The Family of Stars
... Extra-Solar Planets • Hard to see faint planet right next to very bright star • Two main indirect techniques available (Like a binary star system but where 2nd “star” has extremely low mass) – Watch for Doppler “wobble” in position/spectrum of star – Watch for “transit” of planet which slightly dim ...
... Extra-Solar Planets • Hard to see faint planet right next to very bright star • Two main indirect techniques available (Like a binary star system but where 2nd “star” has extremely low mass) – Watch for Doppler “wobble” in position/spectrum of star – Watch for “transit” of planet which slightly dim ...
PowerPoint
... Exploring (Earth-like) Exoplanets • RV search for new low-mass planets • Transit follow-up studies • Gravitational microlensing follow-up studies • Direct imaging studies ...
... Exploring (Earth-like) Exoplanets • RV search for new low-mass planets • Transit follow-up studies • Gravitational microlensing follow-up studies • Direct imaging studies ...
Lecture (Powerpoint)
... mass (more on that next week) Can planets have reasonable orbits in such systems? Yes, but must orbit one star or be far away from both; `Figure 8’ orbits aren’t stable ...
... mass (more on that next week) Can planets have reasonable orbits in such systems? Yes, but must orbit one star or be far away from both; `Figure 8’ orbits aren’t stable ...
Unit 2 Study Guide - Grant County Schools
... LT2.1: I can describe parts of the solar system Because the Solar System is so big, it is hard to create something on Earth that represents them. We make scale models of the size and distances in space. Students should be able to look at pictures of scale models and explain how the sizes and distanc ...
... LT2.1: I can describe parts of the solar system Because the Solar System is so big, it is hard to create something on Earth that represents them. We make scale models of the size and distances in space. Students should be able to look at pictures of scale models and explain how the sizes and distanc ...
Unit 2 Study Guide (word)
... LT2.1: I can describe parts of the solar system Because the Solar System is so big, it is hard to create something on Earth that represents them. We make scale models of the size and distances in space. Students should be able to look at pictures of scale models and explain how the sizes and distanc ...
... LT2.1: I can describe parts of the solar system Because the Solar System is so big, it is hard to create something on Earth that represents them. We make scale models of the size and distances in space. Students should be able to look at pictures of scale models and explain how the sizes and distanc ...
January 23
... • Simpler definition - A “large” object that orbits a star and shines primarily by reflecting light from its star. ...
... • Simpler definition - A “large” object that orbits a star and shines primarily by reflecting light from its star. ...
Circumstellar habitable zone
In astronomy and astrobiology, the circumstellar habitable zone (CHZ), or simply the habitable zone, is the region around a star within which planetary-mass objects with sufficient atmospheric pressure can support liquid water at their surfaces. The bounds of the CHZ are calculated using the known requirements of Earth's biosphere, its position in the Solar System and the amount of radiant energy it receives from the Sun. Due to the importance of liquid water to life as it exists on Earth, the nature of the CHZ and the objects within is believed to be instrumental in determining the scope and distribution of Earth-like extraterrestrial life and intelligence.The habitable zone is also called the Goldilocks zone, a metaphor of the children's fairy tale of Goldilocks and the Three Bears, in which a little girl chooses from sets of three items, ignoring the ones that are too extreme (large or small, hot or cold, etc.), and settling on the one in the middle, which is ""just right"".Since the concept was first presented in 1953, stars have been confirmed to possess a CHZ planet, including some systems that consist of multiple CHZ planets. Most such planets, being super-Earths or gas giants, are more massive than Earth, because such planets are easier to detect. On November 4, 2013, astronomers reported, based on Kepler data, that there could be as many as 40 billion Earth-sized planets orbiting in the habitable zones of Sun-like stars and red dwarfs in the Milky Way. 11 billion of these may be orbiting Sun-like stars. The nearest such planet may be 12 light-years away, according to the scientists. The CHZ is also of particular interest to the emerging field of habitability of natural satellites, because planetary-mass moons in the CHZ might outnumber planets.In subsequent decades, the CHZ concept began to be challenged as a primary criterion for life. Since the discovery of evidence for extraterrestrial liquid water, substantial quantities of it are now believed to occur outside the circumstellar habitable zone. Sustained by other energy sources, such as tidal heating or radioactive decay or pressurized by other non-atmospheric means, the basic conditions for water-dependent life may be found even in interstellar space, on rogue planets, or their moons. In addition, other circumstellar zones, where non-water solvents favorable to hypothetical life based on alternative biochemistries could exist in liquid form at the surface, have been proposed.