Exoplanets Properties of the host stars Characterization of the
... – Will greatly increase the accuracy of exoplanet host stars distances – Stars with distances larger than 50-100 pc will most greatly benefit with respect to the current measurements based on Hipparcos – Mission launched in 2013, nominal end foreseen in 2018 – First data releases start to be ava ...
... – Will greatly increase the accuracy of exoplanet host stars distances – Stars with distances larger than 50-100 pc will most greatly benefit with respect to the current measurements based on Hipparcos – Mission launched in 2013, nominal end foreseen in 2018 – First data releases start to be ava ...
Stars - Stallion Science
... • According to the Big Bang Theory: • Immediately after, the universe was extremely hot and made up of pure energy • There was a period of rapid expansion that caused the energy to cool, and allowed electrons, neutrons and protons to form • Hydrogen nuclei started to form but it was still too hot fo ...
... • According to the Big Bang Theory: • Immediately after, the universe was extremely hot and made up of pure energy • There was a period of rapid expansion that caused the energy to cool, and allowed electrons, neutrons and protons to form • Hydrogen nuclei started to form but it was still too hot fo ...
View the presentation slides
... Fortunately, optical techniques are capable of exquisite accuracy. Let’s look at some data. This is a “Jupiter” (M ~ 0.96 MJ) orbiting a “Sol” (M = 0.88 MS). The orbital period is 9 years (Jupiter’s is 12), because the orbit is a bit smaller (4.2 AU instead of 5.2). This is how astronomers 60 light- ...
... Fortunately, optical techniques are capable of exquisite accuracy. Let’s look at some data. This is a “Jupiter” (M ~ 0.96 MJ) orbiting a “Sol” (M = 0.88 MS). The orbital period is 9 years (Jupiter’s is 12), because the orbit is a bit smaller (4.2 AU instead of 5.2). This is how astronomers 60 light- ...
How to Directly Image a Habitable Planet Around Alpha Centauri
... contrast space telescope of 4m or higher aperture [4,5], capable of surveying hundreds of stars for potentially habitable planets and taking spectra with high enough resolution to determine detailed atmospheric compositions and truly search for signs of life. These missions will surely make great le ...
... contrast space telescope of 4m or higher aperture [4,5], capable of surveying hundreds of stars for potentially habitable planets and taking spectra with high enough resolution to determine detailed atmospheric compositions and truly search for signs of life. These missions will surely make great le ...
Stars, Galaxies & Universe
... A. Satellite telescopes are much closer to the stars. B. Satellite telescopes are able to see through solid objects. C. Satellite telescopes can detect wavelengths that are blocked by the atmosphere. D. Satellite telescopes have the ability to see the future. ...
... A. Satellite telescopes are much closer to the stars. B. Satellite telescopes are able to see through solid objects. C. Satellite telescopes can detect wavelengths that are blocked by the atmosphere. D. Satellite telescopes have the ability to see the future. ...
2.1 Introduction
... If we measure the celestial coordinates (RA and Dec) of a nearby star at the same time each year (or in practice if we correct for the effects of the Earth’s orbit around the Sun), we find that its position in a reference frame based on very distant objects such as quasars is not the same from year ...
... If we measure the celestial coordinates (RA and Dec) of a nearby star at the same time each year (or in practice if we correct for the effects of the Earth’s orbit around the Sun), we find that its position in a reference frame based on very distant objects such as quasars is not the same from year ...
Quantum Well Electron Gain Structures and Infrared
... • If planet is close in, orbit will be unstable and chaotic • Moving in/out of HZ is probably hard on life development • If planet is far away (orbiting BOTH stars), orbit is stable, but typically outside the HZ (!) ...
... • If planet is close in, orbit will be unstable and chaotic • Moving in/out of HZ is probably hard on life development • If planet is far away (orbiting BOTH stars), orbit is stable, but typically outside the HZ (!) ...
Extrasolar Planets = 403
... Planets orbiting stars other than the Sun Smaller than 13 Jupiter masses First planet around ordinary star is 51 Peg 1995 Most found using Iodine cell technique pioneered at DAO, UBC, UVic ...
