PASS Content Standard 5.1
... This picture was taken with the Hubble Space Telescope. There is only one star in the picture, all the others are galaxies. ...
... This picture was taken with the Hubble Space Telescope. There is only one star in the picture, all the others are galaxies. ...
Light Years Away
... If we use the calculations from the previous slide, Voyager traveled ½ light day in approximately 15 years. If we travel at the speed of the Voyager then it would take approximately 30 years to travel one light day One light year would take over 11,000 years!!!!! ...
... If we use the calculations from the previous slide, Voyager traveled ½ light day in approximately 15 years. If we travel at the speed of the Voyager then it would take approximately 30 years to travel one light day One light year would take over 11,000 years!!!!! ...
Topic/Objective: ______ _____ Full Name: __________ Class: __
... and groups of galaxies seems to be increasing with time. Edwin Hubble’s discovery of the redshift in the spectra of galaxies supports the expansion of the universe Discovery of radiation called cosmic background radiation apparently left over from the universe’s beginning. Continues to be test ...
... and groups of galaxies seems to be increasing with time. Edwin Hubble’s discovery of the redshift in the spectra of galaxies supports the expansion of the universe Discovery of radiation called cosmic background radiation apparently left over from the universe’s beginning. Continues to be test ...
proposed research projects for pparc gemini studentships
... formation of S0 galaxies, and their dependency on galaxy mass. To this end, we propose a spectral study of a large sample of lenticular systems to establish the links between the properties of their stellar populations (ages and chemical abundances) and their kinematic properties (masses and dynamic ...
... formation of S0 galaxies, and their dependency on galaxy mass. To this end, we propose a spectral study of a large sample of lenticular systems to establish the links between the properties of their stellar populations (ages and chemical abundances) and their kinematic properties (masses and dynamic ...
Scientific Notation Introduction Activity
... [note: conversion from m to km is three decimal places to the left 1000m = 1.0 km [standard] so 103m = 100km [exponent] and 1.0 x 103m = 1.0 x 100 km [scientific notation] always remember that 100 is equal to 1] ...
... [note: conversion from m to km is three decimal places to the left 1000m = 1.0 km [standard] so 103m = 100km [exponent] and 1.0 x 103m = 1.0 x 100 km [scientific notation] always remember that 100 is equal to 1] ...
The Milky Way Galaxy - Academic Computer Center
... made for the size of the galaxy and the position of the Sun within it. • It was found that certain dense clusters of stars known as globular clusters tended to be distributed in an elliptical region of space. The center would indicate the center of the galaxy. • The Sun was found not to be at the ce ...
... made for the size of the galaxy and the position of the Sun within it. • It was found that certain dense clusters of stars known as globular clusters tended to be distributed in an elliptical region of space. The center would indicate the center of the galaxy. • The Sun was found not to be at the ce ...
27DarkMatter
... and the distance between their centers. All planets have sideways velocity so that they travel in circular orbits. Which planet do you expect to move faster, A or E? A. Planet A will move faster because the gravitational pull from the star is bigger on planet A B. Planet E will move faster because t ...
... and the distance between their centers. All planets have sideways velocity so that they travel in circular orbits. Which planet do you expect to move faster, A or E? A. Planet A will move faster because the gravitational pull from the star is bigger on planet A B. Planet E will move faster because t ...
Objectives for grade E - Particle and Astroparticle Physics
... • In 1850 Fizeau and Foucalt also experimented with light by bouncing it off a rotating mirror and measuring time • The light returned to its source at a slightly different position because the mirror has moved during the time light was traveling • d=rt again gave c ...
... • In 1850 Fizeau and Foucalt also experimented with light by bouncing it off a rotating mirror and measuring time • The light returned to its source at a slightly different position because the mirror has moved during the time light was traveling • d=rt again gave c ...
highen_13_gravwaves - Mullard Space Science Laboratory
... • For the Earth around the Sun, about 200W are emitted – so our orbit should last another 1023 years before it decays by gravitational radiation • When dimensions of orbit approach the Schwarzschild radius, gravitational radiation is pretty serious. ...
... • For the Earth around the Sun, about 200W are emitted – so our orbit should last another 1023 years before it decays by gravitational radiation • When dimensions of orbit approach the Schwarzschild radius, gravitational radiation is pretty serious. ...
The Size of the Universe (1920) Harlow Shapley Heber Curtis
... The Great Debate: The Size of the Universe ...
... The Great Debate: The Size of the Universe ...
11-29
... off the optical axis as a point light source. A ray passing through the focal point runs parallel to the optical axis after a lens. A ray coming through a lens in parallel to the optical axis passes through the focal point. A ray running on the optical axis remains on the optical axis. A ray that pa ...
... off the optical axis as a point light source. A ray passing through the focal point runs parallel to the optical axis after a lens. A ray coming through a lens in parallel to the optical axis passes through the focal point. A ray running on the optical axis remains on the optical axis. A ray that pa ...
Characteristics of Stars PLATO
... –Huge stars with lots of fuel can become a Supergiant – It is like taking the wood from a burning campfire and spreading it out across the beach. It gets cooler and dim, but takes up more space. ...
... –Huge stars with lots of fuel can become a Supergiant – It is like taking the wood from a burning campfire and spreading it out across the beach. It gets cooler and dim, but takes up more space. ...
Introduction to Astrophysics, Lecture 10
... One goal of star formation studies is to predict the Initial Mass Function of stars, usually known as the IMF. This tells us the number of stars forming with a given mass. There is some dispute over the observational form of the IMF, with popular examples being the Salpeter mass function and the Sca ...
... One goal of star formation studies is to predict the Initial Mass Function of stars, usually known as the IMF. This tells us the number of stars forming with a given mass. There is some dispute over the observational form of the IMF, with popular examples being the Salpeter mass function and the Sca ...
ppt - University of Arizona
... years earlier (around z~10) the redshift => z~14 Epoch of first star formation - roles of NICMOS and now seem likely to have been IRAC correspond to NIRCam around z~10-15 from and MIRI on JWST. combining Spitzer and Important to note that a number of WMAP results. similar galaxies have now been fo ...
... years earlier (around z~10) the redshift => z~14 Epoch of first star formation - roles of NICMOS and now seem likely to have been IRAC correspond to NIRCam around z~10-15 from and MIRI on JWST. combining Spitzer and Important to note that a number of WMAP results. similar galaxies have now been fo ...