You could get rid of any of them (I have a vote which ones, too) and nothing much would change.' Recently, with more precise measurements of Neptune's mass, new calculation of its orbit accounted for all observed perturbations and deviations. However, this didn't mean Planet X doesn't exist. The new theory just pushed it more beyond toward the edge of Solar system and it earned new name. This time it is called Tyche and it's location might be somewhere in Oort cloud. But before we encounter this final system's weirdness, let's first see what happens just after Kuiper belt in the very region where couple of man-made robots are currently still flying!

Solar system Heliosphere *4

Gravity is of course the main property of any star system, but from the 'weird' point of view, our path brings us to the region of the solar system, just outside the most eccentric orbit from the swarm of all objects within the scattered disk. And it has nothing to do with rocky objects, tidal forces, or orbital physics. It's name is heliosphere, and it's the first boundary of our system we can positively identify. This is the real edge of the system, where ultimately solar winds finish their travel. Solar wind represents ionized particles emitted by solar corona, and they start traveling at around four times the speed of sound in the interstellar medium. Geometrically speaking, the heliosphere is actually a bubble around the sun and all the planets and other objects, and it starts from the point where solar winds, due to interaction with solar system particles, slow down to the subsonic speed and end at the point when they fully stop, or more precisely, reach pressure balance with the interstellar medium. What is interesting about the heliosphere bubble is that it is not really spherically shaped. The sun is traveling around the center of the Milky Way, and this bubble follows, forming a comet-like shape with a tail called a heliotail, composed of particles that escaped the heliosphere, slowly evaporating because of charge exchange with interstellar media and particles from other stars. It was also speculated that throughout solar system travel, the front edge might create a turbulence edge, a bow shock, similarly to the meteors or satellites that enter the Earth's atmosphere and burn on top. The bow shock is still not confirmed, and perhaps it doesn't exist as the sun might not travel with enough speed to form it. But it is observed in the motion of a star system called Mira, red giant in the constellation Cetus by GALEX, an orbiting ultraviolet space telescope in the previous decade. Thanks to both Voyagers, we today know more about the composition and pressure of interstellar gases. Voyager 1 already 'crossed' the heliosphere edge, while Voyager 2 is still inside in the so-called "Heliosheath" region.

However, if solar wind stops at the outer edge of the heliosphere, the sun's gravity goes on and influences much further. The proposed boundary where the sun's gravity weakens and loses its dominance is at about 1.5 light years from the sun. This edge is also the edge of the theoretical Oort cloud, a spherical disk filled with remnants of the original protoplanetary disc from around the Sun at the time of solar system creation, about 4.6 billion years ago. Due to the large distance, it is suggested that it might contain objects captured from other stars from the time of the 'birth cluster' or the beginning of the solar system and other systems while they were in the process of departing from each other. Oort cloud, even not scientifically confirmed today, could start with its inner circle at about 2000 AU or so. One day, when Voyager 1 reaches the region (in about 300 years), it would need another 30000 years to pass it through entirely. Unfortunately, V'Ger will not be operational by then (unless something happens to it's power source, like in the first Star Trek movie from 1979). The Oort cloud is so big that it's outer circle is not only influenced by the sun's gravity alone but also by the gravity of nearby stars as well as all the influences by tidal forces of the entire Milky Way.

Imagined view of the Oort cloud *5

In a nutshell, the Oort cloud is one giant swarm of icy objects and the potential source of all long-period comets. It is also suggested that many, if not them all, short-period comets originated also from the Oort cloud and were captured by gas giants, especially Jupiter. The story of long-period comets is the one responsible for the new planet X location, or Tyche, I mentioned before. Some 15 years ago, astrophysicists John Matese, Patrick Whitman, and Daniel Whitmire proposed a theory that long-period comets, instead of coming from Oort clouds in random orbits, caused by gravitational perturbations originated in galaxy tidal forces, might be fully clustered and notably inclined to orbital panes of planets. As the solution to this clustering or grouping of long-period comets, they proposed the existence of one giant planet inside the Oort cloud that is either similar to Jupiter, only 3-4 times bigger, or even a brown dwarf, a failed star that would count our solar system as a, sort of, binary star system, which are the most common systems in the galaxy. However, this theory, even though the most plausible of them all encountered, to add more big planets into our solar system, lacks enough data to spot clusters of long-period comets as their orbital periods are in the realm of thousands of years. Additionally, within the Wide-field Infrared Survey Explorer space telescope mission and its all-sky infrared survey data, no such dwarf or big planet was found. Even more, WISE ruled out the possibility of a Saturn-sized object at 10,000 AU and a Jupiter-sized or larger object out to 26,000 AU. If it still exists, Tyche might be even further away, which also might mean that it could also harbor large moons of its own. Another bold theory, but more likely, is that it doesn't exist at all, and we just need to learn more about Oort cloud complex physics to understand it fully.

