'Giant planets' presentation slideshows

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Some planets are closer to the sun* than others…

Some planets are closer to the sun* than others…

Some planets are closer to the sun* than others…. *the solar system ’ s “ heater ”. hottest. coldest. What are the characteristics of the gas giant planets?. Gas giant planets. Surface temperatures of gas giant planets. What are the characteristics of the gas giant planets?.

By JasminFlorian
(198 views)

آموزش طراحی وب سایت جلسه دوازدهم – جاوا اسکریپت 3

آموزش طراحی وب سایت جلسه دوازدهم – جاوا اسکریپت 3

آموزش طراحی وب سایت جلسه دوازدهم – جاوا اسکریپت 3. تدریس طراحی وب برای اطلاعات بیشتر تماس بگیرید تاو شماره تماس: 09125773990 09371410986 پست الکترونیک : TargetLearning@gmail.com. Web Design Training Java Scripts #3. Part 12 Author :Babak Tavatav. Array Object.

By merritt
(211 views)

2 pt

2 pt

Stars. Galaxies. The Sun. Planets. Meteors, Etc. 1 pt. 1 pt. 1 pt. 1 pt. 1 pt. 2 pt. 2 pt. 2 pt. 2 pt. 2 pt. 3 pt. 3 pt. 3 pt. 3 pt. 3 pt. 4 pt. 4 pt. 4 pt. 4 pt. 4 pt. 5 pt. 5 pt. 5 pt. 5 pt. 5 pt. A hot, glowing sphere of gas that produces energy by fusion.

By yon
(140 views)

Sculpting Circumstellar Disks

Sculpting Circumstellar Disks

Sculpting Circumstellar Disks. Alice Quillen University of Rochester. Netherlands April 2007. Motivations. Planet detection via disk/planet interaction – Complimentary to radial velocity and transit detection methods Rosy future – ground and space platforms

By candide
(140 views)

Giant Planets

Giant Planets

Giant Planets. Jupiter, Saturn, Uranus, Neptune. Size Comparison. Jupiter: 318 Earth-masses, Saturn: 95, Uranus: 14.5, Neptune: 17.2. Two subclasses: Jupiter-Saturn and Uranus-Neptune. Terrestrial planets low mass high density slow rotators (  24 hours) few satellites

By donelle
(162 views)

Assessing the Threat of Oort Cloud Comet Showers

Assessing the Threat of Oort Cloud Comet Showers

Assessing the Threat of Oort Cloud Comet Showers. Nathan Kaib & Tom Quinn University of Washington. Outline. Long-Period Comet Production Jupiter-Saturn Barrier Simulation Results Comet Shower Probability. Long-Period Comets. X. 25000 AU. Jupiter-Saturn Barrier.

By posy
(110 views)

Creating a Good Power Point Presentation

Creating a Good Power Point Presentation

Creating a Good Power Point Presentation. Career Technology. What is wrong with the following slides?. Are there Any Interesting Features About my Planet?. Mercury is the smallest planet Mercury has HUNDREDS of craters! The largest crater is called beethoven at 643 km.

By giulio
(87 views)

Open problems in terrestrial planet formation

Open problems in terrestrial planet formation

Open problems in terrestrial planet formation. Sean Raymond Laboratoire d’Astrophysique de Bordeaux. …with audience contributions welcome!. How did the Solar System form?.

By gwidon
(124 views)

TPF/Darwin

TPF/Darwin

TPF/Darwin. Terrestrial Planet Finder Coronagraph: 0.5-0.8 microns 6.5 x 3 m 8 x 7 m Interferometer: 6.5-13 microns 36m, 4x3.2m 70-150m baseline, 4x4m. Structurally-Connected Interferometer. Dual-chopped Bracewell 36 m array Four apertures, 3.2 m diameter

By idalee
(144 views)

Reflection Spectra of Giant Planets With an Eye Towards TPF (and EPIC & ECLIPSE)

Reflection Spectra of Giant Planets With an Eye Towards TPF (and EPIC & ECLIPSE)

Reflection Spectra of Giant Planets With an Eye Towards TPF (and EPIC & ECLIPSE) Jonathan J. Fortney Mark S. Marley NASA Ames Research Center 2005 Aspen Winter Conference on Astrophysics: Planet Formation and Detection February 11, 2005. EGP Characterization with an Eye Towards TPF-C.

