Now on ScienceBlogs: Surveying the "integrative medicine" landscape (2012 edition)

ScienceBlogs Book Club: Inside the Outbreaks

From gluons to galaxies, one scientist takes on all the mysteries the Universe has to offer.

Ethan's Profile

Ethan's Halloween photo Ethan Siegel is a theoretical astrophysicist in Portland, OR. You can learn about him, contact him, or just enjoy the site.

Search

Recent Posts

Awards

2011: Winner - Charm Quark - 3QuarksDaily Prize in Science.

Winner_2011_Charm.jpeg

2010: Best Blog by physics.org.

winner_white.jpeg

2010: People's choice award by physics.org!

winner_black.jpeg

Recent Comments

Archives

Blogroll

Astronomy/Physics Interesting Projects Humor

« Weekend Diversion: The Story of "Me & My Uncle" | Main | The Physics of a Fighter Jet Rainbow! »

Orbiting Earth 101: What You'd See / What You'd Do

Category: Solar SystemSpaceflight
Posted on: September 7, 2010 2:17 PM, by Ethan Siegel

"I saw for the first time the earth's shape. I could easily see the shores of continents, islands, great rivers, folds of the terrain, large bodies of water. The horizon is dark blue, smoothly turning to black. . . the feelings which filled me I can express with one word--joy." -Yuri Gagarin
It takes a tremendous amount of energy to do any type of heavy lifting, and the most extreme example of this is lifting something all the way up off of the Earth, out of the atmosphere, and into space!

atmo.jpeg

And once you're up there, at least 300 km above the Earth's surface, the sights you've got are bound to be absolutely amazing! For example, if you took the US Space Shuttle up, you'd likely dock with the International Space Station, and get to see something as breathtaking as this:

iss_sts119_big.jpeg

But gravity is a funny thing. The same force that pulls the Moon into our planet's orbit is trying to pull your orbiting body (and whatever spacecraft it's inside) back towards Earth.

214811main_EarthMoon-516.jpeg

But while the Moon is 384,000 km away from the center of the Earth and takes about four weeks to orbit the Earth, these man-made satellites and space vehicles, at an altitude of around 300 km, are only 6,700 km away from the center of the Earth.

destiny shuttle_illus_s409.jpeg

(Image credit: Boeing.)

But one of the incredible things that our laws of gravity tells us is that, no matter what distance you are away from any mass, there's only one speed that will keep you moving in a stable, circular orbit!

Any guesses as to what that speed is at the altitude of the International Space Station?

It turns out that you need to travel at a whopping 27,700 km/hr (~17,200 mph) to stay in orbit around the Earth; any slower and you'll fall back down!

satellite_nodes.jpeg

But let's take a look at the Earth itself. Although it's a pretty big place, it's only about 40,000 km all the way around; even at an altitude of 300 km, that makes an orbit of only about 42,000 km all the way around!

This means that it only takes about 90 minutes to make a complete orbit of the Earth, or, in Little Prince terms, you get about 16 sunsets per day.

Space_Sunset_view_from_space_015233_.jpeg

What would it look like, if you were up on the ISS, as you went from Sunset to Sunrise, and got to look at the Earth from space during an entire 40-minute night?

Well, thanks to astronaut Don Pettit, who took a series of images every 15 seconds and stitched it together into a video of one "night" on the ISS, we can see for ourselves!

On a first viewing, I see that it starts out as "day" on Earth. We then get a sunset (and the accompanying lens flare), and then the night side of Earth, pock-marked by cities (the bright lights) clearly shows itself to us. The Moon rises, and the Aurora Borealis (I think) makes an appearance, not just once but twice! And then we pass over some more land (and see some more cities), and finally the Sun rises. Plus, near both sunrise and sunset, you can see the upper atmosphere turn an orange-red color!

And, from up in low-Earth orbit, astronauts get to see this sixteen times a day, speeding at over 27,000 km/hr. Pretty amazing stuff; and thanks to NASA's Solar Dynamics Observatory for posting the video!

Share on Facebook
Share on StumbleUpon
Share on Facebook
Find more posts in: Physical Science

TrackBacks

TrackBack URL for this entry: http://scienceblogs.com/mt/pings/146323

Comments

1

Pretty pictures :)

Something that bugs me is the term "micro-gravity."

I understand that, on the ISS for example, you are still well within the Earth's gravitationl influence (that's why you are falling), but if you are in freefall, you are effectively weightless, yes?

So, what is "micro-gravity"?

