Habitability and Stability of Orbits for Earth
... planet on the orbital stability of terrestrial planets. They argued that orbital stability of terrestrial planets is warranted as most test Earth-mass planets are found to survive within the HZ over 106 -year timescales. On the other hand, this study is only of limited use, as the authors did not co ...
... planet on the orbital stability of terrestrial planets. They argued that orbital stability of terrestrial planets is warranted as most test Earth-mass planets are found to survive within the HZ over 106 -year timescales. On the other hand, this study is only of limited use, as the authors did not co ...
Twitter Feed ITSO Symposium 2017
... nevertheless, the Keck MOSFIRE instrument has been used to detect Lyman-alpha emission from a handful of intrinsically bright galaxies all the way to z = 8.7. These bright sources, however, are not expected to be representative of the galaxy population that existed at the time. I will present our pr ...
... nevertheless, the Keck MOSFIRE instrument has been used to detect Lyman-alpha emission from a handful of intrinsically bright galaxies all the way to z = 8.7. These bright sources, however, are not expected to be representative of the galaxy population that existed at the time. I will present our pr ...
Kepler Mission Workshop Presentation
... lava and much too hot for life as we know it • All five of the exoplanets orbit stars hotter and larger than Earth's sun. ...
... lava and much too hot for life as we know it • All five of the exoplanets orbit stars hotter and larger than Earth's sun. ...
ph709-14
... In the Solar System (ONLY) orbital radii less than giant planets Core: A central metallic core, mostly iron with a surrounding silicate mantle. The Moon is similar, but lacks an iron core. Terrestrial planets have canyons, craters, mountains, and ...
... In the Solar System (ONLY) orbital radii less than giant planets Core: A central metallic core, mostly iron with a surrounding silicate mantle. The Moon is similar, but lacks an iron core. Terrestrial planets have canyons, craters, mountains, and ...
Stellar radii from long-baseline interferometry
... They are a visual binary pair with a very long orbital period (≈ 700 yrs). In 1838, 61 Cyg became the first star whose distance from Earth was estimated accurately (Bessel 1838), shortly before Procyon’s, and it is now known with an exquisite accuracy. Its proper motion of more than 5 per year, firs ...
... They are a visual binary pair with a very long orbital period (≈ 700 yrs). In 1838, 61 Cyg became the first star whose distance from Earth was estimated accurately (Bessel 1838), shortly before Procyon’s, and it is now known with an exquisite accuracy. Its proper motion of more than 5 per year, firs ...
DTU_9e_ch15
... The Sun is located about 26,000 ly from the galactic nucleus, between the spiral arms. The Sun moves in its orbit at a speed of about 878,000 km/h and takes about 230 million years to complete one orbit around the center of the Galaxy. ...
... The Sun is located about 26,000 ly from the galactic nucleus, between the spiral arms. The Sun moves in its orbit at a speed of about 878,000 km/h and takes about 230 million years to complete one orbit around the center of the Galaxy. ...
ppt
... OGLE-TR-3 is NOT a transiting planet. You know this immediately because the RV is not in phase with the transit ...
... OGLE-TR-3 is NOT a transiting planet. You know this immediately because the RV is not in phase with the transit ...
Star formation in galaxies over the last 10 billion
... A long time ago in galaxies far, far away: The HST Ultra Deep Field ...
... A long time ago in galaxies far, far away: The HST Ultra Deep Field ...
A Faint Star Orbiting the Big Dipper’s Alcor Discovered
... technique is powerful and much faster than the usual way of confirming that objects in the sky are physically related.” The more typical method involves observing the pair of objects over much longer periods of time, even years, to show that the two are moving through space together. Alcor and its n ...
... technique is powerful and much faster than the usual way of confirming that objects in the sky are physically related.” The more typical method involves observing the pair of objects over much longer periods of time, even years, to show that the two are moving through space together. Alcor and its n ...
Galaxies (and stars) in the far infrared: results from the AKARI All
... The death of heavy stars : supernovae explosions Stars several times heavier than the Sun repeat expansion and contraction, and change their internal structure a few times depending on the mass. Then, finally they end their life with a very energetic explosion (supernova: SN). The ejected gas from ...
... The death of heavy stars : supernovae explosions Stars several times heavier than the Sun repeat expansion and contraction, and change their internal structure a few times depending on the mass. Then, finally they end their life with a very energetic explosion (supernova: SN). The ejected gas from ...
How big are stars? How do we know?
... orbiting each other, the system is a visual binary – If the stars are so close together (or distant from Earth) that their spectra blur together, the system is called a spectroscopic binary – If the stars are oriented edge-on to the Sun, one star will periodically eclipse the other star in the syste ...
... orbiting each other, the system is a visual binary – If the stars are so close together (or distant from Earth) that their spectra blur together, the system is called a spectroscopic binary – If the stars are oriented edge-on to the Sun, one star will periodically eclipse the other star in the syste ...
Lecture 22 - Cosmic distance scale
... As the Earth moves from one side of the Sun to the other, a nearby star will seem to change its position relative to the distant background stars. ...
... As the Earth moves from one side of the Sun to the other, a nearby star will seem to change its position relative to the distant background stars. ...
