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Light of Distant Stars - Glasgow Science Centre
Light of Distant Stars - Glasgow Science Centre

... The Transit of Venus —Jeremiah Horrocks Jeremiah Horrocks was an English astronomer who lived in the 17th century. He wrote about the first observed transit of Venus. Here is his account of the event, as taken from his book Venus in Sole Visa: When the time of the observation approached, I retired ...
Groups of Stars
Groups of Stars

... generally not close to one another.  Lie in the same general direction of the sky as seen from Earth. ...
Quantification of Distant Luminous Objects
Quantification of Distant Luminous Objects

... the curve can be integrated, and the total energy flux in photons has now been obtained. As supernovae give half of the total energy as neutrinos, double the final answer for the total energy output. Note that a photon of visible light has an energy of about two electron volts, which can be converte ...
Stars
Stars

... • If the remaining mass of the star is about 1.4 times that of our Sun, the core is unable to support itself and it will collapse further to become a neutron star • Neutron star = star remnant that results from collapse of a massive star after a ...
Celestial Coordinate System
Celestial Coordinate System

... Local Mean Time: This is the mean solar time applied to your exact location. L.M.T. is calculated by applying a correction equal to four minutes for each degree you are away from the central meridian of your time zone. The central meridian for the Eastern Time zone is 75 degrees. Providence is locat ...
White dwarfs that crossed the Chandrasekhar limit
White dwarfs that crossed the Chandrasekhar limit

Astronomy Talk July 2016 - Unitarian Universalist Church of
Astronomy Talk July 2016 - Unitarian Universalist Church of

... We, the Member Congregations of the Unitarian Universalist Association, covenant to affirm and promote…Respect for the interdependent web of all existence of which we are a part.” 2) Skeptics and True Believers by Chet Raymo. Page 47 Let this, then, be the ground of my faith: All that we know, now a ...
Study Guide
Study Guide

... • Stars on the lower left of the H-R Diagram fainter than Main Sequence stars of the same Temperature. – Means they must be smaller in radius. – L-R-T Relation predicts: R ~ 0.01 Rsun (~ size of Earth!) ...
WORD - hrsbstaff.ednet.ns.ca
WORD - hrsbstaff.ednet.ns.ca

... 12. An imaginary sphere of infinite extent with Earth at its center on which the stars, planets, and other heavenly bodies appear to be located is known as the a. Zodiac. b. celestial sphere. c. atmosphere. d. Valhalla. 13. Which one of the following statements is true about the celestial coordinat ...
1.1 Current and Evolved Baseline - Mullard Space Science Laboratory
1.1 Current and Evolved Baseline - Mullard Space Science Laboratory

... 1.1.1.7 Advanced Composition Explorer (ACE) (Civil) (Current Baseline) The Advanced Composition Explorer (ACE) spacecraft uses high-resolution sensors and monitoring instruments to sample low-energy solar particles and high-energy galactic particles, energetic ions and electrons, and magnetic field ...
Name: Period: ___ Date: ______ Light-year Calculation
Name: Period: ___ Date: ______ Light-year Calculation

... Distances are so great in space that a special unit of measurement is used. It is called a light-year. This sounds like a measurement of time, but it is a unit used to measure distance. By definition a light-year is the distance that light travels in one year. To calculate the distance of one light- ...
UCO Focus - Lick Observatory
UCO Focus - Lick Observatory

... planets orbiting HD 7924, discovering the innermost planet in 2009 using the HIRES instrument installed on the 10-meter Keck I telescope. This same combination was also used to find other super-Earths orbiting nearby stars in planet searches led by UH astronomer Andrew Howard and UC Berkeley Profess ...
Light & Telescopes
Light & Telescopes

...  Earth’s atmosphere is fairly transparent to most visible light and radio waves, along with some infrared and ultraviolet radiation arriving from space, but it absorbs much of the electromagnetic radiation at other wavelengths. ...
Web SERVICE
Web SERVICE

