PHYS 390 Lecture 31 - Kinematics of galaxies 31
... Galaxies assume a variety of shapes, but certainly one of the more common shapes is a spiral or pinwheel: ...
... Galaxies assume a variety of shapes, but certainly one of the more common shapes is a spiral or pinwheel: ...
lec06_07oct2011
... Advantages of the microlensing technique to detect exoplanets include: * More sensitive than most other techniques to small-mass planets (like Earth) * Most sensitive to planets in our Galaxy that have orbit sizes of a few astronomical units (like those of Mars or Jupiter) * Only method capable of d ...
... Advantages of the microlensing technique to detect exoplanets include: * More sensitive than most other techniques to small-mass planets (like Earth) * Most sensitive to planets in our Galaxy that have orbit sizes of a few astronomical units (like those of Mars or Jupiter) * Only method capable of d ...
The Universe and Galaxies - West Jefferson Local Schools
... I. What is the universe? - universe - sum of all _________ and energy that ever has, does, and ever will exist everything physical that exists in _________ and _________ - _________ – the study of how the universe began, what it is made of and how it continues to evolve and change - Of what is the ...
... I. What is the universe? - universe - sum of all _________ and energy that ever has, does, and ever will exist everything physical that exists in _________ and _________ - _________ – the study of how the universe began, what it is made of and how it continues to evolve and change - Of what is the ...
Name: :______Date:
... 11. What can star spectra tell about a star? __________________________________________________________________________ 12. Scientists can look at light of galaxies that tell them how fast they are moving __________________________________________________________________________ 13. Almost all galax ...
... 11. What can star spectra tell about a star? __________________________________________________________________________ 12. Scientists can look at light of galaxies that tell them how fast they are moving __________________________________________________________________________ 13. Almost all galax ...
astronomy - sfox4science
... The universe is estimated to be over 10 billion years old. The universe is composed of galaxies, stars, planets, asteroids, comets, and meteors, each having different properties. Our solar system exists within the Milky Way galaxy. The known components of our solar system are the Sun, four terrestri ...
... The universe is estimated to be over 10 billion years old. The universe is composed of galaxies, stars, planets, asteroids, comets, and meteors, each having different properties. Our solar system exists within the Milky Way galaxy. The known components of our solar system are the Sun, four terrestri ...
AstronomyQuotes
... Images of broken light which dance before me like a million eyes that call me on and on across the Universe. Limitless undying love which shines around me like a million suns, it calls me on and on across the Universe. ...
... Images of broken light which dance before me like a million eyes that call me on and on across the Universe. Limitless undying love which shines around me like a million suns, it calls me on and on across the Universe. ...
The Universe and Galaxies - West Jefferson Local Schools
... - there are an estimated ________ billion galaxies in the universe A. 3 Types of Galaxies - classified by ________ 1. ________ - disk shaped with spiral arms of dust and gas (fig 26-15, pg. 831) - dust and gas provide a place for new stars to ________ - young stars are ________ in color gives spir ...
... - there are an estimated ________ billion galaxies in the universe A. 3 Types of Galaxies - classified by ________ 1. ________ - disk shaped with spiral arms of dust and gas (fig 26-15, pg. 831) - dust and gas provide a place for new stars to ________ - young stars are ________ in color gives spir ...
Astronomy practice questions for 3-6 test
... 4. Is the Andromeda galaxy red or blue shifted? __________________________________________________________ 5. According to Hubble’s law, which galaxy or planet is moving fastest away from the nearby star? __________________________________________________________ 6. Which galaxy or planet is moving ...
... 4. Is the Andromeda galaxy red or blue shifted? __________________________________________________________ 5. According to Hubble’s law, which galaxy or planet is moving fastest away from the nearby star? __________________________________________________________ 6. Which galaxy or planet is moving ...
PH142 - Mohawk Valley Community College
... -2III. Student Objectives The purpose of this course is to give a student a full introductory coverage of astronomy, to provide a means of scientific explanation for new astronomical discoveries and theories, and to put into practice techniques learned in Descriptive Astronomy 1. At the conclusion ...
... -2III. Student Objectives The purpose of this course is to give a student a full introductory coverage of astronomy, to provide a means of scientific explanation for new astronomical discoveries and theories, and to put into practice techniques learned in Descriptive Astronomy 1. At the conclusion ...
Types of Planets and Stars
... Middle-Aged Stars Main Sequence Stars -- make up the majority of stars in the universe. Earth’s sun is a main sequence star. These stars vary in size, mass, and brightness, but they all convert hydrogen into helium, also known as nuclear fusion. While our sun will spend 10 billion on its main seq ...
