Black Hole

When I was a kid, I struggled to understand the meaning of a “black hole”. I was baffled how an object can suck in everything around it and never be full. In elementary school, my science teacher told us that “your chair were to contract indefinitely, it will become a black hole that will be so small that you will not even be able to see it; however, it will continue to attract everything into itself – including you, who is sitting on that chair right now – forever. 

A black hole is the leftover of a high-mass dead star. For a low-mass star (like our Sun), after its death, it will contract until its core is completely made of carbon, at which point the heat will never be high enough to perform fusion, and the dead body of the star – a sphere of carbon – is called a white dwarf. A medium mass star will become a neutron star on its death. However, for an extremely high mass star, its gravitational collapse will become so strong that it will cause a glorious explosion – supernova – and the leftover core will be indefinitely massive – so massive that all the mass will gather in a point (singularity) and its gravitational force will suck in everything around it. The radius in which every matter including light will be sucked in is called the Schwarzschild Radius, where the escape velocity is the speed of light. In other words, everything that has a speed smaller than or equal to the speed of light will not be able to escape the black hole.

Thus, what my teacher told us in elementary school is somewhat correct. Even though the original mass of the chair is so small that it would only create a Schwarzschild radius of little more than 0, it will still be able to consume whatever is within that radius.

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Stars of Revelation

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Throughout the Bible, celestial bodies are mentioned. Jesus is “The Morning Star.” Abraham would have as many offspring as stars in the sky. Another example many people are familiar is the Book of Revelation in the Bible. It was also mentioned in my discussion of the tilma of Our Lady of Guadalupe. In Chapter 12, Verse 1, the woman whose head was crowned with 12 stars is mentioned. The Church Fathers interpreted this lady as Israel and the Church, the comparison between the Old Testament and the New Testament. It is also commonly inferred to be Mary, with the 12 stars being the tribes of Israel and/or the 12 apostles. But it is touching to me, personally, because stars are a beautiful thing we sometimes take for granted. But to gaze out at the night sky and have it dashed with splashes of light is wonderful to me. They are a part of the beauty that is creation, all of which bows to God and heaven. And Mary, as Queen of Heaven, is venerated and loved by all of creation. As such, she is the pinnacle of heaven, and deserves to be crowned as such. I find it so wonderful for her to be crowned with the jewels of the heavens. Furthermore, these 12 stars were further expanded in the Baroque Period to be 12 privileges and charisms of Our Lady as a special devotion, which I think is beautiful. I just find the imagery utterly glorious, and I hope you all can appreciate it as well. Au revoir, my friends. (University of Dayton)

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Blog #7 Extremophiles

Photo of an extremophile water bear captured using an electron microscope.

Extremophiles are creatures which are capable of living in extreme environments beyond what one might imagine are the limits of life. Extremophiles have attracted attention from the scientific community because of their potential to exist in the most extreme environments in outer space. One specific type of extremophiles, halophiles, are able to survive in highly saline environments with the ability to thrive in places such as the Dead Sea. These organisms are able to balance the salt levels in their cells in order to survive extremely salty conditions. Another type of extremophile, the thermophile, is capable of living in the extremely hot temperatures upwards of even 60 degrees Celsius. Extremophiles could be the most important organisms we have here on Earth for the field of astrobiology because they demonstrate how life might exist in extreme environments on other planets. Adaptations shown by extremophiles could potentially be used by scientists here on Earth for biotechnological improvements in salt-tolerance and heat-resistance. More extremophiles are likely to be discovered in the coming years leading to even more developments in the field of astrobiology.

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Thermophiles on Venus

Venus Cloud Temperatures

Thermophiles are a type of extremophiles that can survive above 45 degrees Celsius. These organisms are usually bacteria, and here on Earth they are found in hot springs.

I wanted to talk about the possibility of life existing on Venus, not on the surface (it is far too hot there – 475 degrees Celsius). But, instead the life could possibly exist in the perpetual clouds above the surface. Above are the temperatures that these clouds get to be. It is hypothesized by scientists that these clouds are cool enough (in reference to the surface temp) that these thermophiles can exist.