... Spatial Data Access – SQL extension ...
29-4 - Fremont Peak Observatory
29-4 - Fremont Peak Observatory

... 14° 48.4’. R Lep is a “Carbon Star,” and as such it is a long period variable star. It is often called “Hind’s Crimson Star” because of its colour. British astronomer J. R. Hind first observed the star in 1845. Hind reported that the star appeared “like a drop of blood on a black field.” R Lep varie ...
Fatal Fling Solar Plasma at a Slow Pace - Max-Planck
Fatal Fling Solar Plasma at a Slow Pace - Max-Planck

... Thus far, a tiny finger bone and two back teeth in a cave in the Altai Mountains are the only known remains of the Denisovans – a humanoid that Max Planck researchers identified two years ago solely through their genetic material. Scientists at the Max Planck Institute for Evolutionary Anthropology ...
printer-friendly version of benchmark
printer-friendly version of benchmark

... would travel 9.46 x 1012 km in a year (thus, this value equals the distance known as a light year). To determine, for comparative purposes, how many light years the Sun is from Earth, divide the distance between the two (149,600,000 km) by 9.46 x 1012 km per light year. This calculation shows the Su ...
An introduction to the HR diagram File
An introduction to the HR diagram File

... • At the bottom right the stars are cool. These low mass stars are very long lived as they use their fuel so slowly. Very low mass M stars live many billions of years and will simply run out of fuel without dramatic events. ...
Physical structure of the local interstellar medium
Physical structure of the local interstellar medium

... The physical structure and morphology of the interstellar medium that surrounds our solar system directly effects the heliosphere and the interplanetary environment. High resolution ultraviolet absorption spectra of nearby stars and the intervening interstellar medium, observed by the Hubble Space Te ...
Star Show FACILITATOR NOTES
Star Show FACILITATOR NOTES

... The “Key Astronomical Facts to Consider” in the Participant are intended as a summary or reference guide, not as original teaching material. If these ideas are new to your students, you will need to invest more time discussing each of the sections in detail. Point out that stars really do come in di ...
TWINKLE – A Low Earth Orbit Visible and Infrared Exoplanet
TWINKLE – A Low Earth Orbit Visible and Infrared Exoplanet

... Twinkle is a space mission designed for visible and near-IR spectroscopic observations of extrasolar planets. Twinkle’s highly stable instrument will allow the photometric and spectroscopic observation of a wide range of planetary classes around different types of stars, with a focus on bright sourc ...
Hubble Error: Time, Money and Millionths of an inch
Hubble Error: Time, Money and Millionths of an inch

... brought in a cot and set it up in a trailer in the parking lot. Opticians traditionally did their work with a kind of black magic, even rubbing their thumbs along a lens or minor to apply the finishing touch. But unlike other Old World opticians in the industry, Geissler fully embraced the idea that ...
Spectra - Auburn University
Spectra - Auburn University

... Attached is a graph of the spectrum of the Sun obtained by our advanced lab electronic spectrometer. Several absorption lines have been marked. Identify the chemicals producing these lines using the wavelengths from the graph and hints below. Put the element producing the lines in the blanks. These ...
Problem Set 2 Solutions Problem 1: A
Problem Set 2 Solutions Problem 1: A

... Absorption: A (relatively) cool transparent gas in front of a source of a continuous spectrum will produce an absorption line spectrum. From this we see that whether we see an emission or absorption depends on temperature, as well as the transparency of a gas. The transparency of a gas is related to ...
The resolved stellar populations of M32 Monachesi, Antonela
The resolved stellar populations of M32 Monachesi, Antonela

... center. We find that this CMD has a wealth of features that reveal the different stellar populations present in M32. With the aid of evolutionary models of stars at a fixed age and chemical composition for different ranges of masses, we can qualitatively analyze the CMD. We find from this analysis t ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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