AST4930 Star and Planet Formation
... Spectroscopic analysis can identify if an early type star is in main-sequence or already leaving the main sequence. In the first case, it follows a given temperature-luminosity relation, which can be exploited to determine their distance (but reddening must be corrected for). ...
... Spectroscopic analysis can identify if an early type star is in main-sequence or already leaving the main sequence. In the first case, it follows a given temperature-luminosity relation, which can be exploited to determine their distance (but reddening must be corrected for). ...
81 KB - CSIRO Publishing
... Milky Way ‘dwarf spheroidal galaxies’ and ‘dwarf elliptical galaxies’ are not galaxies. Hosts a Satellite Stellar System Evidence that a galaxy dominates its environment could come from the presence of smaller satellite stellar systems, such as dwarf galaxies (for large galaxies) or globular clust ...
... Milky Way ‘dwarf spheroidal galaxies’ and ‘dwarf elliptical galaxies’ are not galaxies. Hosts a Satellite Stellar System Evidence that a galaxy dominates its environment could come from the presence of smaller satellite stellar systems, such as dwarf galaxies (for large galaxies) or globular clust ...
Characteristics of Stars
... distance from Earth and how bright the star actually is. The brightness of a star can be described in two different ways: apparent brightness and absolute brightness. A star’s apparent brightness is its brightness as seen from Earth. Astronomers can measure apparent brightness fairly easily using el ...
... distance from Earth and how bright the star actually is. The brightness of a star can be described in two different ways: apparent brightness and absolute brightness. A star’s apparent brightness is its brightness as seen from Earth. Astronomers can measure apparent brightness fairly easily using el ...
EASTERN ARIZONA COLLEGE Lab - Introduction to Astronomy
... those motions to the Earth’s seasons, variation in day length, and climate and to the development of the calendar Learning objectives What you will learn as you master the competency: a. ...
... those motions to the Earth’s seasons, variation in day length, and climate and to the development of the calendar Learning objectives What you will learn as you master the competency: a. ...
Collaborations with East Asian VLBI stations
... 4 others from VLBA • Pitch angle of Perseus arm 16 +/- 3 deg four arm spiral ? ...
... 4 others from VLBA • Pitch angle of Perseus arm 16 +/- 3 deg four arm spiral ? ...
Astro 6590: Galaxies and the Universe Astro
... stars, plus an amount up to 1/2 of as much by mass of gas, and about 10X as much by mass of dark matter. The stars and gas are about 70% hydrogen by mass and 25% helium, the rest being heavier elements (called "metals"). • Typical scales are: masses between 106 to 1012 M (1 solar mass is 2 x 1030 k ...
... stars, plus an amount up to 1/2 of as much by mass of gas, and about 10X as much by mass of dark matter. The stars and gas are about 70% hydrogen by mass and 25% helium, the rest being heavier elements (called "metals"). • Typical scales are: masses between 106 to 1012 M (1 solar mass is 2 x 1030 k ...
Our Galaxy
... 2. What type of galaxy is our galaxy? 3. Where is the sun in our galaxy? 4. Describe the motion of the sun. 5. How old is our galaxy? 6. What make up more than 90% of our galaxy? What is it? 7. Which direction is the center of out galaxy? 8. What will you find out the center of our galaxy? 9. Will o ...
... 2. What type of galaxy is our galaxy? 3. Where is the sun in our galaxy? 4. Describe the motion of the sun. 5. How old is our galaxy? 6. What make up more than 90% of our galaxy? What is it? 7. Which direction is the center of out galaxy? 8. What will you find out the center of our galaxy? 9. Will o ...
Free floating planets
... light to find wobbles in different wave lengths. Those wobbles can reveal the existence of other worlds. What they revealed is a planet circling the red dwarf star, Gliese 581. The discovery of the new planet, named Gliese 581 c, is sure to fuel studies of planets circling similar dim stars. About 8 ...
... light to find wobbles in different wave lengths. Those wobbles can reveal the existence of other worlds. What they revealed is a planet circling the red dwarf star, Gliese 581. The discovery of the new planet, named Gliese 581 c, is sure to fuel studies of planets circling similar dim stars. About 8 ...
30 Doradus - HubbleSOURCE
... 1. Gigantic regions of star formation are complex systems where different generations of star affect each other’s evolution 2. At high redshift we cannot see the complexity of the star forming regions, and we derive a simplified history of star formation 3. A comparison between what we see in nearby ...
... 1. Gigantic regions of star formation are complex systems where different generations of star affect each other’s evolution 2. At high redshift we cannot see the complexity of the star forming regions, and we derive a simplified history of star formation 3. A comparison between what we see in nearby ...
Document
... • The Local Group counts more than 54 galaxies (the majority are dwarf galaxies). • Its center is somewhere between the Milky Way and the Andromeda galaxy (M31). • Its diameter is ~10,000,000 light years. • The total mass of the Local Group is ~1012 the mass of our sun, and more that 2 times the tot ...
... • The Local Group counts more than 54 galaxies (the majority are dwarf galaxies). • Its center is somewhere between the Milky Way and the Andromeda galaxy (M31). • Its diameter is ~10,000,000 light years. • The total mass of the Local Group is ~1012 the mass of our sun, and more that 2 times the tot ...
TMT Scientific Information Brochure
... uncovered. Researchers will be able to use TMT to study supermassive black holes (SMBH) across the entire Hubble sequence and study their demography as a function of environment. TMT observations will also extend dynamical measurements of massive black holes to z~0.4 and SMBHs throughout the Univers ...
... uncovered. Researchers will be able to use TMT to study supermassive black holes (SMBH) across the entire Hubble sequence and study their demography as a function of environment. TMT observations will also extend dynamical measurements of massive black holes to z~0.4 and SMBHs throughout the Univers ...
