PH607 – Galaxies
... Hubble found H0 ~ 500 km/s/Mpc !! Hubble had confused two different kinds of Cepheid variable stars used for calibrating distances and also that what Hubble thought were bright stars in distant galaxies were actually H II regions. Throughout the 20th century we found evidence for H0 in the range 50 ...
... Hubble found H0 ~ 500 km/s/Mpc !! Hubble had confused two different kinds of Cepheid variable stars used for calibrating distances and also that what Hubble thought were bright stars in distant galaxies were actually H II regions. Throughout the 20th century we found evidence for H0 in the range 50 ...
The Age Distribution of Potential Intelligent Life in the Milky Way
... difficult to measure because of our location in the disk (Binney and Tremaine, 2008) and the scale length at the formation of the Galaxy is unknown. Therefore, rd as well as ∑0 are included as variables in our model which are chosen to best match the present day observed quantities of the Galaxy. Th ...
... difficult to measure because of our location in the disk (Binney and Tremaine, 2008) and the scale length at the formation of the Galaxy is unknown. Therefore, rd as well as ∑0 are included as variables in our model which are chosen to best match the present day observed quantities of the Galaxy. Th ...
Extrasolar planets - Astronomisk Ungdom
... planets around other stars, it can also be combined with different mathematic operations and some information about the host star to reveal factors and properties of the planets. It is achievable to calculate such as radius, average mass, orbital velocity, orbital time, semi-major axis (distance to ...
... planets around other stars, it can also be combined with different mathematic operations and some information about the host star to reveal factors and properties of the planets. It is achievable to calculate such as radius, average mass, orbital velocity, orbital time, semi-major axis (distance to ...
By the time astronomers got a big telescope into orbit, they
... good as 0.4 arc second. A better solution ought to be to put a telescope above the atmosphere, in space. Satellites in space have been successfully detecting wavelengths other than the optical for years. The Hubble Space Telescope, with a 2.4-meter mirror, operates in optical (and ultraviolet) wavel ...
... good as 0.4 arc second. A better solution ought to be to put a telescope above the atmosphere, in space. Satellites in space have been successfully detecting wavelengths other than the optical for years. The Hubble Space Telescope, with a 2.4-meter mirror, operates in optical (and ultraviolet) wavel ...
The Formation and Evolution of the Milky Way
... great abundance of metals that could be incorporated into the star. As a general rule [Fe/H] increases with time so old objects are more metal poor than young ones. How stars make “metals” is now reasonably well understood. For the most part they are formed by a chain of fusion of lighter elements. ...
... great abundance of metals that could be incorporated into the star. As a general rule [Fe/H] increases with time so old objects are more metal poor than young ones. How stars make “metals” is now reasonably well understood. For the most part they are formed by a chain of fusion of lighter elements. ...
Kepler Mission
... wheel is a problem that cannot be left unfixed as it could lead to wearing out to the point of breaking.8 If this were to occur, then there would only be two reaction wheels left to keep the spacecraft from shifting from its targeted area. There would be a bigger strain on those two wheels. As a res ...
... wheel is a problem that cannot be left unfixed as it could lead to wearing out to the point of breaking.8 If this were to occur, then there would only be two reaction wheels left to keep the spacecraft from shifting from its targeted area. There would be a bigger strain on those two wheels. As a res ...
Chapter 15 Stars, Galaxies, and Universe
... What are the major types of galaxies? How do astronomers describe the scale of the universe? ...
... What are the major types of galaxies? How do astronomers describe the scale of the universe? ...
TELESCOPES - GeoEcoGeo.com
... 1. The Hubble Space Telescope orbits the earth and is capable of obtaining images of objects emitting most forms of light. 2. Overall, it is the most advanced and best telescope that we have available right now. 3. The mirror of this telescope is 2.5 meters in diameter. 4. Data collected by this tel ...
... 1. The Hubble Space Telescope orbits the earth and is capable of obtaining images of objects emitting most forms of light. 2. Overall, it is the most advanced and best telescope that we have available right now. 3. The mirror of this telescope is 2.5 meters in diameter. 4. Data collected by this tel ...
Curriculum Vitae - Centre for Astrophysics and Supercomputing
... (invited talk) • March 2014: ESO conference: Gas and Stars in Galaxies: A multiwavelength 3D Perspective, Garching, Germany (invited talk) • July 2013: EWASS 2013 Session: Starburst Galaxies Now and Then with ALMA, Turku, Finland (talk) • May – June 2013: Aspen Center for Physics Workshop Dusty Star ...