... Middle-Aged Stars Main Sequence Stars -- make up the majority of stars in the universe. Earth’s sun is a main sequence star. These stars vary in size, mass, and brightness, but they all convert hydrogen into helium, also known as nuclear fusion. While our sun will spend 10 billion on its main seq ...
Hunting for Extrasolar Planets: Methods and Results
... A photometric method: Transits. This is the most active area of planet searching today because 1. It does not require a large telescope! 2. Chances of finding a planet-star system nearly edge-on is small, so need lots of observations; 3. Big payoff: you can learn about a stars diameter and mass, an ...
... A photometric method: Transits. This is the most active area of planet searching today because 1. It does not require a large telescope! 2. Chances of finding a planet-star system nearly edge-on is small, so need lots of observations; 3. Big payoff: you can learn about a stars diameter and mass, an ...
Unit 3: Understanding the Universe
... The universe is made up of stars, gas, and dust, as well as invisible dark matter. Material in the universe is not randomly arranged, but is pulled by gravity into galaxies. ...
... The universe is made up of stars, gas, and dust, as well as invisible dark matter. Material in the universe is not randomly arranged, but is pulled by gravity into galaxies. ...
Lecture 1
... • Explicit dependence on d (radial velocity measurements also less sensitive for distant stars due to lower S/N spectra) • Detection of planets at large orbital radii still requires a search time comparable to the orbital period • Has been used to detect the radial velocity planet GJ 876 b with a pe ...
... • Explicit dependence on d (radial velocity measurements also less sensitive for distant stars due to lower S/N spectra) • Detection of planets at large orbital radii still requires a search time comparable to the orbital period • Has been used to detect the radial velocity planet GJ 876 b with a pe ...
1201 Discussion Notes
... What does this imply? Well, remember that at large distances we are seeing into the past. Since active galactic nuclei are far away, they are young. The galaxies we see nearby are older. Therefore, activity is more common among young galaxies than older ones. Current theory holds that active galacti ...
... What does this imply? Well, remember that at large distances we are seeing into the past. Since active galactic nuclei are far away, they are young. The galaxies we see nearby are older. Therefore, activity is more common among young galaxies than older ones. Current theory holds that active galacti ...
Robotics - UNL CSE
... substance or not. Scientists also use technologies to detect visible and infared light reflecting off of a planet. Chemicals absorb certain wavelengths, and depending on how much of the spectrum is missing, they can tell which chemicals make up the atmosphere of the planet, and therefore if the plan ...
... substance or not. Scientists also use technologies to detect visible and infared light reflecting off of a planet. Chemicals absorb certain wavelengths, and depending on how much of the spectrum is missing, they can tell which chemicals make up the atmosphere of the planet, and therefore if the plan ...
Microsoft Word 97
... 1. When did the Milky Way begin? _____________________________________________________ 2. Where does its name come from? ___________________________________________________ 3. What do we see when we look in the sky? _____________________________________________ 4. What does our galaxy look like from ...
... 1. When did the Milky Way begin? _____________________________________________________ 2. Where does its name come from? ___________________________________________________ 3. What do we see when we look in the sky? _____________________________________________ 4. What does our galaxy look like from ...
Aug 2015 supplement - Hermanus Astronomy
... Big Bang, the universe was full of a fog of hydrogen gas. But as more and more brilliant sources - both stars and quasars powered by huge black holes started to shine, they cleared away the mist and made the universe transparent to ultraviolet light. Astronomers call this the epoch of reionisation, ...
... Big Bang, the universe was full of a fog of hydrogen gas. But as more and more brilliant sources - both stars and quasars powered by huge black holes started to shine, they cleared away the mist and made the universe transparent to ultraviolet light. Astronomers call this the epoch of reionisation, ...
ppt
... • Protons and electrons have mass, charge • Also have angular momentum (spin) which creates tiny magnetic field • So energy of H atom is different depending on orientation of spins (if same ↓, if opposite directions ↑, but energy difference = 10-6 x electron orbits) • photon emitted in a spin-flip t ...
... • Protons and electrons have mass, charge • Also have angular momentum (spin) which creates tiny magnetic field • So energy of H atom is different depending on orientation of spins (if same ↓, if opposite directions ↑, but energy difference = 10-6 x electron orbits) • photon emitted in a spin-flip t ...
Carter K 1 - Mrs. Anthony`s English 2
... giving those planets around it life as well. N is the number of planets per solar system that are suitable for life. Fl is the fraction of planets where life actually appears. Fi is the fraction of planets where intelligent life appears. Fc is the fraction of life that release detectable signs of li ...
