ASTRONOMY 1040


Class Notes #8

Chapter 9

Asteroids

      • Between Mars and Jupiter (and a few ranging from close to the Sun out to Jupiter and perhaps beyond) are hundreds of thousands of mostly rocky bodies too small to be planets. Most orbit in the so-called Asteroid Belt. The largest, Ceres, is about 1000 kilomneters  (600 miles) across, and the smallest ones merge into the meteoroid category (perhaps as small as a few tens of meters across)
      • Asteroids are interesting because, perhaps more even than planetary moons, they represent a very early era in the Solar System

Comets

      • Comets are small, icy bodies usually no more than a few miles across. Typically they orbit the Sun at great distances in two general reservoirs. The Kuiper Belt is just outside the orbit of Pluto, whereas the Oort Comet Cloud is perhaps halfway to the next nearest star.  Due to gravitational influences, a few comets fall in close to the Sun. When close to the Sun, our star's strong radiation turns some of the frozen gases back into gaseous (ionic) form. Some trapped dust is released from the gas as well. Radiation pressure and the Solar Wind causes the gas and dust to stream away from the comet, forming a tail. Radiation causes the gas to fluoresce (glow), and light from the Sun reflects off the dust to form and ion (gas) tail or a dust tail or both. The tail(s) always points away from the Sun, regard of direction of motion of the comet
      • Although the nuclei of comets are small, they can appear very large and impressive as they near the Sun. the gaseous head can grow to tens of thousands of miles across, and the tail can be 10s or even 100s of millions of miles long. Yet the only solid portion is the nucleus, which has sometimes been referrred to as a "dirty snowball" or a "dirty iceberg" because it is mostly ice with some sooty (carbon) or rocky material mixed in
      • Even more than moons or asteroids, comets represent an early stage of solar system evolution, and as such provide a window into the past and solar system formation

Meteoroids

      • Meteoroids are small icy or rocky bodies no more than a hundred meters across at most. (Actually there is no official dividing line between what is an asteroid and what is a meteoroid. My definition of a hundred meters is arbitrary and may be accepted by other authors.) Some of them have been  traced to the Asteroid Belt, whereas others appear to be related to comets (we have meteor showers annually when Earth crosses the orbit certain comets).
      • When meteoroids collide with Earth (at up to 50,000 miles per hour), they heat up with friction with the atmosphere. The incandescent object streaks through the sky and is called a meteor
      • If the meteoroid survives the trip through Earth's atmosphere and reaches the surface, it is called a meteorite
        • Meteorites come in three basic "flavors:"
          • Irons, which are typically about 90-95 percent iron and 5 -10 percent nickle. They are very heavy and unlike Earth rocks.
            • Sometimes the heating as they pass through the atmosphere causes thumblike depressions on their surfaces. They also usually have a thin crust, sometimes reddish with rust
            • When iron meteorites are cut open, polished flat and then etched with acid, they often show distinct pattering called the Widmanstatten Pattern, which are due to iron "crystals." This indicates that the meteoroid cooled very slowly inside another, larger object
          • Stones, which are very similar to Earth rocks in appearance. Although the majority of meteorites that reach the Earth are of the stone variety, fewer of them are found because they appear so much like Earth rocks
          • Stony Irons, which are the most rare of meteorites, and a combination of the other two types. they ahve a matrix of rocky material interspersed with iron

Pluto and (Kuiper Belt Objects)

      • Pluto is very unlike the full planets
        • Pluto has been demoted from planethood, and is now known as a "dwarf planet". To be a full-fledged planet, and object must be in an independent orbit around its star; must be large enough so that its own gravity can pull it into a spherical shape; and must have clear its orbit path of other objects. Pluto qualifies on the first two counts, but fails in the third. There has been an unusual amount of controversy and argument over this move
        • Pluto is small, considerably smaller than our Moon, about 2400 km (less than 1500 miles) in diameter
        • It is cold, hundreds of degrees below zero, and dark due to the vast distance from the Sun
        • At an average distance of 39.5 AU, Pluto is so far from the Sun that our star is little more than an exceedingly bright star
        • Pluto has a satellite (Charon) nearly half its own size (1190 km or about 740 miles in diameter)
        • It's surface is covered with icy nitrogen, methane and carbon monoxide
        • Unlike the Gas Giants, which are mostly atmosphere, Pluto has only an extremely thin atmosphere of nitrogen and methane. Even this freezes out when it is too cold
      • "Dwarf Planets," Kuiper Belt Objects and TNOs
        • Outward from just past the orbit of Neptune to perhaps twice as far as the orbit of Pluto is the Kuiper (KOY-per) belt, a region of cometary nuclei and small icy "dwarf planets" (including Pluto and the newly discovered Eris). Eris is just slighly larger than Pluto (about 100 km wider) and about twice as far from the Sun. Eris was the Greek goddess of chaos and discord, and it is said that the name was chosen to reflect the current status in the astronomical community about changing the status of Pluto. The only other "dwarf planet" currently is Ceres, formerly known as an asteroid.
        • The spacecraft "New Horizons" skirted past Jupiter in February, 2007 on its was to a rendezvous with Pluto in 2015, making it the first spacecraft from Earth ever to visit the dwarf planet
        • Pluto has a relatively large moon and several smaller ones, and Eris is known to have at least one moon, known as Dysnomia, the spirit of lawlessness
        • Several other  In recent years several relatively large objects have been discovered past Pluto. Since these are too small to be planets, and are unlike anything else, they are called Trans Neptunian Objects or TNOs and Kuiper Belt Objects or KBOs. Although you may encounter some defintions that attempt to distinguish differences between TNOs and KBOs, they are essentially the same objects
        • There are now several named Kuiper Belt Objects. Typically farther from the Sun than Pluto, there are several with names like Sedna, Orcas and Quoar
        • The Kuiper Belt objects may well be related to comets, although manty are much larger than any known cometary nucleus
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