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What is a standard candle?
What is a standard candle?

... Both stars have the same average apparent brightness. The star in galaxy A has a bright-dim-bright period of 10 days, while the one in galaxy B has a bright-dim-bright period of 30 days. Which of the two galaxies is at a greater distance from us? a) ...
Neutron Stars and Black Holes
Neutron Stars and Black Holes

The Changing Earth Atmosphere
The Changing Earth Atmosphere

... The ultraviolet and X-ray flux of solar-like stars primarily arises from chromospheric and coronal regions of a stellar atmosphere. These 2 regions are hotter than the underlying photosphere where the bulk of the energy flux is emitted. This heating primarily arises from magnetic fields on the surfa ...
A Reappraisal of The Habitability of Planets around M Dwarf Stars
A Reappraisal of The Habitability of Planets around M Dwarf Stars

... planets from an HZ expanded astronomers’ attention beyond planetary systems that were exact analogs of our Solar System. This broadening of astronomical perspective combined with the discovery of hydrothermal habitats that are apparently independent of the Sun (Corliss et al., 1979), an increasing a ...
A re-appraisal of the habitability of planets around M dwarf
A re-appraisal of the habitability of planets around M dwarf

A n   A n c i e n... How Astronomers Know the Vast Scale of Cosmic Time
A n A n c i e n... How Astronomers Know the Vast Scale of Cosmic Time

... Over a hundred of these stars are now known to have planets, just the way the Sun does. Some stars show evidence of being much older than the Sun, and some are just gathering together from the raw material of the galaxy. One of the nicest things about the universe is that it sends its information to ...
uniview glossary - DMNS Galaxy Guide Portal
uniview glossary - DMNS Galaxy Guide Portal

... Saturn was named for the Roman god of agriculture and lies 885 million miles from the Sun, (9.6 AU). Saturn takes 29.5 years to orbit, but only 10.7 hours to rotate (day). Its diameter is 75,000 miles, making it the second largest planet. Its mass is 95 times that of Earth. It is the second of the f ...
Effect of the stellar spin history on the tidal evolution of close
Effect of the stellar spin history on the tidal evolution of close

... and very low-mass stars (0.1 M ). We tested two stellar spin evolution profiles, one with fast initial rotation (1.2 day rotation period) and one with slow initial rotation (8 day period). We tested the effect of varying the stellar and planetary dissipations, and the planet’s mass and initial orbit ...
Lesson 3: Calculating distances to stars
Lesson 3: Calculating distances to stars

... the star is very far away, then the brightness of the star can be used to estimate the distance to the star. It is a rather simple principle; if a star is close by then it will appear bright, and if the star is far away it will appear dim. This method was first proposed by the Dutch astronomer, Chri ...
Chapter 19. Mapping the Universe from Herschel to Sloan
Chapter 19. Mapping the Universe from Herschel to Sloan

... slow process because you need to get many images of a galaxy spread out over more than a year and discover all the Cepheids, measure their brightnesses as a function of time, etc. Fortunately, a second discovery by Hubble has made this process much easier. While studying the velocities of galaxies ( ...
of light
of light

... TODAY’S Sun as seen in visible light from Earth and from space in X-rays by satellites ...
DSLR Photometry
DSLR Photometry

... CCD chip are not continuous and have gaps separating them, if light only falls on a couple of pixels, a significant amount will fall in the gaps and be lost. The more pixels covered, the less percentage of the light is lost to the cracks. ...
PDF
PDF

... the two nearest wavelengths at which high contrast was constrained (700 and 800 nm). Once a profile is created by optimization, we use equation (9) to calculate the effect of converting a smooth apodization to petals; this petalization tends to reduce the width of the shadow at certain angles. In a ...
Astronomy_Stellar_Evolution_and_Type_II_Supernovae_Exam
Astronomy_Stellar_Evolution_and_Type_II_Supernovae_Exam

The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL)
The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL)

... N2H+, HCN, HCO+, NH2D, ...), tracing a broad range of physical conditions. Such a large dataset also provides valuable information on the chemical processes occurring within the sources. A detailed analysis of these data is in progress (Wyrowski et al., in preparation). A smaller sample was also obs ...
Chapter 1 Seeing the Light: The Art and Science of Astronomy
Chapter 1 Seeing the Light: The Art and Science of Astronomy

... and Saturn. These celestial bodies aren’t wandering through the stars; they orbit around the Sun, our solar system’s central star. Today astronomers know that planets can be smaller or bigger than Earth, but they all are much smaller than the Sun. The planets in our solar system are so close to Eart ...
Here - Amateur Observers` Society of New York
Here - Amateur Observers` Society of New York

Secular Increase of the Astronomical Unit: a Possible Explanation in
Secular Increase of the Astronomical Unit: a Possible Explanation in

... now, several authors have discussed a redefinition of the system of astronomical units, e.g., Huang et al. (1995); Standish (2005); Klioner (2008); Capitaine and Guinot (2009). By using equations (1) and (24), we obtain GMSun in SI units, and so far GMSun is conventionally regarded as being a “fixed ...
X-ray binaries
X-ray binaries

... LMXBs with NSs or BHs The latest large catalogue (Li et al. arXiv: 0707.0544) includes 187 galactic and Magellanic Clouds LMXBs with NSs and BHs as accreting components. Donors can be WDs, or normal low-mass stars (main sequence or sub-giants). Many sources are found in globular clusters. Also ther ...
X-ray binaries
X-ray binaries

... LMXBs with NSs or BHs The latest large catalogue (Li et al. arXiv: 0707.0544) includes 187 galactic and Magellanic Clouds LMXBs with NSs and BHs as accreting components. Donors can be WDs, or normal low-mass stars (main sequence or sub-giants). Many sources are found in globular clusters. Also ther ...
Advanced STARS - WordPress.com
Advanced STARS - WordPress.com

...  It is known as the red planet due to its appearance when seen from earth at night  It is the only planet besides Earth that has seasons  It has a rotational period nearly the same as earth  Its orbit takes 687 days  Mars has 2 moons  It has the largest dust storms in the solar system  It has ...
5 Report of the Panel on Stars and Stellar Evolution
5 Report of the Panel on Stars and Stellar Evolution

... comprise great chunks of introductory astronomy textbooks and although the tools for these investigations are tested and sharp, many of the simplest assertions about the formation of white dwarfs, mass loss from giant stars, and the evolution of binary stars are based on conjecture and a slender fou ...
siamois
siamois

... • launched on December 27th , 2006 • by Soyuz 2, from Baikonour, Kazakhstan • low Earth polar orbit, 896 km altitude • orbital period 6184 s (~1h43mn, 162 mHz) • high precision photometry ...
Document
Document

... Alnilam: "Epsilon Orionis," is a blue supergiant, despite being nearly twice as far from the Sun as Mintake and Alnitak, the other two belt stars. ...
Habitable Planets Webquest
Habitable Planets Webquest

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