WASP-24b: A New Transiting Close-in Hot Jupiter
... Large scale, ground-based surveys for transiting planets are yielding a surprisingly diverse set of close-in giant planets. The last few years have seen the discovery of a number of so-called ‘bloated’ close-in Jovian planets, for example WASP-17 b (Anderson et al. 2010) and Kepler-7 b (Latham et al ...
... Large scale, ground-based surveys for transiting planets are yielding a surprisingly diverse set of close-in giant planets. The last few years have seen the discovery of a number of so-called ‘bloated’ close-in Jovian planets, for example WASP-17 b (Anderson et al. 2010) and Kepler-7 b (Latham et al ...
Galaxies
... the furthest observed galaxies has taken 11 billion years to reach us. These galaxies appear as they were when the universe was very young. ...
... the furthest observed galaxies has taken 11 billion years to reach us. These galaxies appear as they were when the universe was very young. ...
Astro 10B Study Questions for Each Chapter
... Which is larger: the Local Group or the Local Cluster? How are galaxies, groups and clusters distributed through space? Which type of clusters contain the most giant elliptical galaxies? Where would you find a galaxy which is the result of several mergers? What happens when galaxies collide? How wou ...
... Which is larger: the Local Group or the Local Cluster? How are galaxies, groups and clusters distributed through space? Which type of clusters contain the most giant elliptical galaxies? Where would you find a galaxy which is the result of several mergers? What happens when galaxies collide? How wou ...
The Milky Way: Home to Star Clusters
... parts of the Galaxy actually formed first. The standard theory supports that the halo was the original extent of the galaxy, and that this was created first, from the primordial gas that eventually collapsed in on itself, also demonstrated by the old stars contained within the globular clusters. Thi ...
... parts of the Galaxy actually formed first. The standard theory supports that the halo was the original extent of the galaxy, and that this was created first, from the primordial gas that eventually collapsed in on itself, also demonstrated by the old stars contained within the globular clusters. Thi ...
MSci Astrophysics 210PHY412 - Queen's University Belfast
... different masses but with the same age . Lets make a plot of Log(L/L) vs. LogTeff for an age of 1Gyr. The result is an isochrone. Important - think about what we are looking at when we observe a cluster. We are seeing a “freeze-frame” picture at a particular age. We see how stars of different masse ...
... different masses but with the same age . Lets make a plot of Log(L/L) vs. LogTeff for an age of 1Gyr. The result is an isochrone. Important - think about what we are looking at when we observe a cluster. We are seeing a “freeze-frame” picture at a particular age. We see how stars of different masse ...
Debris Belts around Vega - Astronomical Society of the Pacific
... *ESA = European Space Agency Figure is the glowing dust image after the contribution of the star has been taken out. Arrows point to the location of the belts. Colors represent intensity of light, from bright (red) to faint (blue).The inner belt is not resolved into a ring, but rather is detected as ...
... *ESA = European Space Agency Figure is the glowing dust image after the contribution of the star has been taken out. Arrows point to the location of the belts. Colors represent intensity of light, from bright (red) to faint (blue).The inner belt is not resolved into a ring, but rather is detected as ...
public_lector_10
... The dark halo was built up from mergers of smaller sub-halos Saw spiral structure developing in the gas Merging of galaxies is still going on now ...
... The dark halo was built up from mergers of smaller sub-halos Saw spiral structure developing in the gas Merging of galaxies is still going on now ...
Investigate Stars and Galaxies - American Museum of Natural History
... Lower Level (40 minutes) Using their student worksheets, have students visit the following two locations to collect evidence about stars. They can explore individually, in pairs, or in small groups. ...
... Lower Level (40 minutes) Using their student worksheets, have students visit the following two locations to collect evidence about stars. They can explore individually, in pairs, or in small groups. ...
Chapter 20
... case this force eventually became strong enough to counteract the effect of gravity pulling inward. ...
... case this force eventually became strong enough to counteract the effect of gravity pulling inward. ...
PRESENTATION NAME
... Careful examination has shown that the Milky Way viewed from an edge, looks like a flat disc with a central bulge and the thickness tapers off towards the edges. Milky Way is a conglomeration of stars (Such a huge group of stars is called a galaxy). The diameter of the Milky Way is about one lakh li ...
... Careful examination has shown that the Milky Way viewed from an edge, looks like a flat disc with a central bulge and the thickness tapers off towards the edges. Milky Way is a conglomeration of stars (Such a huge group of stars is called a galaxy). The diameter of the Milky Way is about one lakh li ...
Friday, April 25 - Otterbein University
... • In 1920 Hubble used this technique to measure the distance to Andromeda (about 2 million ly) • Works best for periodic variables ...
... • In 1920 Hubble used this technique to measure the distance to Andromeda (about 2 million ly) • Works best for periodic variables ...
Astronomy Talk July 2016 - Unitarian Universalist Church of
... appears every galaxy has one. Galaxies have a collection of stars gas and dust, sometimes in a spiral shapes, and galaxies have a SMBH. And scientists began to wonder, which came first, the SMBH or the stars and gas and dust? Sort of like the chicken and the egg question, which came first? Did a SMB ...
