Time travel is cool

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That, is an attention-grabbing title.

I'm often mildly disappointed with our education system, because it fails to teach a lot of the scientific literacy that is needed in order to understand some of the concepts that science is discovering today, and to appreciate just how cool some of this stuff is. Today, we're talking about light, the speed at which it travels, and the closest thing to a time machine we'll ever actually see.

Let's start with the speed of light. Light is a funny thing. Einstein realized, and then proved scientifically that no matter how fast you're travelling, no matter which direction you are moving in, you will always measure light as moving away from you at 300,000 km/s. This speed is referred to with the constant c. This is counter-intuitive to the way we humans think. Let's say I'm standing still, and my friend Davey runs by me. Let's say I measure that he is moving away from me at 10 km/h. Now, in scenario two, I'm running at 5 km/h in the same direction as Davey. When he passes me and starts to move away from me, I will measure him as moving away from me at 5 km/h, rather than the previous 10. This is because I am moving foward at 5 km/h myself, rather than standing still.

Here comes the counter-intuitive bit - in both of those situations, if a beam of light travels past me and starts to move away, I will always measure it as travelling away from me at c (300,000 km/s). Interestingly, the scientific experiements and evidence collected also shows that this is the theoretical speed limit of the universe. As far as we can tell, nothing can travel faster than this speed.

Okay, we're past the first bit of math.

Let's get into the time travel I alluded to in the title. Because of the rate of speed at which light travels, most of us think of it as travelling instantaneously. That is to say, you turn on your desk lamp, and the light doesn't travel to light up your desk, it's just there. This is a convenient way to think about light on a day-to-day basis, our daily lives do not involve interacting over distances greater than 300,000 km. However, once we start to talk about the stars in the sky, things get a little bit different.

The thing about stars in the sky is that they are very, very far away from us. Sirius, one of our closest neighbours in the galaxy, is about 9 light years away from us. Light years can be a bit of a confusing term, because they contain two concepts: distance and time. A light year means this: The distance that light can travel in one year. So, even though the name includes a notion of time, a light-year is always really a distance measurement, and one light-year will always take one year for light to move that distance.

What this means is that if Sirius the star were to suddenly dissapear from the universe and stop producing light (this is highly implausible, but will work as an example), it would take us nine years before we had any idea that this had occurred. The coolest thing about this is that when we look up and see the star Sirius in our night sky, we are actually seeing it as it looked nine years ago. Remember, it takes nine years for the star's light to reach us.

So, we've got the speed of light down, and we've talked about Sirius. Let's take things up to the next level and talk about stars that are much further away from us. Astronomers these days have some incredible tools at their disposable. The Hubble space telescope is able to look at stars that are billions of light years away. This is incredibly far, but not only that, it means that we are looking back at light that was created and sent on its heavenly journey billions of years ago. This is the most incredible part, and the most difficult for many people to wrap their head around. The further away from us that astronomers are looking, the further back in time they are seeing the state of the universe.

Perhaps some ascii art to help clarify?

1. (Sirius) * ---light travels 9 light-years---> * (Earth)

2. (Starry McOldey) * ---light travels 10 billion light-years---> * (Earth)

The most important thing to remember here is that once light has been emitted from a star, it doesn't matter what happens to the source of the light - the light itself will continue to travel on its path, eventually reaching us.

I've got two helpful analogies too! Think of a really powerful sprinkler: the sprinkler shoots out a blast of water, and then changes its position and shoots a second blast of water. The first blast of water is still travelling in the original direction, regardless of the fact that the sprinkler has now changed its orientation. Analogy number two - imagine two cities that are separated by 1000 km. The first city sends out a messenger to the second city, and it takes him two weeks to get there. By the time the messenger arrives in the second city, the information he's bringing with him is two weeks older. For the sake of this analogy, you can think of light as acting like a messenger from a star (though a messenger that has done an insane amount of steroids).

So, I, and possibly you, think this is pretty cool. By looking into deep, deep space, scientists are able to see the universe as it was when it was very young (most astronomers, through scientific evidence, place the age of the universe to be roughly 13.7 billion years old). They aren't really traveling back in time, but they are able to see a universe from an earlier time.

