Earth Acquires a Quasi-Moon 258
richard_za writes "Earth has acquired a so called quasi-moon, an asteroid: 2003 YN1, which will encircle us for the next couple of years while it orbits the sun on a horse-shoe shaped path. Full story on News24. It was found by team led by Paul Chodas, an asteroid specialist at Nasa's Jet Propulsion Laboratory in California. An orbit simulation can be seen in this Java applet."
no reg link... (Score:5, Informative)
Mike
Re:So it's not a threat (Score:5, Informative)
Catchy, but misleading headline. Still pretty neat, though.
Isn't it Cruithne??? (Score:4, Informative)
And this is a dupe from 4 years ago.
Earth's Second Moon [slashdot.org] 2nd Moon Orbiting Earth Discovered [slashdot.org]
Re:Isn't it Cruithne??? (Score:5, Informative)
Have the other two left already/have there been others in the past?
Re:Obligatory SW Quote (Score:1, Informative)
Re:I wonder... (distributed astronomy) (Score:5, Informative)
Not the first "quasi-moon" for Earth (Score:5, Informative)
This is the third asteroid we've found which has an orbit tied loosely to that of the Earth. The others are 3753 Cruithne and 2002 AA29. You can see pictures and applets and read about these other bodies at Paul Wiegert's web site:
http://www.astro.uwo.ca/~wiegert/ [astro.uwo.ca]
Re:I wonder... (Score:5, Informative)
The kind that you wouldn't be able to detect (except maybe by careful monitoring of the sun with a well-filtered telescope pointed at exactly the right spot). Imagine something much smaller than the moon and even farther away passing in front of the sun. That's what this is.
To experience a solar eclipse from a temporary sattelite would be a once-in-a-lifetime experience.
If it were noticeable. But temporary satellites (like the ISS) cast (highly-attenuated) shadows on the Earth every day.
Re:"Our" moon? (Score:5, Informative)
Re:Is it visible? (Score:5, Informative)
It is essentially invisible unless you have a decent research telescope.
More info on the astronomical magnitude scale can be found here
http://cfa-www.harvard.edu/icq/MagScale.html
Does the applet have correct orbits? (Score:3, Informative)
Re:Horseshoe? (Score:2, Informative)
Re:Does the applet have correct orbits? (Score:4, Informative)
You're very likely looking at a projection from above. Pluto's orbit is tilted about 30 degrees, so, from above, it will look closer than Neptune, but if you ran a tape measure out in a 3d universe, you'd see it was farther.
Re:Isn't it Cruithne??? (Score:4, Informative)
No, Cruithne is projected to be in our neighborhood for thousands of years.
"Earth has a second moon, of sorts, and could have many others, according to three astronomers who did calculations to describe orbital motions at gravitational balance points in space that temporarily pull asteroids into bizarre orbits near our planet.
"The 3-mile-wide (5-km) satellite, which takes 770 years to complete a horseshoe-shaped orbit around Earth, is called Cruithne and will remain in a suspended state around Earth for at least 5,000 years."
Space.com: More Moons Around Earth? It's Not So Loony [space.com]
Re:uh wha'zat? (Score:3, Informative)
Re:So it's not a threat (Score:5, Informative)
From a mathematical standpoint, it would be more appropriate to say that Luna orbits the Sun, rather than that it orbits the Earth.
That said, the Earth+Luna system still has a combined center of gravity which lies beneath the Earth's surface, so in that sense at least Luna is still Earth's satelite.
er, one question here, (Score:3, Informative)
Uh, wouldn't it be easier to fly an elliptical orbit?
Correct simulator link & other links (Score:3, Informative)
The simulator link is incorrect. It points to 2004 YN1. The correct link [nasa.gov]. For a good view in the simulator, tilt the 3D view to straight down, center on earth and zoom in all the way.
New Scientist has an interesting article [newscientist.com] in their latest issue.
For a more technical explanation, read the paper [usra.edu] presented at the Lunary Planetary Science Conference [usra.edu] last week.
Re:Is it visible? (Score:2, Informative)
With a little more specificity, if this object is m=24, then it's about (24-7)=17 magnitudes fainter than the *best* that the human eye can do. To put that into perspective, given that five magnitudes of difference is about 100x difference in actual brightness (~2.5^5), a difference of 17 magnitudes is *roughly* 5.8E6 (2.5^17) times fainter than the human eye is capable seeing in optimal, dark-sky conditions.
Also, see: International Dark-Sky Association [darksky.org]
I need to get out more... (Score:2, Informative)
The picture on the Discovery Channel coverage [discovery.com] is not the asteroid in question. I know this means I need to get out more, but I instantly recognized that picture as 243 Ida [nineplanets.org] and its tiny satellite Dactyl.
Re:space station (Score:4, Informative)
It works like this: picture a bucket on a recirculating rail. The rail is pretty long, hundreds of feet at least. The bucket meglevs along the rail.
There would be at least three railguns on the asteroid, pointing away from the asteroid in opposing directions. Actual orientation is not that important, what is important is that the rails point away.
In operation, the "bucket" stops at a point along the rail on the surface of the asteroid. Some mechanism plonks a pound or so of rock into the bucket. The bucket locks the material down.
The bucket now electromagnetically moves away to the railgun run. On reaching it, it accelerates. At an approprate time, it releases the payload. The bucket slows down, and returns to the loading point.
The process changes the the path of both the payload (reaction mass) and to the asteroid itself. Repeat this process millions of times, and you alter the asteroid's orbit.
The beauty part of a mass driver is that it has no moving parts in contact. You just need something to shovel in the reaction mass, and electricity to run the linear accelerators.
Asteroids can be moved in this manner. Rockets won't hack it, nor ion engines, nor nuclear explosions. Lack of control, or raw power.
We could shape the orbits of these Earth grazers to bring them a little closer to home so that we can exploit them for raw materials to build habitats, build ships, build elevators.
Space elevator projects require a large mass at the opposite end of the tether from the surface to anchor the cable. Asteroids have been suggested for the necessary mass. Mass drivers are the way to go if you want to get that mass.