Parsec Definition

Back

⇐ Use this menu to view and help create subtitles for this video in many different languages. You'll probably want to hide YouTube's captions if using these subtitles.

Parsec Definition

相關課程

0 / 750

You've probably heard the word "parsec" before
in science fiction movies or maybe even in some things dealing with astronomy.
And what I want to do with this video is really just tell you
where this, where the word and the definition of the word really come from
and just to kind of cut to the chase.
It's just a unit of distance.
It's just about 3.26... 3.26 light years.
What I want to do is think about where did this weird distance come from,
this distance that is roughly 3.26 light years?
It comes from... it comes from the distance...
the distance of something...
of something, probably a star, but let me say "something"
because there are no stars exactly this far away from us.
The distance of something whose parallax, or let me say
that has... that has... a parallax... parallax... angle
of... one arc... one arc second, and the word
comes from the "par" in parallax and the second is "arc second".
So it's literally "par"... I'm going to do this in a different color...
It's literally "parsec".
You can think of this as a kind of a parallax... parallax arc second.
How far would this thing be?
It turns out it's 3.26 light years.
So we can actually calculate that, that's essentially what I'm going to do with this video.
So let's say there is something...
let's say... so this is the sun,
this is the earth at some point in time,
this is the earth six months later at the opposite end of the orbit.
And we are looking at some distance,
we're looking at some object, some distance away.
We know that this distance right here is 1 astronmical unit,
and what we want to do is to figure out the distance of this object.
And all we know is that it has a parallax angle of 1 arc second.
So let's remind ourselves of what this means.
If we are looking right at, right at, remember we're looking from above the solar system,
so the earth is rotating in this direction, in either case,
and so in this point in the year, we don't know when this is,
depends on what star that is,
at this point in the year, right at sunrise,
right when we first catch the first glimpses of the sun's light,
if we look straight up, if we look straight up,
the angle, the angle between that object in the night sky
and straight up
is going to be the parallax angle.
So this is going to be 1, this is going to be 1 arc, arc second.
And just to make it consistent with the last few videos we did on parallax,
let's just visualize how that would look in the night sky.
So let me draw the night sky over here,
we'll do that in purple maybe
Let me draw the night sky over here.
This is looking straight up.
This is north, south, west, and east.
And so you can imagine in this situation, the sun is just rising on the east...
The sun is just rising on the east.
Let me make it the color of the sun.
The sun is just rising on the east.
And so this will be towards the direction of the sun.
You could imagine that to some degree... well, this is north.
North is the top of the earth right here, kind of pointed towards us, out of the screen.
South is going into the screen.
Hopefully, that helps with the visualization.
Or another way to think about it, the sun is rising in the east.
This is going to be towards the direction of the sun, of a certain angle from the center.
In this case, it's 1 arc second.
So, it's going to be right over here.
So this, this angle right over here is going to be 1 arc second.
And then if we were to see where that object is six months later, it'll be the opposite.
We're going to be looking, we're going to be looking in the same... the center of the universe.
Or I should say the center of the night sky at that point.
The same direction of the universe.
The universe actually has no center. We've talked about that many times.
If we look at the same direction of the night sky, we'll be looking six months later,
and instead of it being at dawn, it will now be at sunset.
We'll be just getting the last glimpses of the sun.
And so the sun will be setting...
the sun will be setting in the west.
The sun will be setting in the west.
And so this angle, this angle right here, which is also the same thing as a paralax angle,
it'll be... this will also be 1 arc second.
So this will also be 1 arc second.
1 arc second.
So let's figure out how far this object is.
What is... what is an actual parsec in terms of astronomical units or light years.
So if this is 1 arc second, this is going to be...
and remember, 1 arc second is equal to one-thirty-six-hundreth (1/3600) of a degree.
1/3600th of a degree.
So this angle, right over here, is going to be 90-1/3600th.
And we just use a little bit of trigonometry.
The tangent of this angle.
The tangent of 90-1/3600 is going to be this distance in astronomical units divided by 1.
Well, you divide anything by 1, it's just going to be that distance.
So that's the distance right over there.
So we get our calculator out, and we want to find the tangent...
the tangent of 90-1/3600, and we will get our distance in astronomical units.
206,264.
We're going to say 265.
So this is going to be equal to...
This distance over here is going to be equal to 206,265. I'm just rounding, astronomical units.
And if we want to convert that into light years, we just divide.
So there are 63,150 light years per astronomical unit...
I'm sorry, astronomical units per light year.
So this is... let me actually right it down.
Just so you make it... I don't want to confuse you with the unit cancellation.
So we're dealing with 206,265 astronomical units,
and we want to multiply that times 1 light year is equal to 63,115 astronomical units.
And we want this in the numerator and the denominator to cancel out.
And so if you divide 206,265, this number up here,
divided by 63,115, the number of astronomical units in a light year,
63,115... let me delete that right over there,
we get 3.2 or the way, the way the math worked out here,
round to 3.27 light years.
So this is equal to... this is equal to roughly 3.27 light years.
So I should just show it's approximate right over there.
But that's where the parsec comes from.
So hopefully, you now you just realize it is just a distance.
But even more, you understand where it comes from.
It's the distance that an object needs to be from earth
in order for it to have a paralax angle of 1 arc second.
And that's where the word came from. Paralax. Arc second.