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Asteroids, Comets, & Meteors Chapter 6  Minor planets AKA “asteroids” – rocky objects in orbit around the sun  Usually not visible without telescope  Largest is ½ the size of the moon  Discovery of Minor Planets Many found by streak photography – timed photos so their movement makes a streak  so small they look like stars in telescope  Ceres – largest, discovered in 1801  Vesta – brightest   Most asteroids between orbits of Mars & Jupiter in “main asteroid” belt  Naming asteroids  Given name and number (by order of discovery) once orbit known  Ex:  1 Ceres Over 100,000 so given number of year discovered, then 2 letter suffix AA to ZZ  Family   A group of minor planets with a similar orbit Trojan asteroids Family with similar orbit as Jupiter  Same distance from Jupiter as from the sun   One group ahead and one group behind Jupiter  Apollo Asteroids Family with closest orbit to earth  Aphelion are >1ua, perihelions <1ua  Icarus has closest approach to sun (2ua)  Apollos tend to stay outside earth’s orbit   Aten family Moving 200 mph, perihelion <1ua, aphelion >1ua  Tend to stay inside earth’s orbit  Could collide with earth if earth’s gravity stretched asteroid’s orbit  Collisions unlikely (on different plane)   NEAT: Near Earth Asteroid Tracking program  Detects objects over 1 km in diameter near earth Homework: SRQ 6A 1-7 & Minor Planets Assignment
 
									 
									 
									 
									 
									 
									 
									 
									 
									 
									 
                                             
                                             
                                             
                                             
                                             
                                             
                                             
                                             
                                             
                                             
                                            