Moon Phases!

A Timelapse of the Earth’s Moon’s Phases

To start off, I am going to be focusing on our own Earth’s Moon. As we all know, the Moon goes through phases as it orbits the planet. It’s current phase is dependent on where it is in the sky relative to the Sun. For example, the New Moon rises and sets with the Sun and is in the same direction as the Sun. This is why the sunlight is at the back of the Moon and there is no light to illuminate the front face of the Moon. Okay, using the word Moon so much makes it feel like it’s not a real word anymore, so from now on I will be calling the Moon “Steve.” So, as we move through the months, Steve will change positions relative to the Sun. When the Sun is across from him, his face will be fully illuminated and we will have a Full Moon. Between these two phases of fullness and newness, Steve will cycle through many different phases. These are called waxing, meaning increasing, as more of his face becomes illuminated by the Sun’s light and waning, meaning decreasing, and more of his face becomes shadowed. Steve also appears at different times during the day depending on what phase he is in. For example, because Steve must be opposite of the Sun to be fully illuminated, he must rise above the horizon and into view while the Sun is setting on the opposite horizon. So, as the Sun sets in the West, Steve rises in the East. Another example of this is that when Steve’s face is in its ”Third Quarter” phase, then he would need to rise over the horizon and into view around midnight and set around noon of the next day. This is why we can see the Moon during the day sometimes!

    I would like to leave you with this fun fact! Most people believe that the side of the Moon that is always facing away from the Earth is the “Dark Side,” but this is not true. The other side of the Moon actually goes through phases as well, we just can’t see them because the Moon rotates completely on a rate that roughly equals one month. This is why we always see the same face of the Moon facing toward us. Think of it like this: Steve wants to keep his eyes on us, so we never see the back of his head!

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Blog 1 – Initial Review of SkyView Lite

SkyView Lite is an iPhone application that allows the user to point their phone at different parts of the sky and see an overlay of constellations in the direction that they point. I downloaded the app and tried it out. This post is going to be about my experience using the app.

The app works by using a combination of your GPS location and iPhone orientation to calculate what portion of the sky you can see when you point your phone in any given direction. This application is great for inexperienced sky-watchers to learn the about the constellations, planets, and satellites. While using it for a few minutes, I was able to find the North star, locations of the 12 Zodiac constellations, many planets, the ISS and the Hubble space telescope. I noticed that just like in the textbook, the zodiac constellations formed a ring around the Earth going from East to overhead, to West to straight down.

Screenshot from within the Skyview App

In the app, I could see that the Sun is in Capricorn, even though according to the Astrology signs, the Sun is currently in Aquarius. This lines up with what we learned in class, which is that due to the Earth’s precession, the sun is now one sign “behind” of where the original astrologists of star signs saw them 2000 or so years ago.

I am looking forward to going stargazing and using this app to learn more about the sky. I also can’t wait to learn more about the night sky through this astronomy class!

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The speed of light and what it means for the Earth-Sun system.

The speed of light is one of the most important laws (or principles) in our Universe. The speed of light determines what we see and when we see it, as well as providing a universal “speed-limit” for countless celestial objects that zoom throughout the universe. I find it illuminating to consider the speed of light in regards to how it affects my (or humans in general) everyday life. Principles such as special relativity and time-dilation don’t manifest at the relatively sluggish pace of even the fastest man-made contraptions such as cars, trains or planes. On the other hand, the Sun, affects nearly everything that we as humans do, and the Sun’s light is greatly affected by the speed of light. The Sun dictates what we wear each day, when we go to sleep, whether we will go swimming today, or whether we will go ice skating. Because the Sun is located approximately 150 million kilometers from Earth (on average), and because the speed of light is around 300,000 km per second, the light that we observe from the Sun is not the light that is currently being emitted from the Sun, but light that was emitted some time ago. Using some rough math, we can calculate how long ago the Sun emitted the light that we are observing on Earth. (150 * 106 km) / (300 * 103 km/s) = 0.5 * 103 seconds = 500 seconds = 8 minutes and 20 seconds. This means that if the Sun suddenly stopped emitting light, or if a large passing celestial object obstructed the Sun’s light from reaching Earth (or parts of Earth), we would still receive the Sun’s light/heat for more than eight minutes!

Video From NASA: Information about the Sun, solar wind, and the Parker Solar Probe. Info about the Sun begins at 0:38. For more information about the Parker Solar Probe visit the NASA page linked here.
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“Powers of Ten” and the Scale of the Universe

The famous Hubble Ultra Deep Field image, which illustrates the scale of the universe by showing countless galaxies in a region of space previously thought to be nearly empty

I didn’t remember until I started the video, but I had seen “Powers of Ten” before in some science class many years ago. This staying power, evidenced by my recollection and the countless Youtube comments saying similar things, is proof of how mind-blowing the concept of scale is.

Scale determines what we can comprehend and the shape that reality takes for us, but because it is so inherent to our everyday lives, it is very difficult to understand this. That is why videos like “Powers of Ten” are so important: they open our eyes to the fact that there is so much more out there than human-sized things. This is part of why I study physics and astronomy. Yes, human-sized problems are particularly relevant to our lives, but physics deals with the smallest and largest scales. There is so much richness in places that we don’t see everyday that other academic disciplines simply don’t touch. For example, this course focuses only on the Solar System and still has so much content to cover— about the Sun, the planets and their interactions, the moons, and so on. Yet, the Solar System was only at the 13th power of ten in the video, 100 billion times smaller than the upper limit of 24. That is what makes physics and astronomy different from other subjects.

