
Unit 5: Space Exploration Topic 1: Our Eyes Only • Define FRAME
... Massive star: Stellar Nebula àMassive Star à Red Supergiant à Supernovaàif the star is not destroyed entirely the core is left as a Neutron Star or Black Hole • Distribution of matter in space. We live on the planet Earth which has a moon that orbits us. We orbit the sun (a star, and one of many ...
... Massive star: Stellar Nebula àMassive Star à Red Supergiant à Supernovaàif the star is not destroyed entirely the core is left as a Neutron Star or Black Hole • Distribution of matter in space. We live on the planet Earth which has a moon that orbits us. We orbit the sun (a star, and one of many ...
ASTR100 Class 01 - University of Maryland Department of
... C. The temperature starts low and ends high in both the raisin cake and the universe. D. The raisins stay roughly the same size as the cake expands, just as galaxies stay roughly the same size as the universe expands. E. The average distance increases with time both between raisins in the cake and b ...
... C. The temperature starts low and ends high in both the raisin cake and the universe. D. The raisins stay roughly the same size as the cake expands, just as galaxies stay roughly the same size as the universe expands. E. The average distance increases with time both between raisins in the cake and b ...
Pertti Mäkelä The Catholic University of America
... latitudes (CRs are charged particles). • 1930 Carl Størmer (Stoermer) calculated particle trajectories in the geomagnetic field -> latitudinal effect was due to shielding by the geomagnetic field. • 1936 Georg Pfotzer discovered a maximum in CR intensity at an altitude of about 15 km due to the inte ...
... latitudes (CRs are charged particles). • 1930 Carl Størmer (Stoermer) calculated particle trajectories in the geomagnetic field -> latitudinal effect was due to shielding by the geomagnetic field. • 1936 Georg Pfotzer discovered a maximum in CR intensity at an altitude of about 15 km due to the inte ...
Chapter 4: The Solar System
... to their present form from a gas and dust cloud. B. the solar system was once a galaxy, from which the sun and planets are remnants, after evolution. C. the sun captured the planets as they drifted through space. D. planets were spun out of the sun as smaller gas clouds and subsequently condensed. ...
... to their present form from a gas and dust cloud. B. the solar system was once a galaxy, from which the sun and planets are remnants, after evolution. C. the sun captured the planets as they drifted through space. D. planets were spun out of the sun as smaller gas clouds and subsequently condensed. ...
The sun - Salwan Education Trust
... All of us have been troubled by the glare and heat of the Sun on a hot summer day. Stop! Where does the glow come from? Until the nineteenth century it was generally accepted that the process by which the Sun gave heat and light was very similar to the burning of logs to create a fire. But there was ...
... All of us have been troubled by the glare and heat of the Sun on a hot summer day. Stop! Where does the glow come from? Until the nineteenth century it was generally accepted that the process by which the Sun gave heat and light was very similar to the burning of logs to create a fire. But there was ...
The Interstellar Medium
... A World of Interstellar Medium The space between the stars is not completely empty, but filled with very dilute gas and dust, producing some of the most beautiful objects in the sky. We are interested in the interstellar ...
... A World of Interstellar Medium The space between the stars is not completely empty, but filled with very dilute gas and dust, producing some of the most beautiful objects in the sky. We are interested in the interstellar ...
PPT file
... in PRAO. It’s the most long set observations. 125 sources are in the modern list for observation once in the month. Here two type sources: super compact (~1au) gaze clouds in star formation regions and envelopes of variable late spectra classes stars. In star formation regions was found periodicity ...
... in PRAO. It’s the most long set observations. 125 sources are in the modern list for observation once in the month. Here two type sources: super compact (~1au) gaze clouds in star formation regions and envelopes of variable late spectra classes stars. In star formation regions was found periodicity ...
Hubblecast Episode 68: The Hubble time machine Visual notes 00
... edges, still in the middle of evolving into fully-grown galaxies. ...
... edges, still in the middle of evolving into fully-grown galaxies. ...
The Interstellar Medium
... A World of Interstellar Medium The space between the stars is not completely empty, but filled with very dilute gas and dust, producing some of the most beautiful objects in the sky. We are interested in the interstellar ...
... A World of Interstellar Medium The space between the stars is not completely empty, but filled with very dilute gas and dust, producing some of the most beautiful objects in the sky. We are interested in the interstellar ...