I will be careful while concluding anything substantial out of this post. The fact is that I am not a real scientist or astronomer and definitely not a conspiracy theorist or pseudo-science admirer. To be on the safe side, I can say this: posting new theories in astronomy and cosmology from the surface of Earth is way easier than confirming them. We are talking about a vast region of space, and while astronomical instruments, along with science itself, are more sophisticated and better every year, I have no doubts that the real breakthrough in this realm will come only when we eventually rise up and approach closer 'and see' for ourselves. I also have doubts that this will not happen any time soon, especially not in my or your life span.

Until then, metaphorically speaking, we will continue peeking out of the window and doing math from the distance. And continue to dream about wonders and weirdness of the heavens, waiting for us to come, see, and finally understand.

Image credits:
* Credit; Charles Carter/Keck Institute for Space Studies
   https://exoplanets.nasa.gov/news/1400/interstellar-crossing-the-cosmic-void/
   http://www.universetoday.com/32522/oort-cloud
*2 http://map.gsfc.nasa.gov/mission/observatory_l2.html
*3 https://en.wikipedia.org/wiki/Jupiter_trojan
*4 http://sci.esa.int/ulysses/42898-the-heliosphere/
*5 http://www.sciencemag.org/mysterious-oort-cloud-objects

Refs:
http://motherboard.vice.com/blog/new-planets
http://www.scientificamerican.com/article/astronomers-skeptical-over-planet-x-claims/
http://www.universetoday.com/89901/pluto-or-eris-which-is-bigger/
http://news.discovery.com/space/alien-life-exoplanets/mike-brown-planetx-pluto.htm
http://voyager.jpl.nasa.gov/where/
http://physics.stackexchange.com/questions/36092/why-are-l4-and-l5-lagrangian-points-stable
http://www.astrosociety.org/edu/publications/tnl/62/equinox2.html
http://www.nss.org/settlement/L5news/L5history.htm
https://en.wikipedia.org/wiki/L5_Society
https://www.nasa.gov/content/nasa-s-ibex-provides-first-view-of-the-solar-system-s-tail
https://en.wikipedia.org/wiki/Michael_E._Brown

Celestia, Campfire and Astronomy

I remember every little detail from that weekend trip. From the very first moment when we stepped into the bus that took us to the mountain base, throughout the rest of the first day when we climbed down into a small cave with narrow hallways toward the small chamber at its end. I vividly remember the glorious, endless, and hard-to-find second cave we stepped in the very next day, followed by an overwhelming feeling and little fear when we passed through cave chambers, cutting the darkness with handy tools and small flashlights. I will always hate myself for not having a camera to capture the surrounding scenery when we traveled by train later that afternoon, which looked like it came right out of the 19th century with wooden benches rolling the railways slower than Usain Bolt. All those rock formations and abandoned train stations were slowly losing their battles with nature and were looking exactly like a background from Sergio Leone's spaghetti western movies.

Viktor at Rundetårn observatory, Copenhagen

But what I will remember the most is the first camping night between the caves. It was an extraordinary experience only a campfire can provide.

