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Habitability of the Goldilocks planet Gliese 581g: results from
Habitability of the Goldilocks planet Gliese 581g: results from

... Aims. In 2010, detailed observations have been published that seem to indicate another super-Earth planet in the system of Gliese 581, which is located in the midst of the stellar climatological habitable zone. The mass of the planet, known as Gl 581g, has been estimated to be between 3.1 and 4.3 M⊕ ...
What Makes a Planet Habitable?
What Makes a Planet Habitable?

Alone in the Universe - Let There Be Light : The Book
Alone in the Universe - Let There Be Light : The Book

... candidates (planets not yet completely confirmed) that orbit in less than 50 days, University of California at Berkeley astrophysicist Andrew Howard and his team analyzed the trends they represent, including the finding that smaller planets are more abundant. There ...
Chapter 4 Practice Questions
Chapter 4 Practice Questions

... a) a planet that once orbited the Sun but later was destroyed. b) ancient material from the formation of the solar system. c) a collision between Jupiter and one of its larger moons. d) comets that were trapped by Jupiter’s gravitational field. ...
Condensation of the Solar Nebula
Condensation of the Solar Nebula

... The research team estimates the mass of the brown dwarf at 55 to 78 times the mass of planet Jupiter. The discovery raises puzzling questions about how the brown dwarf formed, and it adds to the surprising diversity of extrasolar planetary systems being found with cutting-edge observational techniqu ...
SETI: First Considerations (PowerPoint)
SETI: First Considerations (PowerPoint)

... Numbers of Stars The Milky Way is forming about one new star a year, and an ‘average’ star (like the Sun) might last about ten billion years. In the ‘steady state,’ there will be at least several billion radiating stars out there. Stars much more massive than the Sun burn up their fuel very quickly, ...
Document
Document

document
document

By plugging their latest findings into Earth`s climate patterns
By plugging their latest findings into Earth`s climate patterns

... When analyzing a star’s light, scientists look for spectral “fingerprints,” a pattern of colors different for every individual element, to determine that star’s composition. This process, called spectroscopy, is also useful for determining the chemical makeup of exoplanets and their atmospheres when ...
DAY AND NIGHT, SEASONS
DAY AND NIGHT, SEASONS

... slowly. The time it takes to complete a rotation about its axis is equal to the time it takes to complete an orbit. Its day is as long as its year. Whether the planet experiences any seasonal variations or day-night cycles depends on the tilt of the planets axis. You may choose to limit the discussi ...
Comparative Planetology
Comparative Planetology

The closest extrasolar planet: A giant planet around the M4 dwarf Gl
The closest extrasolar planet: A giant planet around the M4 dwarf Gl

... Fig. 1. Combined ELODIE and CORALIE radial velocities for Gl 876. The solid line is the radial velocity curve for the orbital solution. entirely consistent, and this parameter was thus held fixed to zero for the final solution. Figure 1 shows the individual radial velocity measurements as a function ...
Lecture17-ASTA01
Lecture17-ASTA01

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PH709-10-asn1ans

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Goal: To understand life in our universe.
Goal: To understand life in our universe.

Johannes Kepler
Johannes Kepler

File - We All Love Science
File - We All Love Science

... – Uranus tilts almost to orbital plane – Venus tilts so much it spins “backwards” • Retrograde, but orbits with other planets ...
Chapter 2 Astronomy Notes
Chapter 2 Astronomy Notes

... moons, the plutinos, and all other objects close to its orbit. In 2003, the IAU had also released an official statement that differentiated planets from stars and other massive objects. This is the part of the statement that pertains to planets: Objects with true masses below the limiting mass for t ...
Our Solar System
Our Solar System

Presentation
Presentation

AST 101 Final Exam DO NOT open the exam until
AST 101 Final Exam DO NOT open the exam until

... 20.) You are watching TV in the year 3014, and an ad for a new weight less plan comes on. The plan has you go to the distant planet ”Weightlossian”, which is larger in size than the Earth, but has a much smaller mass than the Earth. The advertisement boasts that you’ll have shed pounds the moment yo ...
Solar System: ground-based
Solar System: ground-based

... • Planetary atmospheres: composition => thermal properties, mass, age – VLT, OWL => high-res spectra; complements JWST NIR, MIRI spectrophotometry and ...
Test - Scioly.org
Test - Scioly.org

Planets - uni
Planets - uni

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Exoplanetology

Exoplanetology, or exoplanetary science, is an integrated field of astronomical science dedicated to the search and study of exoplanets (extrasolar planets). It employs an interdisciplinary approach which includes astrobiology, astrophysics, astronomy, astrochemistry, astrogeology, geochemistry, and planetary science.
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