... giving those planets around it life as well. N is the number of planets per solar system that are suitable for life. Fl is the fraction of planets where life actually appears. Fi is the fraction of planets where intelligent life appears. Fc is the fraction of life that release detectable signs of li ...
Star or planet, or what?
... Moon (which had clear bodily markings). Modern knowledge inflation now decrees that today’s potential occupants of the planetary cage should be dispersed into a row of separate cages, one each for terrestrial planets, gas giant planets, Pluto-like objects in 2, 3 resonances with Neptune, large satel ...
... Moon (which had clear bodily markings). Modern knowledge inflation now decrees that today’s potential occupants of the planetary cage should be dispersed into a row of separate cages, one each for terrestrial planets, gas giant planets, Pluto-like objects in 2, 3 resonances with Neptune, large satel ...
Study Guide: Use your notes and handouts to
... What is a light year? What is it used to measure in space? ...
... What is a light year? What is it used to measure in space? ...
The Solar System Song - Sing-A
... In orbits one by one. Now the planets they have satellites – but we just call them moons And comets made of rock and ice could be harbingers of doom Ast-er-oids are rocks and dust that are floating round the sun If gravity pulls them in to earth, a meteor they become. The Solar System, eight planets ...
... In orbits one by one. Now the planets they have satellites – but we just call them moons And comets made of rock and ice could be harbingers of doom Ast-er-oids are rocks and dust that are floating round the sun If gravity pulls them in to earth, a meteor they become. The Solar System, eight planets ...
Methods Of Discovering Extra solar Planets.
... • This method goes hand in hand with the astrometry. • Once they find out the stars movement, then they look for if the star is moving in real life. • The affects of the planet will be small yet it will be detectable. Of course large planets will be doing this affect. • The downside to this is that ...
... • This method goes hand in hand with the astrometry. • Once they find out the stars movement, then they look for if the star is moving in real life. • The affects of the planet will be small yet it will be detectable. Of course large planets will be doing this affect. • The downside to this is that ...
Space Interferometry Mission
The Space Interferometry Mission, or SIM, also known as SIM Lite (formerly known as SIM PlanetQuest), was a planned space telescope developed by the U.S. National Aeronautics and Space Administration (NASA), in conjunction with contractor Northrop Grumman. One of the main goals of the mission was the hunt for Earth-sized planets orbiting in the habitable zones of nearby stars other than the Sun. SIM was postponed several times and finally cancelled in 2010.In addition to hunting for extrasolar planets, SIM would have helped astronomers construct a map of the Milky Way galaxy. Other important tasks would have included collecting data to help pinpoint stellar masses for specific types of stars, assisting in the determination of the spatial distribution of dark matter in the Milky Way and in the Local Group of galaxies and using the gravitational microlensing effect to measure the mass of stars.The spacecraft would have used optical interferometry to accomplish these and other scientific goals. This technique collects light with multiple mirrors (in SIM's case, two) which is combined to make an interference pattern which can be very precisely measured.The initial contracts for SIM Lite were awarded in 1998, totaling US$200 million. Work on the SIM project required scientists and engineers to move through eight specific new technology milestones, and by November 2006, all eight had been completed.SIM Lite was originally scheduled for a 2005 launch, aboard an Evolved Expendable Launch Vehicle (EELV). As a result of continued budget cuts, the launch date has been pushed back at least five times. NASA has set a preliminary launch date for 2015 and U.S. federal budget documents confirm that a launch date is expected ""no earlier"" than 2015. The budget cuts to SIM Lite are expected to continue through FY 2010. As of February 2007, many of the engineers working on the SIM program had moved on to other areas and projects, and NASA directed the project to allocate its resources toward engineering risk reduction. However, the preliminary budget for NASA for 2008 included zero dollars for SIM.In December 2007, the Congress restored funding for fiscal year 2008 as part of an omnibus appropriations bill which the President later signed. At the same time the Congress directed NASA to move the mission forward to the development phase. In 2009 the project continued its risk reduction work while waiting for the findings and recommendations of the Astronomy and Astrophysics Decadal Survey, Astro2010, performed by the National Academy of Sciences, which would determine the project's future.On 13 August 2010, the Astro2010 Decadal Report was released and did not recommend that NASA continue the development of the SIM Lite Astrometric Observatory. This prompted NASA Astronomy and Physics Director, Jon Morse, to issue a letter on 24 September 2010 to the SIM Lite project manager, informing him that NASA was discontinuing its sponsorship of the SIM Lite mission and directing the project to discontinue Phase B activities immediately or as soon as practical. Accordingly, all SIM Lite activities were closed down by the end of calendar year 2010.