Measuring the Milky Way
... The orbital speed of an object depends only on the amount of mass between it and the Galactic center: ...
... The orbital speed of an object depends only on the amount of mass between it and the Galactic center: ...
Stellar Pops 2
... • CMD studies: Derive age/metallicity mix of a population – to HB (current limit, M31 group) – to 12Gyr main-sequence turnoff (current limit, Milky Way Galaxy companions) ...
... • CMD studies: Derive age/metallicity mix of a population – to HB (current limit, M31 group) – to 12Gyr main-sequence turnoff (current limit, Milky Way Galaxy companions) ...
2007_AO - University of Hawaii
... Applied Optics Group (Imperial College), Herschel 4.2-m Telescope ...
... Applied Optics Group (Imperial College), Herschel 4.2-m Telescope ...
telescope as time machine - Galaxy Evolution Explorer
... that gave the universe its start around 12 billion years ago (give or take a few billion years). The Galaxy Evolution Explorer, or GALEX for short, is an Earth-orbiting telescope that is looking back 10 billion years to help scientists understand how galaxies like our Milky Way came to be and how th ...
... that gave the universe its start around 12 billion years ago (give or take a few billion years). The Galaxy Evolution Explorer, or GALEX for short, is an Earth-orbiting telescope that is looking back 10 billion years to help scientists understand how galaxies like our Milky Way came to be and how th ...
life
... even if they do exist, United Federation of Planets probably precluded by large distances (at least on basis of current physics) ...
... even if they do exist, United Federation of Planets probably precluded by large distances (at least on basis of current physics) ...
Solar systems like ours may be rare - Space.com
... Launch research. "Perhaps some other stars already formed planets. It's only a snapshot in time and as you look at other clusters at different ages you can build up a better picture." Other scientists agree there are many unanswered questions about solar systems beyond our own. "As the precision wit ...
... Launch research. "Perhaps some other stars already formed planets. It's only a snapshot in time and as you look at other clusters at different ages you can build up a better picture." Other scientists agree there are many unanswered questions about solar systems beyond our own. "As the precision wit ...
Miss Nevoral - Ms. Nevoral`s site
... 7. How does the speed at which a galaxy rotates affect its shape? The more spin a galaxy has, the flatter it will be. 8. Besides shape, what other ways do galaxies differ from each other? Galaxies differ in size, mass, brightness, colour, and speed of spin. 9. Describe the two different types of sta ...
... 7. How does the speed at which a galaxy rotates affect its shape? The more spin a galaxy has, the flatter it will be. 8. Besides shape, what other ways do galaxies differ from each other? Galaxies differ in size, mass, brightness, colour, and speed of spin. 9. Describe the two different types of sta ...
Apr - Eugene Astronomical Society
... some galaxies, whatever’s up there. Oh, and I don’t want to spend too much money.” This question, from someone wanting to get their first (or first decent - or sizable) telescope can generate lots of discussion and different opinions. But the qualifier “I don’t want to spend too much money,” for mos ...
... some galaxies, whatever’s up there. Oh, and I don’t want to spend too much money.” This question, from someone wanting to get their first (or first decent - or sizable) telescope can generate lots of discussion and different opinions. But the qualifier “I don’t want to spend too much money,” for mos ...
Testing
... themselves • Indirect: Measurements of stellar properties revealing the effects of orbiting planets ...
... themselves • Indirect: Measurements of stellar properties revealing the effects of orbiting planets ...
GEARS Workshop Monday - Georgia Southern University
... • Complete this exercise in groups of 2 to 3. • This is designed to be completed while you are discussing with other people. • This is not designed to be completed on your own. (despite the fact we keep assigning them as homework) ...
... • Complete this exercise in groups of 2 to 3. • This is designed to be completed while you are discussing with other people. • This is not designed to be completed on your own. (despite the fact we keep assigning them as homework) ...
galaxy.
... Using redshifts to derive distances: Since the Hubble constant H0 is the slope of the line in the Hubble diagram, we can write ...
... Using redshifts to derive distances: Since the Hubble constant H0 is the slope of the line in the Hubble diagram, we can write ...
NAM_f2
... instrument with an effective cadence of 100 minutes and a total mission lifetime of 3 years (2 of which have already been completed) we are able to build up lightcurves of over 34,000 stars with I brighter than 8th mag. Early results suggest that we will be able to achieve the required photometric a ...
... instrument with an effective cadence of 100 minutes and a total mission lifetime of 3 years (2 of which have already been completed) we are able to build up lightcurves of over 34,000 stars with I brighter than 8th mag. Early results suggest that we will be able to achieve the required photometric a ...
Spectral Variations of Several RV Tauri Type Stars Patrick Durant
... We have examined the spectra of several RV Tauri type stars including AC Her, SX Her and V Vul. As is typical of this variable type, the stars show changes in spectral type and line strength in addition to changes in their light curve over time. Our group has acquired spectra of these stars during t ...
... We have examined the spectra of several RV Tauri type stars including AC Her, SX Her and V Vul. As is typical of this variable type, the stars show changes in spectral type and line strength in addition to changes in their light curve over time. Our group has acquired spectra of these stars during t ...
Sample pages 2 PDF
... To understand something of the elements which determine f star we must review some aspects of the current understanding of the history of the universe. Evidence arising from observations of the rate at which stars and galaxies are receding from the earth indicates that, approximately 14 billion year ...
... To understand something of the elements which determine f star we must review some aspects of the current understanding of the history of the universe. Evidence arising from observations of the rate at which stars and galaxies are receding from the earth indicates that, approximately 14 billion year ...
