solar_notes_Feb11
... OA = 1 Astronomical Unit = 1.5*108 km Perihelion Distance = 1.471*108 km Aphelion Distance = 1.522*108 km ...
... OA = 1 Astronomical Unit = 1.5*108 km Perihelion Distance = 1.471*108 km Aphelion Distance = 1.522*108 km ...
Formation of the Solar System • Questions
... of formation of solar system. • Primitive meteorites have very narrow range of ...
... of formation of solar system. • Primitive meteorites have very narrow range of ...
extra
... Viscous stirring: exchange of momentum can also be achieved by extracting from /adding to the Keplerian potential (random energy not preserved, three-body effect) ...
... Viscous stirring: exchange of momentum can also be achieved by extracting from /adding to the Keplerian potential (random energy not preserved, three-body effect) ...
Recognition of Climate Variability within South Florida
... high geomagnetic activity (average Cp value for the nine months prior to the wet season). Quartiles of Lake inflow for the lowest and highest terciles of geomagnetic activity are illustrated in Figure 1. The various combinations of high or low geomagnetic activity are paired to either a strong or w ...
... high geomagnetic activity (average Cp value for the nine months prior to the wet season). Quartiles of Lake inflow for the lowest and highest terciles of geomagnetic activity are illustrated in Figure 1. The various combinations of high or low geomagnetic activity are paired to either a strong or w ...
Alessandro Bettini Introduction to Elementary Particle Physics
... There is a large difference between an electron and proton accelerator: electrons emit synchrotron radiation (SR) when they bend. For a 10 GeV/c electron in a 1 km radius ring, the SR loss is about 1 MeV/turn. ...
... There is a large difference between an electron and proton accelerator: electrons emit synchrotron radiation (SR) when they bend. For a 10 GeV/c electron in a 1 km radius ring, the SR loss is about 1 MeV/turn. ...
1.1 Organization of the Universe
... Order these vocabulary words from largest to smallest: solar system, universe, galaxy, planet What is the difference between the geocentric and the heliocentric model? Which one is ...
... Order these vocabulary words from largest to smallest: solar system, universe, galaxy, planet What is the difference between the geocentric and the heliocentric model? Which one is ...
Tuesday Nov 14 Agenda Saturn`s Hurricane
... • They were further from the Sun and gravity was weaker • They formed beyond the frost line where ices can condense so they included hydrogen compounds • They were far enough from the Sun to escape the heavy bombardment that battered the early solar system ...
... • They were further from the Sun and gravity was weaker • They formed beyond the frost line where ices can condense so they included hydrogen compounds • They were far enough from the Sun to escape the heavy bombardment that battered the early solar system ...
1_31_planetary calculator
... The students will come forward with scales they want to use to make a model of the Solar System. Example of scales they might think of: • The earth is 5 cm diameter and everything is scaled accordingly. • The size of the Earth as unit to make a Solar System hands-on model. • The distance of the Eart ...
... The students will come forward with scales they want to use to make a model of the Solar System. Example of scales they might think of: • The earth is 5 cm diameter and everything is scaled accordingly. • The size of the Earth as unit to make a Solar System hands-on model. • The distance of the Eart ...
Ingrid Mann Dust- plasma processes in the vicinity of planetary
... and nanometer-sized dust are formed. The surrounding environment controls the dynamics of the impact-generated populations, for example through electric- and magnetic fields and radiation pressure. At the same time, the impact-generated ions, neutrals and dust particles affect the local space enviro ...
... and nanometer-sized dust are formed. The surrounding environment controls the dynamics of the impact-generated populations, for example through electric- and magnetic fields and radiation pressure. At the same time, the impact-generated ions, neutrals and dust particles affect the local space enviro ...
Solar System - Spring Branch ISD
... called gas giants. These planets are _______, Neptune These planets ________, Saturn _________, Uranus and ________. are gaseous in nature, composed of mostly hydrogen and helium ____________________. ...
... called gas giants. These planets are _______, Neptune These planets ________, Saturn _________, Uranus and ________. are gaseous in nature, composed of mostly hydrogen and helium ____________________. ...
The Many Faces of the Sun
... -non-thermal energetic particles emitting in: radio, hard Xray, γ-rays ...
... -non-thermal energetic particles emitting in: radio, hard Xray, γ-rays ...
Stellar Evolution and our Sun (Song “The Sun” from “Severe Tire
... axis of rotation but doesn’t affect motion parallel to the rotation axis – so you get a disk rather than a sphere! Material in the disk migrates into a primitive solar nebula Initially, all the angular momentum is in the center inner materials transfer angular momentum outward in the disk ultimately ...
... axis of rotation but doesn’t affect motion parallel to the rotation axis – so you get a disk rather than a sphere! Material in the disk migrates into a primitive solar nebula Initially, all the angular momentum is in the center inner materials transfer angular momentum outward in the disk ultimately ...
friends of the planetarium newsletter
... fact, the star R136a1, which is located in the R136 cluster, is the most massive star ever found. Its current mass is approximately 265 solar masses, and its estimated birth weight was as much as 320 times that of our sun. R136a1 also has the highest luminosity of any star found to date, nearly 10 m ...
... fact, the star R136a1, which is located in the R136 cluster, is the most massive star ever found. Its current mass is approximately 265 solar masses, and its estimated birth weight was as much as 320 times that of our sun. R136a1 also has the highest luminosity of any star found to date, nearly 10 m ...
Advanced Composition Explorer
Advanced Composition Explorer (ACE) is a NASA Explorers program Solar and space exploration mission to study matter comprising energetic particles from the solar wind, the interplanetary medium, and other sources. Real-time data from ACE is used by the NOAA Space Weather Prediction Center to improve forecasts and warnings of solar storms. The ACE robotic spacecraft was launched August 25, 1997 and entered a Lissajous orbit close to the L1 Lagrangian point (which lies between the Sun and the Earth at a distance of some 1.5 million km from the latter) on December 12, 1997. The spacecraft is currently operating at that orbit. Because ACE is in a non-Keplerian orbit, and has regular station-keeping maneuvers, the orbital parameters at right are only approximate. The spacecraft is still in generally good condition in 2015, and is projected to have enough fuel to maintain its orbit until 2024. NASA Goddard Space Flight Center managed the development and integration of the ACE spacecraft.