It was the hot middle of the summer, and the forest was mysterious and kind at the same time. I don't remember the exact year, though, but it surely was during my late teenage years, most likely in July or August of 1987. Along with a couple of my peer friends, I was lying down in the middle of a forest clearing on top of my brand-new sleeping bag, hypnotically staring toward the nightly sky. I glimpsed the watch and saw that midnight passed just an hour ago. The campfire was vividly glowing around the small glade surrounded by dark trees. It was the perfect time, and soon it was about to begin. As planned, the first one came on schedule, leaving a straight line in the sky for a millisecond or two. Shortly after, another one fractured the nightly sky, then another one and another and another...and then it was a shower. The Perseids. The icy fragments entering the Earth's atmosphere every summer are body parts of the comet Swift–Tuttle, which travels in this neighborhood every 130 years, providing lots of meteors for our camping TV. That particular year we planned our adventure by the moon's motion, or, to be precise, we wanted to go on the trip when there was no moon in the sky most of the night during its crescent phase. Without light pollution from the Earth and the Moon, the sight was amazing—perseids, thousands of stars, nebulas, galaxies and planets, the Milky Way in the center of our view, planes, and artificial satellites passing by throughout constellations with their leader of the time—the Russian space station "Mir", which was probably one of those brightest moving dots we saw that night. If you didn't see such a sight, you would be surprised how the night sky is actually dynamic. If you add to the scene strange sounds coming from the surrounding forest made by sleepless birds and wild animals, you get perfect entertainment for the big portion of the night. It was our first camping trip, and the fear of the unknown a little spoiled the event, but in our defense, without any experienced guides or team members, I can assure you that every suspicious sound that came from the forest sounded like the ultimate wild predator hungry for young humans. Anyway, little because of the fear and much because of active heavens, we finally fell asleep a little before dawn and successfully slept for an hour and a half, ready for the next day.

Space station Mir (1986-2001)

That really was one great summer, and this trip would stay on top of my adventurous history, from many perspectives. But it wasn't the one that triggered my interest in science and astronomy. I couldn't say what it was for sure, and probably, among many things, at the very beginning, it was one scientific toy my parents bought for me when I was really young. It was one toolkit box**—an optical set of plastic parts and various lenses allowing you to build different gadgets such as a microscope, binoculars, a spyglass, a kaleidoscope, a diapositive magnifier, prism tools, etc. It was my favorite toy for many years. The other equally important trigger is my failure to comprehend the word "infinite" and my everlasting desire to understand its meaning. It was bugging my mind ever since I started to look up at night. Even today, after dozens of courses of various mathematics I had to pass during my high school and university education, infinity is staying the biggest unknown, lying right there, far beyond my scope. There were years in my youth when I was convinced that infinity actually doesn't exist at all. I loved the idea that the cosmos is curved to 360° in all directions. I desperately wanted to believe that if you go with your spaceship straight up, eventually you will reach the same spot only from the opposite direction, just like the surface of Earth and its two-dimensional fully closed curve. Of course, today within the mainstream scientific thought there is much evidence that the expansion of our universe is real, but still it doesn't solve the infinity of it. At least in my mind. Even though the probable fact that our universe is just a part of a multiverse neighborhood where our cosmos is expanding into something bigger, to me it is only stretching the infinity out, only this time far beyond our borders. Maybe one day we will find the definite answer.

From the other perspective, if we are looking at the 'infinite' trouble only from our rational mind, we have to admit that the human race is extremely young, evolutionarily speaking. The real handicap is that we are living in a 'finite' world. Everything that surrounds us has its beginning and the end. At least it seems so, and even though we today learned a great deal about our position within the celestial realm, we only scratched the surface of it. We only managed to set a foot or two (or 12 to be exact) on the Moon, and we only started to explore our own solar system. Due to our own limitations in the form of our unwillingness and hesitations to deal with the unknown and/or our own animosities for each other in the form of militant behavior throughout our history, this is still a very slow process, but inevitably, one day, in the not-so-far future, the time will come when, lackingenough energy to sustain humanity as we know it, we all will have to start looking up, not for searching for the divine but for our own pure survival. Then our own evolution will speed up and skip some gears toward answers to many inconceivable questions.

