• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Stars - Lauer Science
Stars - Lauer Science

... Hydrogen and some helium was made at the beginning of the Universe (Big Bang). • All other elements were made inside of stars, and then spewed out into space by the supernova ...
Cepheid Calibration
Cepheid Calibration

... The apparent brightness of a light source varies inversely as the square of its distance. In other words, if the distance between an observer and a light source is doubled, the light source will appear four times as faint to the observer. Astronomers can use this inverse square law to estimate dist ...
Lecture 1 – Astronomy
Lecture 1 – Astronomy

... Gemini Observatory/P. Michaud. ...
Untitled - Kapteyn Astronomical Institute
Untitled - Kapteyn Astronomical Institute

... is much colder than the star which it orbits. This means that a planet emits a different colour of light than that star. By looking only to the far infrared light, and not to the visible light, it is possible to see planets orbiting around a star. Unfortunately our telescopes are not good enough yet ...
Word Solar System Definition
Word Solar System Definition

... The star in our solar system that sustains most life on Earth and is the primary source of heat and light. Definition An instrument that gathers light and magnifies, or makes distant objects appear larger. ...
The Mass Assembly of Galaxies
The Mass Assembly of Galaxies

... There is a cluster of B stars in the central 1’’ of the galaxy, the so-called S-cluster. These high proper motion stars - in particular star S2 - show that Sgr A* is a black-hole of 3-4 million solar masses. Large numbers of young stars, in particular O supergiants and WR stars are observed within 2 ...
Lenses - singhscience
Lenses - singhscience

... creates a real image within a telescope of a distant object. Eyepiece lens – magnifies the image of a distant object. ...
MSci Astrophysics 210PHY412 - Queen's University Belfast
MSci Astrophysics 210PHY412 - Queen's University Belfast

... we can measure – age (t) and chemical composition Composition parameterised with X,Y,Z  mass fraction of H, He and all other elements e.g. X = 0.747 ; Y = 0.236 ; Z = 0.017 Note – Z often referred to as metallicity Would like to study stars of same age and chemical composition – to keep these pa ...
Lecture 2 - The University Centre in Svalbard
Lecture 2 - The University Centre in Svalbard

... Gemini Observatory/P. Michaud. ...
• Cassini set out to measure the distance of the Solar system. Recall
• Cassini set out to measure the distance of the Solar system. Recall

... Stellar Parallax ...
Star Types
Star Types

... sun, an O star, a white dwarf, or a red giant? Which of these star is the hottest? What are Sun-like stars (0.4 Msun < M < 8 Msun) in common? What about red dwarfs (0.08 Msun < M < 0.4 Msun) ? Where do stars spend most of their time? ...
Linking Asteroids and Meteorites through Reflectance Spectroscopy
Linking Asteroids and Meteorites through Reflectance Spectroscopy

... Sun out to the Sun’s orbit • Mass-to-Light ratio of our Sun is 1 solar mass per solar luminosity • So most matter is dimmer than the Sun ...
Word - Wichita State University
Word - Wichita State University

... the Milky Way. The theme for this program is the different kinds of objects which are found within our galaxy. During the program everyone has a chance to look through the telescope at a planet, star cluster, and cloud of gas. The program concludes with a view of a spiral galaxy. As people view thes ...
The Comet Cometh
The Comet Cometh

... big and massive are they? How can a canny comet like Kohoutek taunt observers into announcing that it will soon shine spectacularly then whimsically dim its light? These and other questions have baffled astronomers for generations; here was the chance to seek some conclusive answers. Whipple's (1949 ...
pluto
pluto

... Nasa probe visits in 2015 Its orbit around the Sun is also highly tilted compared with the plane of the big planets. In addition, since the early 1990s, astronomers have found several objects of comparable size to Pluto in an outer region of the Solar System called the Kuiper Belt. Some astronomers ...
JFuller Science In A Bag Revised
JFuller Science In A Bag Revised

... The earth is the largest object in the solar system. The solar system is very crowded. The solar system contains only the sun, planets and the moon. Meteors are falling stars. Comets and meteors are out in space and do not reach the ground. The surface of the sun is without visible features. All the ...
Physical Characterization Studies of Near
Physical Characterization Studies of Near

... spacecraft missions require moderate to large-sized telescopes. Good candidate asteroids must have a welldefined orbit and be of a known composition. Knowledge of physical properties such as size, shape, internal structure, rotation rate (and whether the asteroid is tumbling) must also be derived. A ...
Document
Document

... Neutrons (and protons) are made of quarks. Gravity could crush neutrons into free quarks. Called strange matter (a type of quark). Astronomers think they may have seen a quark star. ...
Basic Astronomy Note - Mr. Dewey – Grade 7/8
Basic Astronomy Note - Mr. Dewey – Grade 7/8

... Our sun is one star of billions that make up our galaxy (Milky Way). It is 100,000 light years in diameter, which means it would take 100,000 years to travel from edge to edge at the incredible speed of light (roughly 300,000 kilometers per second). The Milky Way, that bright band of light in the ni ...
Early Astronomies
Early Astronomies

... Aristotle Adopted physical laws and showed in terms of these why the universe functioned the way it did. Circular motion - the only natural motion. Earth not spinning since no great wind - so Earth is stationary. All circular motions centered about the Earth. Four basic elements: earth, air, fire, a ...
Science Exemplary Text
Science Exemplary Text

08 September: How far away are the closest stars?
08 September: How far away are the closest stars?

... enormous • If the distance between the Earth and Sun were shrunk to 1 cm (0.4 inches), Alpha Centauri would be 2.75 km (1.7 miles) away ...
DUPREE_SPLINTER
DUPREE_SPLINTER

... Candidates for second parameter: age, environment (including free-floating planets); primordial He abundance; surface pollution (helium); CNO abundances; rotation; mass loss….. ...
Lecture notes -- pdf file - University of Iowa Astrophysics
Lecture notes -- pdf file - University of Iowa Astrophysics

... So what are the distances to the stars? • First measurements made in 1838 (Friedrich Bessel) • Closest star is Alpha Centauri, p=0.75 arcseconds, d=1.33 parsecs= 4.35 light years • Nearest stars are a few to many parsecs, 5 - 20 light years ...
Basic Observations in Astronomy
Basic Observations in Astronomy

... They move from East to West and also from near to the horizon to higher up in the sky ...
< 1 ... 260 261 262 263 264 265 266 267 268 ... 456 >

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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report