The Last 2 Minutes of History

https://www.scienceabc.com/nature/universe/cosmic-calendar-universe-365-big-bang-compress-history.html
Important Events in the Cosmic Calendar

Down on Earth, it’s easy to think the passage of 100 years is a long time. After all, it’s certainly longer than a human’s life expectancy. However, after hearing that modern humans can only be accounted for in 2 minutes of history, it’s hard to believe that the time spanning from the origins of modern humans until today has occupied a significant amount of time. Now you may wonder why I said that modern humans in history only lasts for 2 minutes when modern humans evolved around 40,000 years ago. Let me explain. If the universe’s history, starting with its inception 14 billion years ago, was put into a calendar of one year, modern human history would only account for two minutes of the time. That means that if you placed all 14 billion years of the universe’s history into a calendar year, modern humans would occupy the calendar at 11:58 on December 31. This calendar, known as the cosmic calendar, begins on January 1st, when the Big Bang occurs. According to this calendar, the Milky Way was formed sometime in February. What is even more fascinating about this cosmic calendar is that when calculated to the scale of a year, dinosaurs roamed the Earth only five days prior to modern humans, on December 26. This is a stark contrast to our record of time, where dinosaurs populated the planet around 225 million years ago. Probably the most important idea that this calendar puts into perspective is the fact that our solar system, despite the fact that it is 4.6 billion years old, has only been a part of the universe for a third of the universe’s existence. That means that according to the cosmic calendar, our solar system only formed on September 3. When put into perspective, it’s hard to believe that any passage of time is truly significant over the span of 14 billion years and when this is compounded with the vast size of the universe, it’s hard to believe that our lives are not anything more than a blip in space and time.

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What is Astrophysics?

I thought I’d start my blog off by talking about what I am most interested in, Astrophysics. While I am a physics major, my passion is astrophysics and studying the life and death of stars. Astrophysics applies the laws of physics and chemistry to explain the birth, life, and death of stars, planets, galaxies and more.  Astrophysicists want to study our universe and better understand our place in it.

I think one of the coolest things about astronomy and astrophysics is that you can get involved and help out, even if you’re not studying the subject or even in school. NASA provides resources for citizen scientists. CosmoQuest and Galaxy Zoo allow citizens to analyze pictures and categorize photos to help increase our database. This allows astronomy to become much more approachable and understandable to anyone!

Source: https://www.space.com/26218-astrophysics.html

main-qimg-da091d392a16b4834e68cd6cab35b101-c
Quora
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A Speck on a Speck in a Speck in a Speck…

Humans are very arrogant creatures, and we often forget just how small we are in relation to the rest of the Universe. So much so that our units of measurement are very impractical to use on a larger scale, so we will mostly be using light seconds, minutes, hours, day, months and years to talk about the size of the Universe. Light travels at a speed of about 299,792 km/s, which means that light can travel around the Earth’s equator (40,030 km) almost 7.5 times in 1 second. That’s pretty fast, especially when you consider that a flight from Columbus, OH to Nashville, TN takes about an hour. With this concept of light speed in mind, consider the fact that it would take light 4 hours to reach Neptune and 1.87 years to reach the edges of the solar system. Remember, this is the same speed as the one that could circle Earth 7.5times in a single second. To keep going, the closest star to our own, Proxima Centauri, is 4.22 light years away! At its current rate, it would take Voyager-1 (the fastest man-made object) 73,000 years to reach this star!!

oort-cloud-nasa-e1424276825581
Scale of our Solar System – Source:Futurism

To zoom out even more, you would find that our galaxy is 1,000,000,000,000,000,000 km in diameter (which is 100,000 light years). So yeah, our galaxy is pretty big. Now take that galaxy and shrink it down even more as it starts to become indistinguishable among the other galaxies until you are at roughly 13.8 billion light-years from our Sun. This is the edge of the observable universe, not to be confused with the actual size of the universe. We call it this because the universe is only 13.8 billion years old, so the light from beyond that edge does not exist yet (from Earth’s prospective) To put it simply, as we look further into space, we also look further back in time so we cannot look further back than the start of the Universe. NASA scientists estimate the actual size of the universe to be 93.6 billion light years away.

So, the next time you forget just how small we all are relative to the size of the universe, take a quick look at the video below from Youtube:

 

 

 

 

 

 

 

 

 

 

 

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First Galaxies Formed Today

…according to the cosmic calendar.

The cosmic calendar is a visualization method to help comprehend the age of the universe. This calendar puts the beginning of the universe at the start of the first of January, and the end of December 31st at our current point in time. In this demonstration model, January 22nd (today!) is when the first galaxies began forming and cosmic dust started drifting together to eventually form stars.