Chapter 15
... • Early in the history of the universe, hydrogen and helium (and other forms of matter) clumped together by gravitational attraction to form countless trillions of stars. Billions of galaxies, each a cluster of billions of stars, now form most of the visible mass in the universe. ...
... • Early in the history of the universe, hydrogen and helium (and other forms of matter) clumped together by gravitational attraction to form countless trillions of stars. Billions of galaxies, each a cluster of billions of stars, now form most of the visible mass in the universe. ...
L6-Diskproperties
... Spiral Galaxies: Disk Kinematics As in all spiral galaxies, everything in our Galaxy orbits around the Galactic Center (GC) The disk rotates with differential rotation material closer to the center travels on faster orbits (takes less time to make one full orbit) Similar to the motion of the ...
... Spiral Galaxies: Disk Kinematics As in all spiral galaxies, everything in our Galaxy orbits around the Galactic Center (GC) The disk rotates with differential rotation material closer to the center travels on faster orbits (takes less time to make one full orbit) Similar to the motion of the ...
Chapter 4 Practice Questions
... Question 3 a) mass times surface gravity b) mass divided by volume c) size divided by weight d) mass times surface area e) weight divided by size ...
... Question 3 a) mass times surface gravity b) mass divided by volume c) size divided by weight d) mass times surface area e) weight divided by size ...
Lecture 12
... Only in the past 20 years have astronomers really started agreeing about the distances to other galaxies (when I did a similar course in about 1990 estimates varied by factors of two). ...
... Only in the past 20 years have astronomers really started agreeing about the distances to other galaxies (when I did a similar course in about 1990 estimates varied by factors of two). ...
Chapter 15, Galaxies
... Where are the galaxies located? Are they located within the Milky Way, or are they much further away from us than the stars? • Before the 1920s, there were no reliable methods of measuring the distance to the galaxies. Many people believed that the galaxies were located within the Milky Way… How do ...
... Where are the galaxies located? Are they located within the Milky Way, or are they much further away from us than the stars? • Before the 1920s, there were no reliable methods of measuring the distance to the galaxies. Many people believed that the galaxies were located within the Milky Way… How do ...
New Worlds on the Horizon: Earth-Sized Planets Close to Other Stars.
... Earth-mass planets could exist on even closer orbits around other stars. The theory of in situ formation begins with a disk of gas and kmsized bodies (planetesimals); the latter accrete into ~100 Moon- to Mars-sized protoplanets in about 1 million years; these in turn collide and coalesce to form pl ...
... Earth-mass planets could exist on even closer orbits around other stars. The theory of in situ formation begins with a disk of gas and kmsized bodies (planetesimals); the latter accrete into ~100 Moon- to Mars-sized protoplanets in about 1 million years; these in turn collide and coalesce to form pl ...
Summary Of the Structure of the Milky Way
... has yielded the orbital speed of the Sun as it orbits the galactic center and the age of the Milky Way. • Finally, when knowledge of the orbital speed of Sun is combined with its distance from the galactic center an estimate of the mass of the galaxy can be obtained. ...
... has yielded the orbital speed of the Sun as it orbits the galactic center and the age of the Milky Way. • Finally, when knowledge of the orbital speed of Sun is combined with its distance from the galactic center an estimate of the mass of the galaxy can be obtained. ...
Galaxies - Stockton University
... – Black-holes are also efficient although less so than neutron stars • This is because black-holes have no surface so much of the energy is never released but is swallowed up by the black-hole directly and also orbits are unstable within three times the Schwarschild radius and little energy is retur ...
... – Black-holes are also efficient although less so than neutron stars • This is because black-holes have no surface so much of the energy is never released but is swallowed up by the black-hole directly and also orbits are unstable within three times the Schwarschild radius and little energy is retur ...
charts_set_7
... These bands are formed at the telescope by using colored filters that pass only light of certain wavelengths. Mgnitudes in B and V are used to form a star’s color index, a rough estimate of its temperature (blueness). ...
... These bands are formed at the telescope by using colored filters that pass only light of certain wavelengths. Mgnitudes in B and V are used to form a star’s color index, a rough estimate of its temperature (blueness). ...
Measuring the Properties of Stars (ch. 17)
... largest telescopes (with a very few exceptions, using interferometry for the largest nearby stars: see Fig. 17.11 for the best example), we can’t get their diameters directly. Instead we use a method that is based on Stefan’s law (see ch.3 if you have forgotten): The rate of emission of energy of al ...
... largest telescopes (with a very few exceptions, using interferometry for the largest nearby stars: see Fig. 17.11 for the best example), we can’t get their diameters directly. Instead we use a method that is based on Stefan’s law (see ch.3 if you have forgotten): The rate of emission of energy of al ...
New results on a Cn2 profiler for GeMS
... generation of extremely large telescopes (ELT). It is also of prime importance for the tomographic process for Adaptive Optics wide field imaging. Usually, the Cn2 profile is measured by dedicated instruments located outside of the telescope dome, or even at a different altitude than the telescope i ...
... generation of extremely large telescopes (ELT). It is also of prime importance for the tomographic process for Adaptive Optics wide field imaging. Usually, the Cn2 profile is measured by dedicated instruments located outside of the telescope dome, or even at a different altitude than the telescope i ...
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.