... Planets orbiting stars other than the Sun Smaller than 13 Jupiter masses First planet around ordinary star is 51 Peg 1995 Most found using Iodine cell technique pioneered at DAO, UBC, UVic ...
Gilmore
... galaxies, ‘classical’ L ~ 106L, V >> 24 mag/sq Apparently dark-matter dominated ~ 10km/s, 10 < M/L < 100 Metal-poor, all contain very old stars; but ...
... galaxies, ‘classical’ L ~ 106L, V >> 24 mag/sq Apparently dark-matter dominated ~ 10km/s, 10 < M/L < 100 Metal-poor, all contain very old stars; but ...
The Edge of the Solar System The Oort Cloud
... 12 comets per year leave Oort Cloud to become long-range comets o Pushed out by large molecular clouds, passing stars, or tidal interactions with Milky Way's disc o 5 of these enter inner solar system per year o It takes thousands of years for them to orbit the sun ...
... 12 comets per year leave Oort Cloud to become long-range comets o Pushed out by large molecular clouds, passing stars, or tidal interactions with Milky Way's disc o 5 of these enter inner solar system per year o It takes thousands of years for them to orbit the sun ...
Wide-eyed Telescope Finds its First Transiting
... attached to a conventional telescope mount. SuperWASP has a field-of-view some 2000 times greater than a conventional astronomical telescope. The instruments run under robotic control and are housed in their own customised building. The eight individual cameras on each mount are small by telescope s ...
... attached to a conventional telescope mount. SuperWASP has a field-of-view some 2000 times greater than a conventional astronomical telescope. The instruments run under robotic control and are housed in their own customised building. The eight individual cameras on each mount are small by telescope s ...
Wide-eyed Telescope Finds its First Transiting
... attached to a conventional telescope mount. SuperWASP has a field-of-view some 2000 times greater than a conventional astronomical telescope. The instruments run under robotic control and are housed in their own customised building. The eight individual cameras on each mount are small by telescope s ...
... attached to a conventional telescope mount. SuperWASP has a field-of-view some 2000 times greater than a conventional astronomical telescope. The instruments run under robotic control and are housed in their own customised building. The eight individual cameras on each mount are small by telescope s ...
Dark Matter -24-------------------------------~-----------R-E-S-O-N-A-N-C
... There have been three reactions to the discovery of dark matter: (i) It doesn't exist; the law of gravitation must be modified so that the stars are all there is to a galaxy. (ii) Dark matter exists, but consists entirely of ord~nary matter - Jupiter-like objects called broum dwarfs that are not mas ...
... There have been three reactions to the discovery of dark matter: (i) It doesn't exist; the law of gravitation must be modified so that the stars are all there is to a galaxy. (ii) Dark matter exists, but consists entirely of ord~nary matter - Jupiter-like objects called broum dwarfs that are not mas ...
PowerPoint - StarDate`s Black Hole Encyclopedia
... Even then, they couldn't quite fathom what they saw. Photographic plates showed only an inconspicuous blue star. But when astronomers split the star's light into its individual wavelengths, they found that it was unlike any known star, galaxy, or nebula. Further study eventually revealed that it's b ...
... Even then, they couldn't quite fathom what they saw. Photographic plates showed only an inconspicuous blue star. But when astronomers split the star's light into its individual wavelengths, they found that it was unlike any known star, galaxy, or nebula. Further study eventually revealed that it's b ...
Birth of Stars
... The dust-shrouded interiors of molecular clouds where stellar births are thought to take place cannot be observed with visible light, but only with infrared and radio telescopes The timescale for the initial collapse is estimated to be very short astronomically (thousands of years), implying that st ...
... The dust-shrouded interiors of molecular clouds where stellar births are thought to take place cannot be observed with visible light, but only with infrared and radio telescopes The timescale for the initial collapse is estimated to be very short astronomically (thousands of years), implying that st ...
Test #4
... 12. We cannot see the other side of the galaxy primarily because our view is blocked by a) too many stars, b) glowing interstellar gas, c) interstellar dust, d) planetary nebulae 13. The mass of the galaxy has been found by a) counting the stars it contains, b) determining its gravitational force on ...
