The Speculist: Just a Pile of Gravel?

logo.jpg

Live to see it.


« Pura Vida | Main | It's a New Phil, Week 22 »


Just a Pile of Gravel?

Very interesting:

The small asteroid Itokawa is just a loosely packed pile of rubble that collected after a collision between asteroids, according to a slew of new studies based on data from Japan's Hayabusa spacecraft. The asteroid appears to be plagued by recurring impacts and tremors today, making its continued survival a mystery.

Hayabusa made two attempts to collect samples from the 535-metre-long space rock in November 2005. The attempts appear to have failed, but that will not be clear unless the spacecraft can be returned to Earth, which scientists are hoping to do in 2010. But during its approach, the spacecraft did take images and other data on Itokawa's topology, composition and gravity field.

According to the article, the asteroid is 40% porous, compared with a handful of sand which is about 20% porous. Over time, one would expect that it would have collided with other objects, either breaking it apart or condensing it together. It's current form seems highly unlikely.

(Continued / Comments after advertisement.)

Comments

Let me throw out this scenario:

Two asteriods collide, one is wiped out, the other, a porous rock, is damaged, but a large chunk of it survived intact. The particles from the wiped out asteriod are attracted back by the large chunk's gravity. You end up with an asteriod that is sandy on the outside, with a porous chunk on the inside.

Maybe this happened recently enough that it hasn't had a chance to either break apart or condense further.

Post a comment

(If you haven't left a comment here before, you may need to be approved by the site owner before your comment will appear. Until then, it won't appear on the entry. Thanks for waiting.)






Be a Speculist

Share your thoughts on the future with more than

70,000

Speculist readers. Write to us at:

speculist1@yahoo.com

(More details here.)



Blogroll



Categories

Powered by
Movable Type 3.2