Disks around new stars and planet formation
... inclination of planet orbit (Mp sin(i) è Mp). Atacama Large Millimeter Array (ALMA) – World wide project to be completed in 2010. Will study how planets form by imaging accretion & debris disks, trace disk velocity structure, image proto-Jupiter planets, map gaps in disks where planets may be formin ...
... inclination of planet orbit (Mp sin(i) è Mp). Atacama Large Millimeter Array (ALMA) – World wide project to be completed in 2010. Will study how planets form by imaging accretion & debris disks, trace disk velocity structure, image proto-Jupiter planets, map gaps in disks where planets may be formin ...
Accretion Disks around Stars and the Process of Planet Formation
... inclination of planet orbit (Mp sin(i) è Mp). Atacama Large Millimeter Array (ALMA) – World wide project to be completed in 2010. Will study how planets form by imaging accretion & debris disks, trace disk velocity structure, image proto-Jupiter planets, map gaps in disks where planets may be formin ...
... inclination of planet orbit (Mp sin(i) è Mp). Atacama Large Millimeter Array (ALMA) – World wide project to be completed in 2010. Will study how planets form by imaging accretion & debris disks, trace disk velocity structure, image proto-Jupiter planets, map gaps in disks where planets may be formin ...
Document
... • We define our age by trips around the Sun. • How many trips of Sun around Milky Way? R = 8.5 kpc V = 220km/s P = 2.5x108 yrs ...
... • We define our age by trips around the Sun. • How many trips of Sun around Milky Way? R = 8.5 kpc V = 220km/s P = 2.5x108 yrs ...
Powerpoint presentation, Created by Debra Shepherd, NRAO, 2002
... being built in Chile, PRIMA available in 2005. Will be able to solve for inclination of planet orbit (Mp sin(i) Mp). Atacama Large Millimeter Array (ALMA) – World wide project to be completed in 2010. Will study how planets form by imaging accretion & debris disks, trace disk velocity structure, i ...
... being built in Chile, PRIMA available in 2005. Will be able to solve for inclination of planet orbit (Mp sin(i) Mp). Atacama Large Millimeter Array (ALMA) – World wide project to be completed in 2010. Will study how planets form by imaging accretion & debris disks, trace disk velocity structure, i ...
TRANSIT
... and data reduction; there will be something for everyone from the very beginner to the ambitious student. Apart from the astronomical program, there are many non-astronomical activities such as group games, sporting events, singing evenings, hiking tours and an excursion. Since it is an internationa ...
... and data reduction; there will be something for everyone from the very beginner to the ambitious student. Apart from the astronomical program, there are many non-astronomical activities such as group games, sporting events, singing evenings, hiking tours and an excursion. Since it is an internationa ...
The Dynamics-Based Approach to Studying Terrestrial Exoplanets
... of which 239 are M dwarfs and only 21 are G dwarfs. Projecting these numbers by volume, we expect 10,000 M-dwarf stars within 35 pc. This estimate is consistent with the number of Mdwarfs in that volume identified by large proper motions and 2MASS photometry (Lepine & Shara 2005; Lepine 2005) but fo ...
... of which 239 are M dwarfs and only 21 are G dwarfs. Projecting these numbers by volume, we expect 10,000 M-dwarf stars within 35 pc. This estimate is consistent with the number of Mdwarfs in that volume identified by large proper motions and 2MASS photometry (Lepine & Shara 2005; Lepine 2005) but fo ...
Integrative Studies 410 Our Place in the Universe
... – large mass contained in a very small volume at center of our Galaxy – Much of the mass of the Galaxy is not observed • consists neither of stars, nor of gas or dust • extends far beyond visible part of our galaxy (“dark ...
... – large mass contained in a very small volume at center of our Galaxy – Much of the mass of the Galaxy is not observed • consists neither of stars, nor of gas or dust • extends far beyond visible part of our galaxy (“dark ...
Stellar Explosions
... Johannes Kepler (1571–1630) was a German mathematician, astronomer, astrologer, and key figure in the 17th century astronomical revolution. Kepler is most famous for his three laws of planetary motion, which explained and predicted the positions of the planets much better than previous ideas. His wo ...
... Johannes Kepler (1571–1630) was a German mathematician, astronomer, astrologer, and key figure in the 17th century astronomical revolution. Kepler is most famous for his three laws of planetary motion, which explained and predicted the positions of the planets much better than previous ideas. His wo ...
The Milky Way * A Classic Galaxy
... Udalski et al. 2001), as long as one uses infrared luminosities. This is what modern astronomers do. (in the old days, before IR technology, this issue caused a lot of confusion in using Cepheids as distance indicators!) ...
... Udalski et al. 2001), as long as one uses infrared luminosities. This is what modern astronomers do. (in the old days, before IR technology, this issue caused a lot of confusion in using Cepheids as distance indicators!) ...
the rest of the univ..
... A myriad of comets and other debris orbiting at distances up to ;;; complete our Solar System. The Kuiper Belt and The Oort Cloud In 1950 Jan Oort noticed that: 1.no comet has been observed with an orbit that indicates that it came from interstellar space. 2.there is a strong tendency for aphelia of ...
... A myriad of comets and other debris orbiting at distances up to ;;; complete our Solar System. The Kuiper Belt and The Oort Cloud In 1950 Jan Oort noticed that: 1.no comet has been observed with an orbit that indicates that it came from interstellar space. 2.there is a strong tendency for aphelia 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.