hour 3: star and planet formation, history of our solar system, planets around other stars...

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Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks & Solar System Formation Two Kinds of Planets & the Condensation Sequence Era of Heavy Bombardment - Frustration of Life ? Extrasolar Planets & the “Hot Jupiter” Puzzle

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Page 1: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Hour 3: Star and Planet Formation,History of our Solar System,Planets Around Other Stars

• Interstellar Clouds & Star-Forming Regions• Protoplanetary Disks & Solar System Formation• Two Kinds of Planets & the Condensation Sequence• Era of Heavy Bombardment - Frustration of Life ?• Extrasolar Planets & the “Hot Jupiter” Puzzle

Page 2: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Take-aways:• Clouds of material between the stars are sites of stars formation• Earth plus the other planets in our solar system evidently formed

from a disk around the Sun as it formed; such protoplanetary disks are seen around many young stars

• Planets like Earth are believed therefore to form as normal by-products of stars forming

• There are two types of planets in our solar system, Earth-likeand Jupiter-like, results of a process we think we understand

• Almost 200 planets have now been found around other stars, but those planetary systems often have “hot Jupiters” - is our solar system weird, or are those systems weird ?

• All the planets sustained heavy bombardment from remnant construction material soon after they formed; that may have set the timescale for the beginning of life on Earth

Page 3: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Interstellar Cloudsand Star-forming Regions

Page 4: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

The OrionNebula:

An ActiveStar-FormingRegion

Page 5: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Constellation Orionleft: visual wavelength image

right: far-infrared image

Page 6: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

p.194c

Page 7: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

p.195b

Page 8: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

p.194b

Page 9: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

GlobulesEvaporating gaseous globules (“EGGs”): Newly forming stars

exposed by the ionizing radiation from nearby massive stars

Page 10: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

p.177b

Page 11: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

p.177d

Page 12: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Globules

Bok globules:

~ 10 – 1000 solar masses;

Contracting to form protostars

Page 13: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Shocks Triggering Star Formation

Henize 206 (infrared)

Page 14: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Protoplanetary Disks & Solar System Formation

Page 15: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 1-7, p.7

Page 16: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

p.364a

Page 17: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Table 16-1, p.367

Page 18: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 16-1, p.357

Page 19: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 16-2, p.358

Page 20: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 16-3, p.358

Page 21: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Two Kinds of Planets &The Condensation Sequence

Page 22: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Two Kinds of PlanetsPlanets of our solar system can be divided

into two very different kinds:

Terrestrial (earthlike) planets: Mercury, Venus, Earth, Mars

Jovian (Jupiter-like) planets: Jupiter, Saturn, Uranus, Neptune

Page 23: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Table 16-3, p.369

Page 24: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Asteroids

Last remains of planetesimals that built the planets 4.6 billion years

ago!

Small, irregular objects,

mostly in the apparent gap between the

orbits of Mars and Jupiter.

Page 25: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 16-7, p.363

Page 26: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

The Geology of Comet NucleiComet nuclei contain ices of water, carbon dioxide, methane, ammonia, etc.:

Materials that should have condensed from the outer solar nebula.

Those compounds

sublime (transition from solid directly to gas phase) as

comets approach the

sun. Densities of comet

nuclei: ~ 0.1 – 0.25 g/cm3

Not solid ice balls, but fluffy material with

significant amounts of empty space.

Page 27: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 16-4c, p.359

Page 28: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Extrasolar Planets &the “Hot Jupiter” Puzzle

Page 29: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 16-5, p.360

Page 30: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks
Page 31: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Artist’s Conception HD 209458

Planet passing in front of parent star -- size indicates density like Jupiter

Page 32: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Hot Jupiters:

• They seemingly go against the neat “Condensation Sequence” theory that seems to explain our solar system’s arrangement

• Did the “Hot Jupiters” form “cold”, i.e. at the expected location beyond the “ice line”, and then migrate toward the Sun ?

• If so, wouldn’t that destroy any Earth-like planets ?• In our system Jupiter did NOT migrate -- is our system weird

or are the Hot Jupiter systems the unusual ones, but just easier to detect with present technology ?

Page 33: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Era of Heavy Bombardment - Frustration of Life ?

Page 34: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 16-13b, p.374

Page 35: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

p.389c

Page 36: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 17-9, p.394

Page 37: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Fig. 18-3, p.424

Page 38: Hour 3: Star and Planet Formation, History of our Solar System, Planets Around Other Stars Interstellar Clouds & Star-Forming Regions Protoplanetary Disks

Take-aways:• Clouds of material between the stars are sites of stars formation• Earth plus the other planets in our solar system evidently formed

from a disk around the Sun as it formed; such protoplanetary disks are seen around many young stars

• Planets like Earth are believed therefore to form as normal by-products of stars forming

• There are two types of planets in our solar system, Earth-likeand Jupiter-like, results of a process we think we understand

• Almost 200 planets have now been found around other stars, but those planetary systems often have “hot Jupiters” - is our solar system weird, or are those systems weird ?

• All the planets sustained heavy bombardment from remnant construction material soon after they formed; that may have set the timescale for the beginning of life on Earth