I think this is super interesting because it expands our parameters of what conditions life could possibly survive in. It allows us to question if intelligent life could evolve from these bacteria in other solar systems, and it could even change what our definition of what intelligent life could look like on other planets; it may not (and is most likely) to not even look humanoid at all! Isn’t that interesting? 🙂

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Drake Equation

How many civilizations are there in our galaxy? As a kid, I was awestruck by the knowledge of just how small we are as compared to the universe. The concept of “me” is nothing more than a tiny stardust living in 1 of the 100 billion star systems in our galaxy. However, if there are 100 billion stars in the Milky Way, how likely is it that there are millions of civilizations out there just like us? I have always thought that there would be no way of knowing this, since how can we detect new civilizations if we cannot even fly out of our solar system? However, the Drake Equation might help us get an estimate of this question that we, as a species, may never know the answer to.

In 1961, an astrophysicist named Frank Drake developed the “Drake Equation” to provide an estimate of how many detectable civilizations there are in our galaxy. In this equation, we can fill in a series of variables to get an estimate, N, that represents the number of civilizations. 

The uniqueness of the Drake equation is that instead of asking the question, “are there civilizations out there”, it asks, instead, “are there any other technologically advanced species other than humans that has ever existed in the galaxy”. What I loved most about the equation is the “L” factor, which stands for the length of time a technological civilization can stay for. For my estimate, I used the length of the dinosaur – 165 million years – as the estimate, optimistically hoping that we as a species can sustain as long as the dinosaurs have. Another interesting addition to the Drake equation can be a “recurrence factor”, where we include the probability of a civilization repeatedly happening on a planet. 

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Seager Equation

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So the Seager Equation was made to mimic Drake’s Equation. It doesn’t find communicable aliens, but rather just that life which is detectable from Earth. It also doesn’t specify intelligent life, so it searches for any discernible life at all, from microbes to megafauna. The equation goes like this:

N* : Number of observable stars x

FQ : Fraction of those stars with minimal activity x

FHZ : Fraction of those stars with rocky planets within the habitable zone x

FO : Fraction of those planets that can be observed x

FL : Fraction of those that have life x

FS : Fraction of those that produce gaseous bio-signatures =

Number of planets observable planets with life. (Ghost Theory)

There are some obvious practical concerns with this equation. The number of observable stars is a tough number to get a hold of. Although there are around a septillion number of stars in the universe, we can only see a fraction of that. The mission Gaia is monitoring around 1 billion stars, so it is definitely at least that many. (Space)

Those stars with minimal activity includes those with infrequent and small solar flares and radiation expulsions. These large radiation bursts would destroy atmospheres and any hope of life forming.

Planets with gaseous bio-signatures would include, likely, a significant portion of oxygen. But the limiting factor here is that we assume life would produce large amounts of oxygen, which is not necessarily true. That is only if they use similar processes to our own. Gaseous water is also likely, but again that assumes Earth-like analogs. So any guesses we have are purely from the Earth standpoint.

Essentially, we have a start for how to start looking for life, but we won’t ever be certain until we find it. Life is extremely adaptable, and can take many possible forms. So to narrow down what life would look like is extremely hard. But if we were to find life on Titan or Europa, a lot of our current assumptions may change.

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The Apollo 11 Quarantine

The Apollo 11 Astronaut Quarantine

When Neil Armstrong, Buzz Aldrin, and Michael Collins returned from space after the Apollo 11 moon landing, they were immediately placed into a quarantine. This was the first manned mission to the moon, and the scientists weren’t sure if there would be any dangerous particles on the moon that the astronauts might bring back to Earth. In fact, the astronauts were surprised at how much moon dust stuck to the mission components. The regolith “went everywhere and attached itself to everything in sight.” Nobody was positive how toxic the dust would be, so to be 100 percent safe, the astronauts were placed into quarantine.

The secondary reason for the astronaut quarantine was due to the possibility of alien microbes attached to the dust. Nobody was sure if there was any life on the moon yet. Extremophile bacteria had already been observed surviving in environments similar to space, so it is not too outlandish to suggest that microbes could survive on the moon. It is also technically possible that these microbes could make it back to Earth on an astronaut. So, the quarantine is designed to protect people from any possibly dangerous microbes as well as protecting the possible microbes themselves so that they may be studied.

