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Consequences for Detection

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Presentation on theme: "Consequences for Detection"— Presentation transcript:

1 Consequences for Detection
Asteroid Albedos & Consequences for Detection by NEA Survey Programs Contributed by Eric B. Grosfils Pomona College

2 Astronomy: Sky Surveys
Great idea! But not so simple in practice… It’s a big solar system out there! Trade off between detection size limit and survey speed/effectiveness. Asteroids are dark… much like asteroid Eros (10 km x 30 km) shown here (it really is here, even if you cannot see it) with albedos of a few percent, think looking for lumps of coal set against the black vastness of space! Eros’ Albedo: 5% Goals and problems with sky survey… Flip through next few slides to illustrate why albedo poses such a large problem!

3 Astronomy: Sky Surveys
10% 10%

4 Astronomy: Sky Surveys
20% 20%

5 Astronomy: Sky Surveys
30% 30%

6 Astronomy: Sky Surveys
40% 40%

7 Astronomy: Sky Surveys
50% 50%... You get the point!


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