... appears every galaxy has one. Galaxies have a collection of stars gas and dust, sometimes in a spiral shapes, and galaxies have a SMBH. And scientists began to wonder, which came first, the SMBH or the stars and gas and dust? Sort of like the chicken and the egg question, which came first? Did a SMB ...
ppt - Astronomy & Physics
... Even stars like the Sun will become red giants, engulfing inner planets, and generally making life “difficult” throughout the solar system Supernovae also destroy life on nearby planets ...
... Even stars like the Sun will become red giants, engulfing inner planets, and generally making life “difficult” throughout the solar system Supernovae also destroy life on nearby planets ...
Galaxies - senwiki
... that nothing, not even light, can escape. -Why? Black holes have extremely strong gravitational pulls. They can pull in stars and accumulate the mass of the stars. -Where are black holes located? Astronomers believe that each galaxy contains at least one supermassive black hole at its centre. ...
... that nothing, not even light, can escape. -Why? Black holes have extremely strong gravitational pulls. They can pull in stars and accumulate the mass of the stars. -Where are black holes located? Astronomers believe that each galaxy contains at least one supermassive black hole at its centre. ...
the Full Chapter 6 -
... on board Earth-orbiting satellites. NASA’s Compton Gamma Ray Observatory flew in the 1990s. At the time, it was the biggest and most massive scientific satellite ever launched ...
... on board Earth-orbiting satellites. NASA’s Compton Gamma Ray Observatory flew in the 1990s. At the time, it was the biggest and most massive scientific satellite ever launched ...
Lecture9_2014_v2 - UCO/Lick Observatory
... causes it to spiral inwards » or scattering from other giant planets causes migration » why does it stop? ...
... causes it to spiral inwards » or scattering from other giant planets causes migration » why does it stop? ...
Variable Stars: Pulsation, Evolution and applications to Cosmology
... Recall equations of stellar structure. Nuclear energy generation rate ε(ρ,T) slowly changes the composition decreasing the amount of Hydrogen and increasing the amount of Helium on a nuclear time scale – the characteristic time for stellar properties to change as a result of nuclear burning: tnuc ~ ...
... Recall equations of stellar structure. Nuclear energy generation rate ε(ρ,T) slowly changes the composition decreasing the amount of Hydrogen and increasing the amount of Helium on a nuclear time scale – the characteristic time for stellar properties to change as a result of nuclear burning: tnuc ~ ...
Galaxies have different sizes and shapes.
... Our solar system lies within the Milky Way galaxy. The Sun lies within a galaxy called the Milky Way. Remember that a galaxy is a huge grouping of stars, gas, and dust held together by gravity. Without a telescope, you can only see nearby stars clearly. Those stars are a tiny fraction of the several ...
... Our solar system lies within the Milky Way galaxy. The Sun lies within a galaxy called the Milky Way. Remember that a galaxy is a huge grouping of stars, gas, and dust held together by gravity. Without a telescope, you can only see nearby stars clearly. Those stars are a tiny fraction of the several ...
The GAIA astrometric survey of extra
... the GAIA instrument [19] must meet the stringent requirement of 4 µas final astrometric accuracy on positions, proper motions, and parallaxes for bright targets (V < 13). In fact, in order to keep the ratio α/σψ = const., an increase in the measurement error implies an increase in the astrometric si ...
... the GAIA instrument [19] must meet the stringent requirement of 4 µas final astrometric accuracy on positions, proper motions, and parallaxes for bright targets (V < 13). In fact, in order to keep the ratio α/σψ = const., an increase in the measurement error implies an increase in the astrometric si ...
10.5 The Hertzsprung
... Many stars are in binary pairs; measurement of their orbital motion allows determination of the masses of the stars. Orbits of visual binaries can be observed directly; Doppler shifts in spectroscopic binaries allow measurement of motion; and the period of eclipsing binaries can be measured using in ...
... Many stars are in binary pairs; measurement of their orbital motion allows determination of the masses of the stars. Orbits of visual binaries can be observed directly; Doppler shifts in spectroscopic binaries allow measurement of motion; and the period of eclipsing binaries can be measured using in ...
The Missing Mass
... Centripetal force does not strongly effect the gas that is above and below the rotation plane. So … • Gas falling in from the top collides with gas falling in from the bottom. This gas sticks together and forms the galaxy’s disk. • All star formation now occurs in a disk (where all the gas is). The ...
... Centripetal force does not strongly effect the gas that is above and below the rotation plane. So … • Gas falling in from the top collides with gas falling in from the bottom. This gas sticks together and forms the galaxy’s disk. • All star formation now occurs in a disk (where all the gas is). The ...
PHYS178 2008 week 11 part-1
... recent report based on data from the Hubble Space Telescope seems to confirm this result. The even more recent observations made with the Spitzer Space Telescope of the warm infrared glows of two previously detected "hot Jupiter" planets is another interesting result in this context. This wealth of ...
... recent report based on data from the Hubble Space Telescope seems to confirm this result. The even more recent observations made with the Spitzer Space Telescope of the warm infrared glows of two previously detected "hot Jupiter" planets is another interesting result in this context. This wealth of ...
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.