... (invited talk) • March 2014: ESO conference: Gas and Stars in Galaxies: A multiwavelength 3D Perspective, Garching, Germany (invited talk) • July 2013: EWASS 2013 Session: Starburst Galaxies Now and Then with ALMA, Turku, Finland (talk) • May – June 2013: Aspen Center for Physics Workshop Dusty Star ...
Formation of Globular Clusters: In and Out of Dwarf Galaxies
... in the context of galaxy formation? Not easy. Assuming that GCs follow galactic star formation rate produces too many red/metal-rich clusters with a unimodal metallicity distribution. Globular clusters formed earlier than the majority of field stars in host galaxy. ...
... in the context of galaxy formation? Not easy. Assuming that GCs follow galactic star formation rate produces too many red/metal-rich clusters with a unimodal metallicity distribution. Globular clusters formed earlier than the majority of field stars in host galaxy. ...
Optical Design of Giant Telescopes for Space
... Planetary science has been limited by the power of telescopes to the study of just our own solar system. Now the presence of numerous planets orbiting stars other than the sun is inferred from stellar reaction motion, but we lack the ability to see these planets directly. We also lack the technology ...
... Planetary science has been limited by the power of telescopes to the study of just our own solar system. Now the presence of numerous planets orbiting stars other than the sun is inferred from stellar reaction motion, but we lack the ability to see these planets directly. We also lack the technology ...
Report of the HST-JWST Transition Panel
... Except for the gyroscopes, only the thermal insulation and one of the Fine Guidance Sensors are presently degraded. SM4 is scheduled to repair the thermal insulation and replace the faulty Fine Guidance Sensor. Informed engineering estimates show that the HST must be revitalized by the Shuttle ever ...
... Except for the gyroscopes, only the thermal insulation and one of the Fine Guidance Sensors are presently degraded. SM4 is scheduled to repair the thermal insulation and replace the faulty Fine Guidance Sensor. Informed engineering estimates show that the HST must be revitalized by the Shuttle ever ...
1 Astrobiologically Interesting Stars within 10
... disrupted. Masses larger than 1.20 solar may remain acceptable if allowance is made for a faster evolution of complex life than was the case on Earth. Yet, besides these well-accepted notions, quite a few other considerations have recently been increasingly considered as playing fundamental roles fo ...
... disrupted. Masses larger than 1.20 solar may remain acceptable if allowance is made for a faster evolution of complex life than was the case on Earth. Yet, besides these well-accepted notions, quite a few other considerations have recently been increasingly considered as playing fundamental roles fo ...
Which planet has never been orbited or flown past by a
... Dr. C. Renee James NASA Top Stars 2010 ...
... Dr. C. Renee James NASA Top Stars 2010 ...
M81/M82/NGC3077
... M81 — -35 km/sec (3.63 ± 0.34 Mpc) (CBR value: 48 km/sec) M82 — 202 km/sec (3.9 ± 0.3 Mpc) (CBR value: 296 km/sec) M81 is closer and approaching, while M82 is farther away and receding; ...
... M81 — -35 km/sec (3.63 ± 0.34 Mpc) (CBR value: 48 km/sec) M82 — 202 km/sec (3.9 ± 0.3 Mpc) (CBR value: 296 km/sec) M81 is closer and approaching, while M82 is farther away and receding; ...
prof.-j.hill
... mounted side-by-side on the same mount to produce a collecting area equivalent to an 11.8-meter circular aperture. The two Gregorian telescope sides point at the same object, or groups of objects close together (1 arcmin) on the sky. A unique feature of LBT is that the light from the two primary mir ...
... mounted side-by-side on the same mount to produce a collecting area equivalent to an 11.8-meter circular aperture. The two Gregorian telescope sides point at the same object, or groups of objects close together (1 arcmin) on the sky. A unique feature of LBT is that the light from the two primary mir ...
Nulling Interferometer
... Send one beam through focus (Gay and Rabbia) Balance dispersion in air by dispersion in glass (Angel, Burge and Woolf) ...
... Send one beam through focus (Gay and Rabbia) Balance dispersion in air by dispersion in glass (Angel, Burge and Woolf) ...
Characterization of the four new transiting planets KOI
... orbital periods of 3.8 and 3.2 days, and masses of 0.25 and 0.34 MJup . They are located in the low-mass range of known transiting, giant planets. KOI-192b has a similar mass (0.29 MJup ) but a longer orbital period of 10.3 days. This places it in a domain where only a few planets are known. KOI-830 ...