Posted by: gruebait | September 7, 2010 4:02 PM

2

From what I have read, microgravity is simply free fall within a gravitational field. I guess its called that simply because there are always residual acceleration present so you can't really call it 0g. My 2cents....

Posted by: Eric Juve | September 7, 2010 6:43 PM

3

Those temperatures in the first diagram threw me for a loop (the shuttle orbits in 950degC?!). Oh yeah, the atoms are fast but there aren't enough of them to hit you and transfer any really heat. How about a post on that?

Posted by: Steve | September 7, 2010 8:14 PM

4

Steve,

Although I only gave it one paragraph, I talked about the analogous problem in the Sun, of the Sun's Corona being a higher temperature than the surface of the Sun.

http://scienceblogs.com/startswithabang/2010/07/whats_the_most_fundamental_thi.php

And your explanation is pretty good, too.

Posted by: Ethan Siegel | September 7, 2010 9:01 PM

5

I am curious about the "one speed" to keep you in orbit at a particular altitude. Is there an explanation or formula to figure out the speed?

Posted by: Waydude | September 8, 2010 12:15 AM

6

Waydude:

Sure. That's the speed when the centrifugal (or centripetal, if you insist) force is strong enough to counter-act the gravity.

So the equation is: v^2/r * m = G*m*M/r^2

m is the mass of your spacecraft, r is the radius from the Earth's center.
v^2/r is the centrigugal acceleration, so v^2/r * m is the centrifugal force.

M is the mass of the Earth, G is the gravitational constant.
G*m*M/r^2 is the Newton's gravity law.

So simplifying and solving this equation, we get: v = sqrt(G*M/r) - note, that the speed actually doesn't depend on your spacecraft's mass.

Substituting numerical values:
G=6,67*10^-11 N(m/kg)^2
M=5.9736*10^24 kg
r~=6378000 m.

So v = sqrt((6.67*10^-11 * 5.9736*10^24) / (6378000)) ~= 8000 meters per second. Or about 28,000 km/hr.

PS: though there is just one circular orbit for a given radius, there are infinitely mane elliptical orbits.

Posted by: Alex Besogonov | September 8, 2010 7:33 AM

7

An even better way to look at this (following Eric Juve) is that "microgravity" is describing what you "feel." And one of the consequences of General Relativity is that you cannot in principle feel gravity if it is sufficiently nearly constant over your whole body. Consider when you walk. When you talk about feeling your weight you feel it in your feet; you are feeling the normal force from the floor, NOT your weight. So if weight is the only force (and the acceleration is the same over your whole body) you do not "feel" any force at all. By consequence, there is not (in the GR sense) any force at all -- if you can't feel a force, it's not there....

Posted by: Taxorgian | September 8, 2010 10:37 AM

8

Newbie question: what on earth fuels something that goes 27,000 km/h?

Posted by: Rokkaku/Ewan | September 8, 2010 1:47 PM

9

Quite commonly, liquid hydrogen and oxygen are used to get into orbit. For rockets, you commonly get the best thrust for the weight if you use light elements that release a lot of energy when they combine. Hydrogen+oxygen are great for this.

Posted by: Ben W | September 8, 2010 2:40 PM

10

Thanks Taxorgian for the explanation of "micro gravity". It really helped me understand the concept better with your description.

Posted by: Halloween Sid | September 8, 2010 3:22 PM

11

Many thanks, Ben W.

Posted by: Rokkaku/Ewan | September 8, 2010 4:26 PM

12

Ah, appreciate the responses. I feel less like there was some li'l something that was escaping me.

Posted by: gruebait | September 8, 2010 5:05 PM

13

A question for those who can handle both math and literature. The ISS orbits the Earth in 90 minutes, but we know from Shakespeare that Puck can "...put a girdle 'round the Earth in forty minutes" - or at least he claims he can: the evidence suggests he's more than a bit of a braggart. But taking his boast as fact, how does he do it?

Posted by: James | September 9, 2010 1:22 PM

14

Ur was right impresive but help me concernin d mass of d earth

Posted by: Kingsley emmanuel | December 13, 2010 9:26 PM

15

be coded along with something about 128 bit. With the

Posted by: Jean Prophete | July 11, 2011 3:43 AM

Post a Comment

(Email is required for authentication purposes only. On some blogs, comments are moderated for spam, so your comment may not appear immediately.)





ScienceBlogs

Search ScienceBlogs:

Go to:

Advertisement
Follow ScienceBlogs on Twitter

© 2006-2011 ScienceBlogs LLC. ScienceBlogs is a registered trademark of ScienceBlogs LLC. All rights reserved.