Interesting stuff right? No? Whatever. If you like reading about this kind of thing, you should check out the Bad Astronomy Blog. Phil Plait, a widely-known astronomer in skeptic circles, runs the blog and mixes things up with the latest cool astronomy news, reviews of bad movies using bad science (his review of The Core is pretty good), and skepticism regarding things like the Moon Landing Hoax. Worth a browse!

3 Comments

Interesting post, and on the subject of things I too like to think about. I'd like to shed some more light (hah) on the subject by calculating, in this very comment form, how far (in kilometers), Sirius is away from us. To do this, we will have to figure out how far a light year actually is, and then multiply that by 9, since Sirius is 9 light years away from us.

First, we must calculate the number of seconds in a year:
(60 seconds) * (60minutes) * (24hour) * (365days) = 31536000

Then multiply this times the number of kilometers light can travel in one second: 300,000, or c as Einstein likes to say:

"I just ran c dude!"

c * 31536000 = 9,460,800,000,000 km = 1 light year

Sirius is 9 light years away from us, so lets multiply that by 9. I'll spare you this complex equation. The answer is that Sirius is approximately 85,147,200,000,000 km away from us.

And that's the closest non-sun star to us? Zounds.

i love being used as examples.

Also I love this classic (and relevant dialog) that takes place after Murray pays to have some stars named after the band.

Murray: There's something I need to talk to you about. It's not good news. Planet Jermaine. It's supernova-ed. Yeah, there's nothing left of it apparently, just a huge gaseous cloud and the beginning of a black hole.

Jermaine: When did this happen?

Murray: About 4 million years ago.

Also:

Something else that's crazy, is that radio transmissions (and tv signals, and stuff), never go away. They constantly beam through space. Somewheres in the universe, Perfect Strangers is still on the air.

The radio waves that were created during the Big Bang still exist. It's called John McCain's radio show.

HEY-OOOOO

Radio signals - well, to an extent. It depends on how focused the source is, and also how strong the transmission is.

There's lots of talk about the first big broadcast made by Earth was the Nazi's Olympics, and how this would be the first thing that is seen by intelligent life outside of our own sphere.

This isn't entirely true though. Radio and TV waves, are all just forms of light. So are all the other forms of electromagnetic radiation - when scientists refer to light, they are actually referring to the entire spectrum of electromagnetic radiation, which includes X-rays, Gamma-rays (the most powerful, highest frequency rays), ultra-violet rays (just slightly above our visible spectrum, and what gives you your tan), the visible spectrum of light, down to infrared, radio waves, etc.

The thing is, as light propagates forward, it can get absorbed by electrons, and then re-emitted in different directions. This causes a scattering effect, and will disperse the bgeam that you originally send out. This is why, when you point your flashlight at the sky at night, the beam disperses, rather than blasting straight up out of the sky forever. There's a lot of stuff in our sky on Earth, because we have an atmosphere and a lot of stuff is contained in the atmosphere (air, methane, CO2, etc.). This means that there's more things in play that can absorb your flashlight's beam and send it out in a new direction.

For very powerful radio sources, such as radio galaxies (typically galaxies with extremely active nuclei, that are blasting out tons of radiation as radio waves), the radio waves just keep on going, because the source is so damn powerful, and so plentiful. Even if a bunch of the radiation that is beaming out gets absorbed and then re-transmitted in a new direction, there's still SO much remaining that carries along the original path. Our initial broadcasts of the Olympics? It's pretty likely that they've died out.

Davey's right about one thing that is especially cool though, and that's the radiation created during the Big Bang. Astronomers refer to this as the "Background Microwave Radiation", and it's a slight amount of energy that exists in all portions of the universe. According to experimental evidence, and theories that have been put to the tests multiple times, this is microwave radiation that is left over from the Big Bang. That's crazy stuff.

Davin - your comment explains pretty accurately why a lot of scientifically-minded people are skeptical that we are being regularly visited by extra-terrestrials (but seriously, if they *were* going to come to Earth, they would definitely be making crop circles. That shit is tight!).

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  • Adam: Radio signals - well, to an extent. It depends on read more
  • daveyb: i love being used as examples. Also I love this read more
  • Davin: Interesting post, and on the subject of things I too read more