Measuring the Masses of Galaxies in the Sloan Digital Sky Survey
... the redshift is measured from the observed positions of atomic lines in the spectra of galaxies and quasars for example, the red line of hydrogen (Hα) has a wavelength of 6.563 × 10-5 cm, 6563 Ångstroms, 656.3 nm suppose it were observed at 6603 Ångstroms (1 + z) = 6603 / 6563 = 1.0061 all other li ...
... the redshift is measured from the observed positions of atomic lines in the spectra of galaxies and quasars for example, the red line of hydrogen (Hα) has a wavelength of 6.563 × 10-5 cm, 6563 Ångstroms, 656.3 nm suppose it were observed at 6603 Ångstroms (1 + z) = 6603 / 6563 = 1.0061 all other li ...
R. Bender (ESO)
... assembly of galaxies and dust-enshrouded violent star formation processes that may have produced a large fraction of all stars in the universe, especially those in spheroids. ALMA will allow to probe the collapse of the first massive galaxy fragments before they have largely turned into stars. A ...
... assembly of galaxies and dust-enshrouded violent star formation processes that may have produced a large fraction of all stars in the universe, especially those in spheroids. ALMA will allow to probe the collapse of the first massive galaxy fragments before they have largely turned into stars. A ...
Astronomy 10B List of Concepts– by Chapter
... • Definitions (Cosmological principle, isotropic) • Giant elliptical galaxies and clusters • Distributions of galaxies, groups and clusters in space • Galactic evolution & collisions • How has star formation changed compared with 8 Byrs ago? ...
... • Definitions (Cosmological principle, isotropic) • Giant elliptical galaxies and clusters • Distributions of galaxies, groups and clusters in space • Galactic evolution & collisions • How has star formation changed compared with 8 Byrs ago? ...
Dec 2013 - Bays Mountain Park
... temperature of 110 Kelvin (-163 °C / -261 °F), Io is home to the most extreme temperature differences from locationto-location outside of the Sun. Just by orbiting where it does, Io gets distorted, heats up, and erupts, making it the most volcanically active world in the entire Solar System! Other mo ...
... temperature of 110 Kelvin (-163 °C / -261 °F), Io is home to the most extreme temperature differences from locationto-location outside of the Sun. Just by orbiting where it does, Io gets distorted, heats up, and erupts, making it the most volcanically active world in the entire Solar System! Other mo ...
Dark Matter - the stuff of the Universe?
... look for neutrino oscillations—change of neutrino type (depends on difference between masses of the two types) these do happen but the implied mass is very small indeed ...
... look for neutrino oscillations—change of neutrino type (depends on difference between masses of the two types) these do happen but the implied mass is very small indeed ...
Year 9 space ppt
... pressure. The hydrogen atoms are broken into pieces, which smash into each other at high speed. This can make the pieces of hydrogen atoms join together to become helium. This also produces gamma radiation, which travels outward and heat and light is radiated into space in all directions. ...
... pressure. The hydrogen atoms are broken into pieces, which smash into each other at high speed. This can make the pieces of hydrogen atoms join together to become helium. This also produces gamma radiation, which travels outward and heat and light is radiated into space in all directions. ...
Astronomy 350 Fall 2011 Homework #1
... Now consider a objects which have part of their orbit inside 1 AU and part outside of 1 AU. Can any such object have a period > 1 year? If so, give an example of such an orbit. If not, explain why not. Same thing for a period < 1 yr. The most massive solar system object beyond Neptune is not Pluto, ...
... Now consider a objects which have part of their orbit inside 1 AU and part outside of 1 AU. Can any such object have a period > 1 year? If so, give an example of such an orbit. If not, explain why not. Same thing for a period < 1 yr. The most massive solar system object beyond Neptune is not Pluto, ...
Teacher`s Guide - Discovery Education
... How to Use the DVD The DVD starting screen has the following options: Play Video—This plays the video from start to finish. There are no programmed stops, except by using a remote control. With a computer, depending on the particular software player, a pause button is included with the other video c ...
... How to Use the DVD The DVD starting screen has the following options: Play Video—This plays the video from start to finish. There are no programmed stops, except by using a remote control. With a computer, depending on the particular software player, a pause button is included with the other video c ...
30galaxies and the universe
... Black holes in the centers of giant galaxies—some more than one billion solar masses—had enough infalling gas to once blaze as quasars. The final mass of a black hole is not primordial, but instead is determined during the galaxy formation process. This shows that there is a close relationship betwe ...