... 12. We cannot see the other side of the galaxy primarily because our view is blocked by a) too many stars, b) glowing interstellar gas, c) interstellar dust, d) planetary nebulae 13. The mass of the galaxy has been found by a) counting the stars it contains, b) determining its gravitational force on ...
I. Determination of stellar Parameters
... a major step in the study of stellar streams. • … more to come with GAIA! ...
... a major step in the study of stellar streams. • … more to come with GAIA! ...
Conference Summary Richard Ellis (Caltech) ITALIA
... Zeldovich (1978): “One can be pretty sure that the problem of galaxy formation will be solved in the 1980’s” 1990’s: unwarranted confidence from theorists & observers: extended SF histories was an early prediction of CDM models matching optical data only ...
... Zeldovich (1978): “One can be pretty sure that the problem of galaxy formation will be solved in the 1980’s” 1990’s: unwarranted confidence from theorists & observers: extended SF histories was an early prediction of CDM models matching optical data only ...
A DEDICATED M DWARF PLANET SEARCH USING THE HOBBY
... astrometric database (ESA 1997). In order to minimize the effects of stellar activity on our RV measurements (especially rotational modulation by starspots), we chose only targets with no detected or low X-ray emission, using the ROSAT All-Sky Survey results from Hünsch et al. (1999). In our observi ...
... astrometric database (ESA 1997). In order to minimize the effects of stellar activity on our RV measurements (especially rotational modulation by starspots), we chose only targets with no detected or low X-ray emission, using the ROSAT All-Sky Survey results from Hünsch et al. (1999). In our observi ...
Foundation 1 - Discovering Astronomy
... • Cepheid variables (periods between 1 & 100 days) • Mira variables (periods greater than 100 days) ...
... • Cepheid variables (periods between 1 & 100 days) • Mira variables (periods greater than 100 days) ...
charts_set_9
... • Most of Galaxy within ~ 20 kpc (1011 - 1012 stars) • 800 kpc to M31 • Local group (about 20), radius ~ 1 Mpc • Local supercluster (about 2500), distance ~ 15 Mpc to Virgo cluster • Several other galaxy clusters to ~75 Mpc • Increasing numbers of AGNs out to radius ~ 100 Mpc • QSOs to extent of obs ...
... • Most of Galaxy within ~ 20 kpc (1011 - 1012 stars) • 800 kpc to M31 • Local group (about 20), radius ~ 1 Mpc • Local supercluster (about 2500), distance ~ 15 Mpc to Virgo cluster • Several other galaxy clusters to ~75 Mpc • Increasing numbers of AGNs out to radius ~ 100 Mpc • QSOs to extent of obs ...
Kepler Mission: The Search for Earth-sized Planets
... How big an area is that? Imagine, if you shrunk our solar system to a little larger than a quarter: Our whole Solar System ...
... How big an area is that? Imagine, if you shrunk our solar system to a little larger than a quarter: Our whole Solar System ...
The Universe - Smithsonian Education
... The lessons in this issue address the questions, therefore, by first asking the students. In Lesson 1, the class works together to arrange pictures from space according to the students’ best ideas of size, distance, and age. This active introduction to the cosmos can be a pre-assessment for a unit o ...
... The lessons in this issue address the questions, therefore, by first asking the students. In Lesson 1, the class works together to arrange pictures from space according to the students’ best ideas of size, distance, and age. This active introduction to the cosmos can be a pre-assessment for a unit o ...
Astronomy 1020 Exam 4 Review Questions
... 16. How is a black hole defined? What is a singularity, an Einstein-Rosen bridge, and a wormhole? How are they related to each other? How are the Schwarzschild radius and the event horizon related? What is hyperspace? 17. What happens to tidal forces and time as you approach a black hole? 18. Calcul ...
... 16. How is a black hole defined? What is a singularity, an Einstein-Rosen bridge, and a wormhole? How are they related to each other? How are the Schwarzschild radius and the event horizon related? What is hyperspace? 17. What happens to tidal forces and time as you approach a black hole? 18. Calcul ...
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.