COSMICWell, surely earth shows up somewhere in the middle of the year right? Well, no. Our galaxy, the Milky Way, was only formed by around March in this visualization, with the disk part (which contains all the stars, dust, and such) forming around May. The earth formed along with the rest of the solar system around 3 months later in the Orion Spur. So, from New Years to now (first galaxy formation) on the cosmic calendar was around 0.95 billion years. By the time the semester is over and we’ve taken the final for astro, the Milky Way will be a few days short of fully forming its disk component, and the Earth will only have formed a few weeks after classes start for the next academic year!

Sources:

Wikipedia, “Cosmic Calendar”

Science ABC, “Cosmic Calendar: History of The Universe In Just 365 days”

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Seasons, Solstices and Equinoxes

 

 

Sun
Solstices and Seasons via Dogfoose

What causes the seasons?  Not only is this asked on page 32 of Chapter 2, but it is often asked by many individuals residing on Earth.  However, a surprisingly few number of people actually know.  Seasons occur because the title of Earth’s axis causes sunlight to fall differently on Earth at different times of year.  Notice that the seasons on Earth are caused by axis tilt not by its distance from the Sun.  While Earth’s distance to the Sun changes over a year, Earth is only about 3% farther at its farthest point than it is at its closest point.  Interestingly, Earth is farthest away from the Sun in July and closest to the Sun in January!  The difference in strength of sunlight is completely overwhelmed by the difference in the Earth’s tilt.  We use Solstices and Equinoxes to help us mark the change of seasons, and there are four special positions in Earth’s orbit that mark the change in seasons.  The June solstice, known as the summer solstice for those who reside in the Northern Hemisphere, occurs arround June 21 and is the moment when the Northern Hemisphere is tipped most directly toward the Sun and receives the most direct sunlight.  The longest day and the highest solar noon almost always occur during the June solstice, too.  The December solstice, called the winter solstice by people in the Northern Hemisphere, occurs on December 21 and is the moment when the North Hemisphere receives the least direct sunlight.  Coincidentally, the shortest day and lowest solar noon almost always occur on this day.   The March equinox, called the spring equinox by people in the Northern Hemisphere, occurs around March 21 and is the moment when the Northern Hemisphere transitions from being tipped slightly away from the Sun to being tipped slightly toward the Sun.  Lastly, the September equinox, called the fall equinox in the Northern Hemisphere, occurs around September 22 and is the moment when the Northern Hemisphere first starts to be tipped away from the sun.

The exact dates and times of the equinoxes and solstices can vary up to a couple days from the given dates above.  Also, the Solstices and Equinoxes happen in reverse for the Southern Hemisphere.  For example, the June Solstice results in the Southern Hemisphere being tipped most away from the Sun and receives the least direct sunlight.  All in all, many people believe that seasons are caused by variations in the Earth’s distance from the sun.  If this was true, the Northern and Southern Hemispheres would have the same seasons at the same time, which we know is not true.  The real cause of seasons is the Earth’s axis tilt, which causes the two hemispheres to rotate being tipped toward the sun over the course of a year.

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Seasons, Solstices and Equinoxes

 

 

Sun
Solstices and Seasons via Dogfoose

What causes the seasons?  Not only is this asked on page 32 of Chapter 2, but it is often asked by many individuals residing on Earth.  However, a surprisingly few number of people actually know.  Seasons occur because the title of Earth’s axis causes sunlight to fall differently on Earth at different times of year.  Notice that the seasons on Earth are caused by axis tilt not by its distance from the Sun.  While Earth’s distance to the Sun changes over a year, Earth is only about 3% farther at its farthest point than it is at its closest point.  Interestingly, Earth is farthest away from the Sun in July and closest to the Sun in January!  The difference in strength of sunlight is completely overwhelmed by the difference in the Earth’s tilt.  We use Solstices and Equinoxes to help us mark the change of seasons, and there are four special positions in Earth’s orbit that mark the change in seasons.  The June solstice, known as the summer solstice for those who reside in the Northern Hemisphere, occurs arround June 21 and is the moment when the Northern Hemisphere is tipped most directly toward the Sun and receives the most direct sunlight.  The longest day and the highest solar noon almost always occur during the June solstice, too.  The December solstice, called the winter solstice by people in the Northern Hemisphere, occurs on December 21 and is the moment when the North Hemisphere receives the least direct sunlight.  Coincidentally, the shortest day and lowest solar noon almost always occur on this day.   The March equinox, called the spring equinox by people in the Northern Hemisphere, occurs around March 21 and is the moment when the Northern Hemisphere transitions from being tipped slightly away from the Sun to being tipped slightly toward the Sun.  Lastly, the September equinox, called the fall equinox in the Northern Hemisphere, occurs around September 22 and is the moment when the Northern Hemisphere first starts to be tipped away from the sun.

The exact dates and times of the equinoxes and solstices can vary up to a couple days from the given dates above.  Also, the Solstices and Equinoxes happen in reverse for the Southern Hemisphere.  For example, the June Solstice results in the Southern Hemisphere being tipped most away from the Sun and receives the least direct sunlight.  All in all, many people believe that seasons are caused by variations in the Earth’s distance from the sun.  If this was true, the Northern and Southern Hemispheres would have the same seasons at the same time, which we know is not true.  The real cause of seasons is the Earth’s axis tilt, which causes the two hemispheres to rotate being tipped toward the sun over the course of a year.