By cody
(111 views)

The Pluto System in the Context of Kuiper Belt Formation & Evolution

The Pluto System in the Context of Kuiper Belt Formation & Evolution

The Pluto System in the Context of Kuiper Belt Formation & Evolution. A. Morbidelli (OCA – Nice). THIS TALK WILL FOCUS ON THE DYNAMICAL ASPECTS OF THE KUIPER BELT EVOLUTION

By jenaya
(117 views)

PX437 EXOPLANETS

PX437 EXOPLANETS

PX437 EXOPLANETS. Peter Wheatley (PS009) p.j.wheatley@warwick.ac.uk. Outline. Before Exoplanets Detecting exoplanets Direct imaging Reflex Motion of Star Transiting exoplanets Planet Formation Extra-Terrestial Life. Terrestrial planets. Gas giants. Ice giants. Asteroid belt.

By dacian
(178 views)

Solar-system observations with Herschel/ALMA

Solar-system observations with Herschel/ALMA

Solar-system observations with Herschel/ALMA. T. Encrenaz, D. Bockelée-Morvan, J. Crovisier, E. Lellouch LESIA, Observatoire de Paris. Outline. Why the far-IR/submm/mm range? Major objectives of solar-system research Venus, Mars and the giant planets Satellites, distant asteroids and TNOs

By rufina
(124 views)

Ge/Ay133

Ge/Ay133

Jovian planet formation. Core-accretion or gravitational instability?. Ge/Ay133. Properties of the Jovian Planets in the Solar System. P  r 2 for H 2 -He I/MR 2 =0.4 for a uniform sphere I/MR 2 =0.26 for P  r 2.

By butch
(146 views)

Alessandro Morbidelli (OCA, Nice) Kevin Walsh (SWRI, Boulder) Sean Raymond (CNRS, Bordeaux)

Alessandro Morbidelli (OCA, Nice) Kevin Walsh (SWRI, Boulder) Sean Raymond (CNRS, Bordeaux)

The Grand Tack Scenario: Reconstructing The Migration History Of Jupiter And Saturn In The Disk Of Gas. Alessandro Morbidelli (OCA, Nice) Kevin Walsh (SWRI, Boulder) Sean Raymond (CNRS, Bordeaux) David O’Brien (PSI, Tucson) Avi Mandell (NASA Goddard).

By nuri
(196 views)

Different Flavors of Planet Formation

Different Flavors of Planet Formation

By akamu
(221 views)

WITNESSING PLANET FORMATION WITH ALMA AND THE ELTs

WITNESSING PLANET FORMATION WITH ALMA AND THE ELTs

WITNESSING PLANET FORMATION WITH ALMA AND THE ELTs. Transition disk. Typical SED of CTTS disk. Cieza et al. (2010).

By dyan
(90 views)

Catching Planets in Formation with GMT

Catching Planets in Formation with GMT

Catching Planets in Formation with GMT. What sets the stellar/substellar mass function and how universal is it? Do all stars form planets and if not, why not? What causes the diversity of planetary systems?. SPECIMEN. Nearby Star Forming Regions. Good News: Most are in the South

By shaw
(79 views)

Planetary Lunch Seminar Fall 2012 Seminar Series

Planetary Lunch Seminar Fall 2012 Seminar Series

Planetary Lunch Seminar Fall 2012 Seminar Series. Yu-Cian Hong Cornell, Astronomy. Larry ’ s Lookout. Jibsheet. Image Credit: Avatar. Orbital Stability of Exomoons of Giant Planets in Planet-planet Scattering Monday, October 29th, 2012 12:30 pm, 622 Space Sciences.

By adin
(149 views)

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

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:.

By vanida
(99 views)

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