... orbital periods of 3.8 and 3.2 days, and masses of 0.25 and 0.34 MJup . They are located in the low-mass range of known transiting, giant planets. KOI-192b has a similar mass (0.29 MJup ) but a longer orbital period of 10.3 days. This places it in a domain where only a few planets are known. KOI-830 ...
4-3.8 - S2TEM Centers SC
... By 1904, the Snow Solar Telescope was built and then moved to its permanent home atop Mount Wilson. It could study the sun in detail. In 1990, The unprecedented images that Hubble delivered represented the fulfillment of a 50-year dream and more than two decades of dedicated collaboration between sc ...
... By 1904, the Snow Solar Telescope was built and then moved to its permanent home atop Mount Wilson. It could study the sun in detail. In 1990, The unprecedented images that Hubble delivered represented the fulfillment of a 50-year dream and more than two decades of dedicated collaboration between sc ...
The Telescope - Salt Lake Astronomical Society
... History of the Telescope For as long as man has been capable of wondering, the night sky has provided subject material to wonder about. Trying to see more clearly and to find greater detail of the objects in the sky had been a desire of all the ancient astronomers. The true beginning of telescopes i ...
... History of the Telescope For as long as man has been capable of wondering, the night sky has provided subject material to wonder about. Trying to see more clearly and to find greater detail of the objects in the sky had been a desire of all the ancient astronomers. The true beginning of telescopes i ...
Lecture 12: Evolution of the Galaxy
... heavy element mass fraction, Z, at the time of their birth. The youngest stars are therefore the most heavy-element rich, and the oldest ones (Population II stars) are the most deficient in heavy elements relative to the Sun. • Halo Population II stars have Z ~ 10-3 to 10-1 Z⊙ • Disk Population I st ...
... heavy element mass fraction, Z, at the time of their birth. The youngest stars are therefore the most heavy-element rich, and the oldest ones (Population II stars) are the most deficient in heavy elements relative to the Sun. • Halo Population II stars have Z ~ 10-3 to 10-1 Z⊙ • Disk Population I st ...
The Milky Way disk
... Abstract / This review summarises the invited presentation I gave on the Milky Way disc. The idea underneath was to touch those topics that can be considered hot nowadays in the Galactic disk research: the reality of the thick disk, the spiral structure of the Milky Way, and the properties of the ou ...
... Abstract / This review summarises the invited presentation I gave on the Milky Way disc. The idea underneath was to touch those topics that can be considered hot nowadays in the Galactic disk research: the reality of the thick disk, the spiral structure of the Milky Way, and the properties of the ou ...
The Milky Way thin disk structure as revealed by stars and young
... experienced quite a significant burst of activity. This is mostly because of the failure of HI studies, that cannot go much beyond the detection of gas density peaks in the velocity space (McClure-Griffiths et al. 2004; Dame et al 2011), and struggle in the process of translating these velocities into ...
... experienced quite a significant burst of activity. This is mostly because of the failure of HI studies, that cannot go much beyond the detection of gas density peaks in the velocity space (McClure-Griffiths et al. 2004; Dame et al 2011), and struggle in the process of translating these velocities into ...
File 11 - School of Astronomy, IPM
... Galaxy Morphology Discovering Galaxies • In late 1700, Messier made a catalog of 109 nebulae so that comet hunters wouldn’t mistake them for comets! ~40 of these were galaxies • NGC New General Catalogue (Dreyer 1888) had 7840 objects, of which ~50% were galaxies • In the 20th century, many catalog ...
... Galaxy Morphology Discovering Galaxies • In late 1700, Messier made a catalog of 109 nebulae so that comet hunters wouldn’t mistake them for comets! ~40 of these were galaxies • NGC New General Catalogue (Dreyer 1888) had 7840 objects, of which ~50% were galaxies • In the 20th century, many catalog ...
powerpoint - Physics @ IUPUI
... the universe therefore the sizes and distributions tell you something about the distribution of dark matter when the universe formed! • Also, since the curvature of the universe (aka the cosmological constant) changes the shapes of voids as we see them, we can gain some understanding of what the cur ...
... the universe therefore the sizes and distributions tell you something about the distribution of dark matter when the universe formed! • Also, since the curvature of the universe (aka the cosmological constant) changes the shapes of voids as we see them, we can gain some understanding of what the cur ...
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.