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Earth Measured Relative to the Cosmic Scale

The Universe is an unbelievably vast entity. Earth’s radius is about 6.4*106 meters. In overwhelming contrast to this, the radius of the observable universe is approximately 4.4*1026  meters. That is a difference of 20 orders of magnitude. If the earth’s radius, and the universe as a whole, was scaled down such that the earth was the size of a single proton, the universe would occupy the space of a mid-sized city. It is nearly impossible to comprehend or visualize such scales without losing sight of earthly sizes or distances. This arguably  frames astronomy as the broadest of all fields.  While most areas of study are limited to our tiny speck of a planet, astronomy explores the vast majority of the universe outside of our familiar rock.

universe scale
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Earth Measured Relative to the Cosmic Scale

The Universe is an unbelievably vast entity. Earth’s radius is about 6.4*106 meters. In overwhelming contrast to this, the radius of the observable universe is approximately 4.4*1026  meters. That is a difference of 20 orders of magnitude. If the earth’s radius, and the universe as a whole, was scaled down such that the earth was the size of a single proton, the universe would occupy the space of a mid-sized city. It is nearly impossible to comprehend or visualize such scales without losing sight of earthly sizes or distances. This arguably  frames astronomy as the broadest of all fields.  While most areas of study are limited to our tiny speck of a planet, astronomy explores the vast majority of the universe outside of our familiar rock.

universe scale
Mic News
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Proxima b

We’ve alluded to exoplanets and habitable zones in class, but you may be wondering just how similar these planets are to Earth – and if we can even get there.

Proxima b is a rocky mass larger than Earth that orbits our Sun’s closest neighbor, Proxima Centauri. Astronomers have determined that Proxima b lies in a much closer Goldilocks zone than Earth (due to Proxima Centauri’s size and low temp.) and its orbit is the ideal distance for liquid water at the surface, suggesting a close potential alien host.

How close is close, though?

At less than half the distance of the next nearest exoplanet, Proxima b is still 4.2 light-years away from us. If one could travel the speed of light, it would take just over four years to reach Proxima b at the very least. 32,000kph is super fast for us, and this speed would get us there in 142,000 years. Considering that this speed is less than 0.003% the speed of light, we have a long way to go before we even consider exploring the closest exoplanet (or a major breakthrough). There are also issues of time dilation that would contort the travelers relative sense of time during light-speed travel that I think deserves an entire blog of its own (interesting question: would light-speed trips need to be coordinated across multiple generations to account for time dilation?).

Putting our distance to Proxima b in perspective

While it’s unfortunate these celestial bodies are so far away, I’m optimistic that immensely more efficient space travel is a possibility of the near future. With clean fusion almost reached and breakthroughs such as metallic hydrogen surfacing year after year, there’s no telling what the future may hold.

 

 

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2017 Solar Eclipse

My junior year at Vanderbilt University began in the most spectacular way – witnessing a total solar eclipse through a skylight within Nashville airport, immediately upon arrival. Surrounded by a gathering of fellow traveller’s experiencing this magical moment, the moment in which the Sun was reduced to a radiant ring wrapped around the black outline of the Moon was even more breathtaking than I could have imagined.

The phenomenon known as a solar eclipse occurs when the Moon falls directly between the Earth and the Sun, causing the Moons shadow to cover the Earth. Due to the Earth being of a far larger size than the Moon, only a certain portion of the Earth is covered and so the spectacle can only be witnessed from particular locations. Here in Nashville, we were fortunate enough to be directly within the pathway of the Moon’s shadow, known as the path of totality. Solar eclipses can only occur during the new phase of the Moon, and when the Moon is very close to a node. Nodes are the points within the Moon’s orbit that sees it cross through the ecliptic plane.

As previously mentioned, the solar eclipse seen in Nashville was a total solar eclipse. A total solar eclipse occurs when the Moon, within its orbit, is relatively close to Earth. In this stage, the Moon’s shadow, also known as its umbra, can cover an area of the Earth of up to 270 kilometers. From when the Moon very first begins to cover the Sun, it takes a couple hours for the Moon to entirely block the Sun and enter a state known as totality. It was at this point where I had just stepped off my plane and was looking up at the sky. Everyone in the airport was awestruck as the sky outside went completely black. Although I was inside at the time, people would later tell me of the temperature dropping and reports of birds flying around in utter confusion and insects chirping as if it was nighttime. After a couple minutes of darkness, the Sun began to slowly reemerge and on I went to begin my Junior year at Vanderbilt. While it was a quick process, I could not think of a more magical way to begin my year.

Below is an image of the solar eclipse that I captured through the airport skylight.

IMG_0104
Nashville International Airport, August 21st 2017

 

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