I’d also like to touch on a question that is invoked by thinking deeply about scale: do you think that scale goes on infinitely in either direction? I personally think that the universe should be scale invariant because there is no reason that things should stop existing once they get very big or very small. The video discusses how there is a pattern of “alternation between great activity and relative inactivity” as you zoom in and out, and in my mind this should go on forever. However, that concept of infinite scale also has logical issues. What do you think?

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Blog 1

Wikipedia

The scale, and “end points” to our universe, is widely unknown. Because as humans have not ventured or seen any type of universe ending barrier, the question of infinity comes into play. One common assumption that a human naïve to the theories of astronomy would have is that the universe is never ending. This, however, provides no insight nor bounds to the volume of our universe. Instead, astronomers track the end of the universe based on the farthest light we can see. The image above comes from the Hubble telescope and pictures remote galaxy’s billions of light years away. As of right now, the edge of the observable universe is 47 billion light years away. There is absolutely no evidence that this, however, the edge of the universe. It is odd how the length is depicted in this way, because this by no means is the size of the universe.

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The Scale of the Universe (Post 1)

Source: NASA

The universe is so massive that it can be difficult for humans to comprehend its scale, so I will break it down using something that we can easily understand. Earth is 1 AU (astronomical unit) from the sun or 150 million KM. If a human were travelling this distance in a car at 100 miles per hour, it would take approximately 41,166 days or 112 years. Now this doesn’t seem too crazy; however, the distance from the earth to the sun pales in comparison to the size of the entire universe. The distance from the sun to the edge of the solar system is roughly 145 billion KM. When travelling from the sun to the edge of our solar system at the same pace it would take 3.7 million days or roughly 10,000 years. This is substantially longer than a human lifetime, but let’s go even further out. From the center of the Milky Way (our galaxy) to its edge it is 500 quadrillion KM. At 100 miles per hour, it would take 350 billion years to reach the edge of the Milky Way. But the universe can’t be much bigger than that right? Wrong. There are billions of galaxies in the observable universe and the Milky Way is just one. From the center of the observable universe to its edge is 4.4 x 10^23 KM. To travel this distance at 100 miles per hour would take approximately 3.1 x 10^17 years or 310 quintillion years. While our solar system and even our planet appear to be giant from a human perspective, they are merely a speck in the grandiose universe we inhabit.

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Blog 1-Why the Cosmic Calendar is so interesting

By far one the most interesting aspect of understanding the cosmos for me revolved around the cosmic calendar. Essentially, The Cosmic Calendar takes the time span of the entire universe and condenses it into single year based on the calendar. Just like any other calendar year, time starts on January first and ends at 11:59 on December 31st. Now at the surface this may not seem very interesting, but when you take a closer look, there are many shocking facts and aspects of it. With the universe being around 13.8 billion years old all condensed in one calendar year, it is crazy to see how many things can occur in even one day of the year. For reference, one day can equate to roughly 40 million years, so of course many things can occur.  Another particularly shocking revelation made apparent by The Cosmic Calendar is that dinosaurs survived roughly a week relative to the calendar while humans only appear on the last day of the year and fairly late in the day as well. This just shows in grand fashion the extremely long period of time the dinosaurs ruled the earth and how late and short period of time in which our ancestors came into fruition. The picture shown below helps give a visual on these timelines.

The Cosmic calendar from CosmicCalendar.net

Based on this calendar it is so fascinating to see just how short a period of time humans have existed in the grand scheme of things, just one of the reasons why I am eager to learn more about universe around us.

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The Vastness of the Universe

Our universe is composed of two: the observable and entire. There is a distinction between the two because light takes time to travel through space. From what we know, the observable universe is 13.8 billion years old. Already, that’s an intimidating age, but the thought of the entire universe makes it even more intimidating. There is so much to learn about the universe. 

How could there possibly be so much that exists that I simply cannot see? 

It is hard to realize how small we actually are. The world is already so big compared to us. The circumference of Earth is roughly 40,075 kilometers. The sun is roughly 4.366 kilometers across. The Milky Way galaxy is roughly 102,000 light years thick. The thought of how large the universe is daunting, but it’s important to realize this. It’s comforting to know that so much around us has been around for so long that we can’t wrap our minds around. I used to not like the feeling of awareness around my small existence, but it’s freeing to know that there are so much bigger things that will outlive me and anyone else I know. It goes to show that my worries don’t hold as much as I think they do.

The Observable Universe by Pablo Carlos Budassi

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Blog 0 Quick Introduction

Hello everyone, my name is Jadon Roy. This is a picture of me and my best friend who visited me in Nashville last semester. We are from Louisiana so it is always fun when he visits!

Taken on Broadway, by me

This is my introductory blog for Astro 2110

Here is my blog https://wordpress.com/posts/jadonroyastronomy.wordpress.com

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Totality

On August 21, 2017, my family and I drove from Atlanta, Georgia to Clemson University in South Carolina to witness the solar eclipse in totality. Atlanta reached 97% totality, but Clemson reached complete totality:

Great American Eclipse

At about 2:37 PM, the moon completely covered the sun, positioning itself perfectly between earth and the sun and casting a shadow directly over Clemson. The sky darkened considerably, cheers erupted from all who attended, and the sun’s corona became visible around the dark disk of the moon. Below are two images I captured of the event, the first of the sun’s corona peeking around the moon, and the second of the sky and landscape to give an idea of how much light the moon truly blocked. As you look at this image, remember that this was taken at about 2:37 PM, when the sky should be almost as bright as ever.

By me
By me
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