... Black holes in the centers of giant galaxies—some more than one billion solar masses—had enough infalling gas to once blaze as quasars. The final mass of a black hole is not primordial, but instead is determined during the galaxy formation process. This shows that there is a close relationship betwe ...
Astronomy Questions
... Is there such a thing as antimatter in space? Are there such things as falling stars? What happens to something once it enters a black hole? What’s the total mass of everything in the universe? How did ancient cultures view the solar system? Are there more than four dimensions? What’s the deal with ...
... Is there such a thing as antimatter in space? Are there such things as falling stars? What happens to something once it enters a black hole? What’s the total mass of everything in the universe? How did ancient cultures view the solar system? Are there more than four dimensions? What’s the deal with ...
PPT File - Brandywine School District
... The Kuiper Belt is made up of millions of icy and rocky objects that orbit our Sun beyond the orbits of Neptune and Pluto. It's hard to say exactly what's going on in the Kuiper Belt. Even the biggest of the Kuiper Belt Objects is smaller than the United States and it is billions of miles away where ...
... The Kuiper Belt is made up of millions of icy and rocky objects that orbit our Sun beyond the orbits of Neptune and Pluto. It's hard to say exactly what's going on in the Kuiper Belt. Even the biggest of the Kuiper Belt Objects is smaller than the United States and it is billions of miles away where ...
Stars and the Sun
... • Brief periods don’t cause damage – more likely to for young people or at high elevation • UV Exposure believed to contribute to Cataracts (not from looking directly at sun) • Looking thru binoculars can damage eyes (concentrated) • Looking at Partial eclipses without filters is dangerous – the eye ...
... • Brief periods don’t cause damage – more likely to for young people or at high elevation • UV Exposure believed to contribute to Cataracts (not from looking directly at sun) • Looking thru binoculars can damage eyes (concentrated) • Looking at Partial eclipses without filters is dangerous – the eye ...
SolarSystem Powerpoint lesson
... The Kuiper Belt is made up of millions of icy and rocky objects that orbit our Sun beyond the orbits of Neptune and Pluto. It's hard to say exactly what's going on in the Kuiper Belt. Even the biggest of the Kuiper Belt Objects is smaller than the United States and it is billions of miles away where ...
... The Kuiper Belt is made up of millions of icy and rocky objects that orbit our Sun beyond the orbits of Neptune and Pluto. It's hard to say exactly what's going on in the Kuiper Belt. Even the biggest of the Kuiper Belt Objects is smaller than the United States and it is billions of miles away where ...
JSchreiberTalk3 - FSU High Energy Physics
... Background info (formation/evolution of galaxies) Implications of theories ...
... Background info (formation/evolution of galaxies) Implications of theories ...
Kepler-Laws-SatelliteMotion
... line using a spreadsheet––Kepler spent 10 years! The significance of a linear graph is whatever you’re graphing along the vertical axis is proportional to whatever you’re graphing along the horizontal axis. Since the graph of r 3 vs. T 2 is a straight line, r 3 ~ T 2, ...
... line using a spreadsheet––Kepler spent 10 years! The significance of a linear graph is whatever you’re graphing along the vertical axis is proportional to whatever you’re graphing along the horizontal axis. Since the graph of r 3 vs. T 2 is a straight line, r 3 ~ T 2, ...
Outer space
Outer space, or just space, is the void that exists between celestial bodies, including the Earth. It is not completely empty, but consists of a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium as well as electromagnetic radiation, magnetic fields, neutrinos, dust and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvin (K). Plasma with a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvin in the space between galaxies accounts for most of the baryonic (ordinary) matter in outer space; local concentrations have condensed into stars and galaxies. In most galaxies, observations provide evidence that 90% of the mass is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Data indicates that the majority of the mass-energy in the observable Universe is a poorly understood vacuum energy of space which astronomers label dark energy. Intergalactic space takes up most of the volume of the Universe, but even galaxies and star systems consist almost entirely of empty space.There is no firm boundary where space begins. However the Kármán line, at an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which was passed by the United Nations in 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights, followed by manned rocket launches. Earth orbit was first achieved by Yuri Gagarin of the Soviet Union in 1961 and unmanned spacecraft have since reached all of the known planets in the Solar System. Due to the high cost of getting into space, manned spaceflight has been limited to low Earth orbit and the Moon.Outer space represents a challenging environment for human exploration because of the dual hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is high.