Cartwheel Galaxy - Chandra X
... Galaxy was probably a normal spiral structure galaxy similar to the Milky Way Galaxy before the collision. The spiral structure is beginning to re-emerge, as seen in the faint arms or spokes between the outer ring and the bulls-eye shaped nucleus. The gravitational disruption of a smaller intruder g ...
... Galaxy was probably a normal spiral structure galaxy similar to the Milky Way Galaxy before the collision. The spiral structure is beginning to re-emerge, as seen in the faint arms or spokes between the outer ring and the bulls-eye shaped nucleus. The gravitational disruption of a smaller intruder g ...
ch 31, stars
... • A spectroscope uses a prism or diffraction grating to disperse the light into its component wavelengths. • The separated wavelengths are called the spectrum of the star. • The spectrum can determine a star’s chemical composition, its surface temperature, and whether it is moving away from or towar ...
... • A spectroscope uses a prism or diffraction grating to disperse the light into its component wavelengths. • The separated wavelengths are called the spectrum of the star. • The spectrum can determine a star’s chemical composition, its surface temperature, and whether it is moving away from or towar ...
STApr18
... So what has all this to do with brown dwarfs? Solving the missing mass problem requires objects with high mass-to-light ratios – Vega – 2.5 solar mass A star: M/L ~ 0.05 Sun - 1 solar mass G dwarf: M/L = 1 Proxima – 0.1 solar mass M5 dwarf: M/L ~ 85 Gl 229B – 0.05 solar mass BD: M/L~ 8000 low mass ...
... So what has all this to do with brown dwarfs? Solving the missing mass problem requires objects with high mass-to-light ratios – Vega – 2.5 solar mass A star: M/L ~ 0.05 Sun - 1 solar mass G dwarf: M/L = 1 Proxima – 0.1 solar mass M5 dwarf: M/L ~ 85 Gl 229B – 0.05 solar mass BD: M/L~ 8000 low mass ...
Stars
... • These stars are extremely large! (about 10x the diameter of the Sun) • They have an extremely high ...
... • These stars are extremely large! (about 10x the diameter of the Sun) • They have an extremely high ...
FROM MOLECULAR CLOUDS TO STARS 1 Star formation and the
... circumstellar material, but still grouped in a cluster that demonstrates their common origin. Region 1b) where star formation is going on since ~ 7 Myr: on the right side of the cloud some new formed stars appear free from the cloud material (among them ε Ori), while others are still embedded at the ...
... circumstellar material, but still grouped in a cluster that demonstrates their common origin. Region 1b) where star formation is going on since ~ 7 Myr: on the right side of the cloud some new formed stars appear free from the cloud material (among them ε Ori), while others are still embedded at the ...
The Parallax Activity: Measuring the Distances to
... 1. The distance of Earth to the sun (one AU) is very small compared to interstellar distances, so parallax angles are smaller than one arcsecond, which is 1/3600 of a degree. 2. An alternative distance measurement for stars used by most astronomers is the ...
... 1. The distance of Earth to the sun (one AU) is very small compared to interstellar distances, so parallax angles are smaller than one arcsecond, which is 1/3600 of a degree. 2. An alternative distance measurement for stars used by most astronomers is the ...
Gemini - Sochias
... Gemini/Hokupa’a. BD can exist that close to the main star (Liu et al. AJ, 2002) ...
... Gemini/Hokupa’a. BD can exist that close to the main star (Liu et al. AJ, 2002) ...
Investigate Planets, Stars, Galaxies, and the Universe
... the city, state, country, and continent. Continue with Earth, the Solar System, the Milky Way Galaxy, the Virgo Supercluster, and the observable universe (the school’s “long address”). This will give students a sense of their place in space. Next, have them watch a video called “The Known Universe” ...
... the city, state, country, and continent. Continue with Earth, the Solar System, the Milky Way Galaxy, the Virgo Supercluster, and the observable universe (the school’s “long address”). This will give students a sense of their place in space. Next, have them watch a video called “The Known Universe” ...
Ecosystems, from life, to the Earth, to the Galaxy
... Our Milky Way galaxy displays the same characteristics that we associate with ecosystems if we view it on appropriately large scales of distance and time. This can most clearly be seen if we take an imaginary trip outside our Galaxy, to view it from afar. Seen face-on the Galaxy appears as a spiral, ...
... Our Milky Way galaxy displays the same characteristics that we associate with ecosystems if we view it on appropriately large scales of distance and time. This can most clearly be seen if we take an imaginary trip outside our Galaxy, to view it from afar. Seen face-on the Galaxy appears as a spiral, ...
Lecture 3, Optical and UV Astronomy
... (an example of spherical aberration) The Hubble primary mirror was polished to an incorrect shape meaning it is slightly too flat on the edges and light was not all focused to the same point. Hubble was then given eyeglasses in the form of COSTAR (Corrective Optics Space Telescope Axial Replacement) ...
... (an example of spherical aberration) The Hubble primary mirror was polished to an incorrect shape meaning it is slightly too flat on the edges and light was not all focused to the same point. Hubble was then given eyeglasses in the form of COSTAR (Corrective Optics Space Telescope Axial Replacement) ...
Planet Formation
... Planets form from the accretion disk present around a young star. Rocky planets like the terrestrial planets of the solar system form mainly from the dust inside this disk while gas giants are mainly build out of gas, with a solid core. The formation occurs in various steps. The first step is for th ...
... Planets form from the accretion disk present around a young star. Rocky planets like the terrestrial planets of the solar system form mainly from the dust inside this disk while gas giants are mainly build out of gas, with a solid core. The formation occurs in various steps. The first step is for th ...
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.