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Fermi Paradox

When ordinary people ask, where are the aliens? We usually just laugh it off and take it as a joke. However, when this sentence is uttered from the mouth of a scientific authority, it becomes a question that is terribly thoughtful. The sun is a relatively young star, which means that there are terrestrial planets that are much older than the earth. In theory, their civilization should be far more developed than ours. Earth is 4.54 billion years old. Assuming we compare with a planet P which is 10 billion years old. If P’s experience is similar to that of Earth, their civilization should be 5.46 billion years ahead of us. Their technology will be beyond our comparison. This gap is like the monkey seeing human civilization. So why haven’t we discovered alien civilization so far?

One explanation for the Fermi Paradox is that alien civilizations tend to self-destruct before making contact with other civilizations (such as Earth). e.g. climate change, nuclear war

Another explanation is that intelligent civilizations are rare, either because the conditions necessary for the evolution of intelligent life are scarce, such as humans needing oxygen to live.

Or the alien civilization has received the signal sent by the earth, but they may not reply to us for some reason.

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Blog #8 – Black Holes and How to Find Them

Black Holes are quite a popular topic in astronomy, but I still would like to talk about them for my last post, since they are truly revolutionary. Black Holes, in short, are gravity’s ultimate victory over stars. After a star supernova explosion, the core of a star remains. But if this core weighs more than 3 solar masses, gravity overcomes the neutron degeneracy pressure, causing the star’s core to collapse into oblivion and form a black hole! The star becomes infinitely small, but still contains its mass. While its finite mass is still there, the black hole has no physical dimensions! Within the event horizon of a black hole, Newton’s 3rd law is no longer valid. This singularity at the center of the black hole cannot currently be explained by physics and mathematics.

Of course, you can’t talk about black holes without mentioning Einstein’s theory of relativity. According to his theory, gravity is actually the warping of space-time around an object with mass. Einstein asserts that even light, although it has no mass, is affected by gravity. As such, gravity around a black hole imposes a curvature in space that bends light. Within the event horizon, light cannot climb back out. As matter approaches the event horizon, tidal forces are intense and “spaghettify” any object. Contrary to media depictions, black holes do not “suck” things into them. Black holes, like any other object according to Newton’s law, exerts gravitational force. Gravity only deviates from Newton’s law at the Schwarzschild Radius (distance from a black hole when escape speed equals the speed of light).

Finding black holes is just as interesting. We can detect them in X-ray binary stars (where matter from one star falls onto another). Astronomers observe orbiting planets experiencing tidal disruption, where matter heats up as it falls in a gravity well, emitting X-ray light for us to detect. However, we cannot see the companion star where all the matter is falling. Kepler’s 3rd law tells us that the mass of said unseen companion is greater than 3 solar masses, but it can’t be a neutron star otherwise we would see it. The only thing that massive, but small enough to be invisible, is a black hole!

The first ever candidate for this procedure was Cygnus X-1, a binary star system. The left image depicts its location within an active star-forming nebula. The right image is an artistic depiction of matter from the companion star falling into the black hole.

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Blog Post 8: How astro2110 Has Changed My View On Astronomy

Star Gazing

Before coming into astro2110, I knew very little about astronomy. Now, after completing the course, my appreciation for astronomy has greatly increased. A few days before the semester started, one of my friends who is an astronomy nerd laughed at me for not knowing the phases of the Moon. I thought to myself, “I’m a CS nerd, why would I need to know the phases of the Moon”? I had forgotten just how interesting astronomy is as a whole. Never had I sat down and actually thought that there’s more to astronomy than just the phases of the Moon. There’s the Milky Way , and extremophiles, and dwarf planets, the Kuiper Belt, moons of other planets, constellations, nebulas, aliens, space missions, and much more. Learning about all of these topics and more makes me excited to learn more in the future. The galaxy is way bigger than I thought, and we’re just a mere speck in the midst of it all. Which means that I still have tons more to learn about what’s here on Earth and what is out there beyond the stars. Watching the lecture that Alan Stern gave about the New Horizons mission visiting Pluto refueled my curiosity about space exploration. The fact that we don’t know what’s out there and we’re constantly learning new things has influenced me to continue to keep up with astronomy in the future. Now I can go back to my friend and tell him every single one of the phases of the moon and maybe even throw one of my own astronomy questions at him.

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