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Exoplanet Detection: Methods, Kepler Mission, and the Search for Habitable Planets, Slides of Geology

An overview of exoplanet detection methods, including the transit method, radial velocity wobble, and direct observation infrared. It also discusses the kepler mission and its goal to determine the statistical probability of earth-like planets in our galaxy. The document also touches on the search for habitable planets in the milky way and the role of black holes in galaxy structures.

Typology: Slides

2012/2013

Uploaded on 04/29/2013

arpanay
arpanay 🇮🇳

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Exoplanet detection (500+)
1
Gravitational attraction between a stellar mass
(sun) and planets (bigger the better, why?)
makes sun’s position wobble about barycenter.
Big question is: How many planets are in life-
zone where liquid water is stable?
Life zone is where a sun’s luminosity and a
planet’s orbital radius are correct: the green
zone below. The red zone is too hot (Mercury-
like) and the blue zone is to cold and makes
gaseous planets (Jupiter-like)
2 detected exoplanets
to scale for planet orbital
radius (planets not to
scale!)
Our solar system to scale
for Jupiter and Saturn
orbital radius
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Exoplanet detection (500+)

1

Gravitational attraction between a stellar mass (sun) and planets (bigger the better, why?) makes sun’s position wobble about barycenter.

Big question is: How many planets are in life- zone where liquid water is stable?

Life zone is where a sun’s luminosity and a planet’s orbital radius are correct: the green zone below. The red zone is too hot (Mercury- like) and the blue zone is to cold and makes gaseous planets (Jupiter-like)

2 detected exoplanets to scale for planet orbital radius (planets not to scale!)

Our solar system to scale for Jupiter and Saturn orbital radius

Exoplanet detection methods

2

Transit method: light dims

Radial velocity wobble (Doppler shift)

Direct observation infrared

Kepler mission (launched 2009): watching 100,000 nearby stars. We will know

statistical probability of earth-like planets (liquid water) in 4 years

4

The Kepler-scope: measure 100,000 stars brightness (photometry) at same time (wide view field) to find planets

The local structure of our Galaxy, the Milky Way. The stars sampled are similar to the immediate solar neighborhood. Young stellar clusters, ionized hydrogen (HII) regions and the neutral hydrogen (HI) distribution define the arms of the Galaxy.

3,000 light-year search of stars in Sagittarius Arm

5

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Galactic core black-hole sun motion for 8 yrs

10

Gravity is a busy force moving stuff around rapidly

Supermassive black holes at center of most all galaxies

11

Milky way galaxy center

Andromeda central SM blackhole