'Giant planet' presentation slideshows

Radial Velocity Detection of Planets: II. Results

Radial Velocity Detection of Planets: II. Results. To date 1783 exoplanets have been discovered ca 558 planets discovered with the RV method. The others are from transit searches 98 are in Multiple Systems (RV). ? exoplanet.eu. Campbell & Walker: The Pioneers of RV Planet Searches. 1988:.

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Radial Velocity Detection of Planets: II. Observations

Radial Velocity Detection of Planets: II. Observations. Period Analysis Global Parameters Classes of Planets Dependence on Stellar Parameters Sources of Noise. Lecture notes: www.tls-tautenburg.de. Click on Teaching -> lectures -> Extrasolar Planets. Binary star simulator:.

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Lesson 9b extra-planets

Lesson 9b extra-planets. Origin of the Solar System And extra-solar planets. In the inner solar system it was cool enough for iron and silicate compounds to form and make rocky material. But not cool enough for ice to accumulate. The inner planets were devoid of these volatile compounds. .

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The Doppler Method, or the Radial Velocity Detection of Planets: II. Results

The Doppler Method, or the Radial Velocity Detection of Planets: II. Results. Campbell & Walker: The Pioneers of RV Planet Searches. 1988:.

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The Doppler Method, or the Radial Velocity Detection of Planets: II. Results

The Doppler Method, or the Radial Velocity Detection of Planets: II. Results. Campbell & Walker: The Pioneers of RV Planet Searches. 1988:.

562 views • 46 slides

The Doppler Method, or the Radial Velocity Detection of Planets: II. Results

The Doppler Method, or the Radial Velocity Detection of Planets: II. Results. Campbell & Walker: The Pioneers of RV Planet Searches. 1988:.

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Frontier Science Enabled by a Giant Segmented Mirror Telescope

Frontier Science Enabled by a Giant Segmented Mirror Telescope. Rolf-Peter Kudritzki 1 for the GSMT Science Working Group 1 Chair, GSMT Science Working Group Institute for Astronomy, University of Hawaii. http://www.aura-nio.noao.edu/gsmt_swg/SWG_Report/SWG_Report_7.2.03.pdf.

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The Origin of Gaps and Holes in Transition Disks Uma Gorti (SETI Institute)

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Solar System Formation

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Galactic Base

Galactic Base. Culture. Bypass. Interstellar Biosphere. 10. 10. 10. 10. 10. 10. Supergiant. 30. 30. 30. 30. 30. 30. Supernova. Culture. Dryport. ?. ?. Desolation Landing. Desert World. Ice Station. ?. ?. Culture. ?. ?. Ice Planet. Rainfall. Culture. 10. 10. 10.

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STScI May Symposium 2005

Phil Armitage (University of Colorado). Migration. Migration regimes Time scale for massive planet formation Observational signatures. Ken Rice (UC Riverside) Dimitri Veras (Colorado). + Mario Livio, Steve Lubow & Jim Pringle. STScI May Symposium 2005. Migration.

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Peering into the Birthplaces of Solar Systems

Early ALMA and EVLA Observations of Circumstellar Disks. Peering into the Birthplaces of Solar Systems. K. Teramura UH IfA. David J. Wilner. Atacama Large Millimeter/ submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Large Baseline Array.

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Star W Grant

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On the Frequency of Gas Giant Planets in the Metal-Poor Regime

On the Frequency of Gas Giant Planets in the Metal-Poor Regime. Alessandro Sozzetti 1 , D.W. Latham 2 , G. Torres 2 , R.P. Stefanik 2 , S.G. Korzennik 2 , A.P. Boss 3 , B.W. Carney 4 , J.B. Laird 5 (1) INAF/OATo - (2) CfA - (3) CIW - (4) UNC - (5) BGSU.

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Which number (from 1 to 9) is your planet from the Sun?

Which number (from 1 to 9) is your planet from the Sun?. Saturn is the sixth planet from the Sun. What does it look like inside?

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Planets and Other Planetary Bodies

Planets and Other Planetary Bodies. By Carter Perry. Our Solar System. 1: The Sun 2: Mercury 3: Venus 4: Earth 5: Mars 6: Jupiter 7: Saturn 8: Uranus 9: Neptune. Pluto and beyond are either Dwarf Planets. Mercury. Mercury is the smallest of all the planets in our solar system.

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Probing for Puny Planets

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Saturn is the messenger of gods

Saturn is the messenger of gods. Saturn is not a solid planet like earth is. Saturn is one of the largest planets in the solar system. Saturn takes about 29 years to orbit the sun once.

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