Night Sky and Perseids by Brad Goldpaint (Goldpaint Photography)*

Anyway, astronomy is one of few scientific playgrounds simply because it contains many unanswered questions. There are plenty of proposed theories that will surely stay in their theoretical phases for many years until we finally get ultimate proof. It is entirely based on studying electromagnetic radiation we are picking up on the surface of Earth and several instruments in orbit. All possible frequencies within electromagnetic radiation are telling us many stories from its origin point and the path it is traveling through. Of course, studying full spectrum requires big and even large instruments in both size and money needed for their manufacturing. Especially if they require being lifted into orbit in order to avoid atmospheric disturbances. Secondly, it is amazing what must be done in order to look up one particular spot in the heavens simply because everything in the cosmos is in motion. We need to solve the rotation and revolution of the planet and, if posted in orbit, compensate for the extremely fast speed of the spacecraft carrying the instruments. As the monitoring object is farther away, the less amount of radiation is picked up by the sensors, so astronomy is one of those indirect or asynchronous sciences where we need to collect the data for some time, which could be years or even more time, and then for an equally considerable time analyze the data, compare the resulting images, and conclude science out. For example, take the Kepler orbital space laboratory. It orbits the Sun following the Earth in order to get a clear view toward the monitoring stars, and it is simply continuously taking images of 'nearby' stars (about 145,000 stars) and sending the data to the Kepler team for analysis. Over time, the team and their sophisticated software measure slight brightness changes during possible orbits of potential planets, and only by these small changes in brightness of the main star is it possible to roughly determine the size and orbit of the planet causing the dimming of the light from the star. However, in order to get all those facts out of the data, Kepler must take lots of images and cover the planet's full orbit. That means in order to confirm the planet, Kepler must take at least two images separated by time in order to confirm the revolution time of the planet. It's a slow process, and considering lots, and I mean LOTS, of received data, I am sure we will hear about more and more planets found by this technique.

Among all possible wavelengths within the full electromagnetic spectrum, the coolest one is the one situated between infrared and ultraviolet waves. The greatest visible light. The one we can see. Even though it is just a tiny portion of the full spectrum, this is the one we can enjoy with our own eyes. This is the one we see every night we look up toward the amazing heavens. Thanks to relatively cheap optical instruments, we are able to enhance the view and zoom it in and see further. Some time after I enjoyed my optical set toy I mentioned earlier, I got my own first refracting telescope. It was small without any tripods and fully mobile, but looking at the moon for the first time was something I will always remember. Discovering the fact with my own eyes that Venus, like the Moon, also has phases and seeing it in its crescent shape was the next best thing I experienced. I still have it, and every time I grab this small piece of optics, I can't help myself and instantly remember the times when I was fixing it on the ladder positioned on the top of our garage and spending hours looking toward the stars.

Transit of Mercury over Sun by Sky-Watcher 150/750

Today I have in my possession an educational reflecting telescope with a respectable mirror size and focal distance mounted on an equatorial tripod along with a motion tracking system capable of fixing the spot on the sky for hours. Unfortunately, amateur astronomy requires lots of free time, which I regretfully don't have enough of. In addition to a lack of free time, watching the heavens requires an unpolluted environment, and life in big cities is beneficial for everything but astronomical observation. Sometimes I feel like that character from the Michael Keaton movie—I don't remember the title now, but in the movie he found a way to clone himself in order to get finished various tasks in his life... Similarly, I would like to have one me for work, one for astronomy and science, one for family and writing... Simply, the day is too short, and to support the family and life, the work is always number one. But it is a good thing to have spare moments and spend them in the most enjoyable way. Even today, from time to time, I point the scope up and peek a little. Sometimes I take photos out, like this one of Mercury transiting the Sun disc.

To conclude with some short 'observations', if you want to do some amateur astronomy, you will need star maps. Before they were black and white and printed in the form of atlas books. Today all that changed with the speed of the internet and graphic tools on the average personal computer. They are all online, and you can access them with many apps. I recommend 'Celestia' and 'Stellarium'. Even without a real telescope, they provide endless fun.

Image refs:
https://amsmeteors.org/2017/08/viewing-the-perseids-in-2017/
https://goldpaintphotography.com/

Kepler project:
http://kepler.nasa.gov/
http://www.youtube.com/watch?v=54fnbJ1hZik

** Toolkit box (~1978):


Refs:
http://en.wikipedia.org/wiki/Perseids
http://en.wikipedia.org/wiki/Electromagnetic_spectrum
http://www.shatters.net/celestia/
http://www.stellarium.org/