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Chapter 29
Chapter 29

... light from short to long wavelengths ...
31_Finding Earths
31_Finding Earths

Astronomy Basics
Astronomy Basics

... Beyond the frost line, planetesimals can grow from rock and ice. This leads to the formation of “planetary cores”, which are rocky/icy planetesimals around 10x as massive as Earth. These cores are so massive that they accrete gas, forming gas giant planets. ...
File
File

Farthest Known Planet Opens the Door for Finding New Earths
Farthest Known Planet Opens the Door for Finding New Earths

... • We will use MOST to detect the reflected light from known “hot Jupiters”; • The details of the reflected light will tell us about the particle size & composition of the planet’s clouds. ...
Big Bang
Big Bang

... Spectral Signature of Life • Particularly, spectroscopic observation is a powerful tool to investigate the chemical composition of exoplanets. • Not only on Earth but also in the interstellar space, carbon exists abundantly in several oxidized (e.g., CO2) and reduced (e.g., CH4), forms. This allows ...
Document
Document

... *** The third method is based on detecting the small drop in apparent luminosity of a star as a planet transits in front of it, between the star and the Earth. ...
Ch 10 Slide Show
Ch 10 Slide Show

...  Allowed him to see objects about 20x closer. ...
Solar System and Astronomy puzzle 001
Solar System and Astronomy puzzle 001

... a star system consisting of two stars orbiting around their common center of mass 10. natural satellite 12. a massive, gravitationally bound system consisting of stars, stellar remnants, an interstellar medium of gas and dust 13. growth of a massive object by gravitationally attracting more matter ...
Cat`s EyE - Chandra X
Cat`s EyE - Chandra X

ch. 5 study guide
ch. 5 study guide

... o What is a meteorite? a meteor that hits the earth o Know all of the following about the outer planets. (You will be asked to identify one which is not true about them.) They are the farthest from the Sun. They are all bigger than the inner planets. They all have rings. o The Sun is a medium-sized ...
2b Astronomer space units
2b Astronomer space units

Star Constellations - rosedalegrade9astronomy
Star Constellations - rosedalegrade9astronomy

Starshade - Northrop Grumman Corporation
Starshade - Northrop Grumman Corporation

... model occulters to prove that the Starshade functions as expected. Component hardware has been built to determine the state-of-the-art capability to produce the required structure. ...
Grade 9 Academic Science – Space
Grade 9 Academic Science – Space

... Grade 9 Academic Science – Space ...
Astronomy and Space articles by Martin George of the Launceston
Astronomy and Space articles by Martin George of the Launceston

... Many readers, no doubt, have watched one or more of the famous science fiction movies or series, with spectacular planetary landscapes and weird atmospheric effects. Some of them have two moons in the sky - quite a possible scenario for some planets, although we of course have only one. Another type ...
File
File

... 9. What is the largest object in the solar system? The sun 10. Which way does Venus rotate? North and south (like rolling a ball) 11. What is the hottest planet in the solar system? Venus 12. What is Earth’s atmosphere made of? Water vapor and other gases 13. What features do the inner planets share ...
22.2 Stars Change Over Their Life Cycles
22.2 Stars Change Over Their Life Cycles

... Stars Change Over Their Life Cycles ...
Are we Alone? The Search for Life Beyond the
Are we Alone? The Search for Life Beyond the

... • They observed Tau Ceti and Epsilon Eridani for a total of two months, but only detected the, then top secret, U2 Spy plane! ...
Powerpoint file
Powerpoint file

... The CoRoT Ground-based Follow-up Effort CoRoT only finds transit „candidates“. An extensive ground-based effort is required to confirm that this is indeed a planet. For Space-based transit searches, Ground-based observations are „part of the Mission“ But before the ground-based follow up starts one ...
Skymapper and Kepler K2: Finding the Origin of Hot Gas Giants
Skymapper and Kepler K2: Finding the Origin of Hot Gas Giants

Extrasolar planets
Extrasolar planets

... • The radial velocity method can only detect massive planets (at least one-fifth of the mass of Jupiter) with relatively short periods. • Most planets are detected very close to their stars (less than ~0.1AU) ...


... method (see graphic), which picks up slight wobbles in a star’s position caused by the gravitational tug of an orbiting planet. This method is most likely to find large planets close to their stars, however. Transits are better suited to finding something more like Earth in size and orbit. So far, 5 ...
Homework 7
Homework 7

... between the terrestrial and Jovian planets? ...
PHYSICS DEPARTMENT Syllabus: Phys 200 (3 cr
PHYSICS DEPARTMENT Syllabus: Phys 200 (3 cr

... Stellar Evolution and the Death of Stars Birth of stars. Evolution from the main-sequence to Red Giants. Testing stellar evolution using observed star clusters. Evolution to white Dwarfs, Neutron Stars or Black Holes. ...
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