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Stellar evolution
Stellar evolution

... - First occurs in a runaway process: "the helium flash". Energy from fusion goes into re-expanding and cooling the core. This slows fusion, so star gets dimmer again. - Then stable He -> C burning. Still have H -> He shell burning surrounding it. ...
Use Example problem 8-2 to solve practice
Use Example problem 8-2 to solve practice

... on March 16, 2880, but the torino scale only works for impact possibilities within 100 years, and thus cannot apply to this asteroid. Objects with diameters smaller than 10 m (33 ft) are called meteoroids (or meteorites if they strike the ground). An estimated 500 meteorites reach the surface each y ...
July 2008 - Warren Astronomical Society
July 2008 - Warren Astronomical Society

Moons of the planets
Moons of the planets

... Saturn was 19 arcseconds (remember what an arcsecond is). At that time, the angular diameter of the moon Titan (the star off to the left that night) was 0.84 arcseconds, smaller than the “seeing disk” due to the Earth’s atmosphere. ...
The Constellations
The Constellations

... Circle-upon-Circles Greek philosopher Claudius Ptolemy (A.D. 100-170) proposed a planet model in which the planets move around a small circle which in turns orbits the earth, pretty much like the moon is orbiting the Earth while the Earth is orbiting the Sun. This model can explain the retrograde mo ...
Magic
Magic

... Meridian. A circle of longitude passing from the South point of the horizon, through the zenith to the North point of the horizon. It coincides with geographical longitude - a great circle crossing the equator and passing through the poles. Every point on the Earth's surface has its own meridian or ...
ESCI 100 Exam 1 Review Name Explain inductive and deductive
ESCI 100 Exam 1 Review Name Explain inductive and deductive

... What is the modified Mercalli intensity scale (called Mercalli Intensity scale in lecture notes) based on? ...
Review Packet
Review Packet

... _____ The force of gravity pulls a nebula together forming clumps called protostars. _____ Hydrogen atoms are fused together generating an enormous amount of energy igniting the star causing it to shine. ...
Planetary Orbit Simulator – Student Guide
Planetary Orbit Simulator – Student Guide

A_Changing_Planet - Illinois State University
A_Changing_Planet - Illinois State University

... billion years ago. (The sub is at least a second generation star.)  Most of the cloud is Hydrogen and Helium formed just after the start of the Universe.  Heavier elements are the remnants of older star that have burned out and exploded. ...
PLANET VISIBILITY Appearance of the planets
PLANET VISIBILITY Appearance of the planets

... skies. Venus is readily identified by its brightness – being exceeded by only the Sun and Moon. Venus is often referred to as either the Evening Star (when visible in the west after sunset) or the Morning Star (in the east before sunrise). Mars is notable for its orange-red appearance and is popular ...
Lecture 11
Lecture 11

... – If we know how bright something is and how bright it appears, we can figure out how far away it is ...
Earth - Mrs. Christov`s Physical Geography Class
Earth - Mrs. Christov`s Physical Geography Class

... flattened, disk- shaped mass estimated to contain nearly 200 billion stars, dust, and gases. • Vast distances: - A light year= 6 trillion mi (the distance the light travels in 1 year) V of light= 186,000 mi/sec ...
Basic Information about the Solar System Handout
Basic Information about the Solar System Handout

... 510 planets orbiting other stars. This number is up from the milestone of 100 exoplanets discovered as of January 2004. Most known exoplanets are gas giants, Jupiter-like planets, since current methods favor the detection of the more massive worlds. Most are relatively nearby, within 5,000 light yea ...
Binary Stars (Professor Powerpoint)
Binary Stars (Professor Powerpoint)

... The primary importance of binaries is that they allow us to measure stellar parameters (especially mass). The center of mass is the location where a fulcrum would be placed to balance the stars on a seesaw. ...
Document
Document

... • In modern times, it was discovered that the human eye has a nonlinear response to light: if one source of light has twice the light as a second source, then the first source would not appear by eye to be twice as bright. • The response of the eye is logarithmic, so that differences of magnitudes c ...
Here
Here

... • In modern times, it was discovered that the human eye has a nonlinear response to light: if one source of light has twice the light as a second source, then the first source would not appear by eye to be twice as bright. • The response of the eye is logarithmic, so that differences of magnitudes c ...
Intelligent Life in the Milky Way Galaxy
Intelligent Life in the Milky Way Galaxy

... Individuals with traits that best allow them to survive and reproduce will on average produce the greatest number of surviving offspring. ...
Pluto Evidence
Pluto Evidence

The Life Cycle of a Star and the Hertzsprung
The Life Cycle of a Star and the Hertzsprung

... stars of different ages and in different stages, all at the same time. It is also a great tool to check your understanding of the star life cycle. In the Hertzsprung-Russell (HR) Diagram, each star is represented by a dot. There are lots of stars out there, so there are lots of dots. The position of ...
Astronomy 1400: Homework 5
Astronomy 1400: Homework 5

... able to resolve the solar granulation cells? Ignore possible atmospheric effects. In this price range, you should find telescopes about ∼ 2 – 10 in (∼ 60 – 300 mm). Refractors are definitely more expensive that reflectors of the same size because making a lens (that light has to travel through) is m ...
Planetary Configurations
Planetary Configurations

... • Mass can transfer from a normal star to a WD, resulting in an accretion disk. • This is a disk of gas orbiting the WD with gas slowly “seeping” inward to the WD. • NOVAE: Hydrogen gas accumulates and heats up until fusion switches on. Leads to an explosion and ejection of mass. Repeats. • SUPERNOV ...
Gravitational Force Problem Set
Gravitational Force Problem Set

... kg. In one of its orbits, the electron is 5.3 × 10-11 m from the proton. What is the mutual attractive force between the electron and proton? A) 1.8 × 10-47 N B) 3.6 × 10-47 N C) 5.4 × 10-47 N D) 7.0 × 10-47 N 11. The gravitational attractive force between two masses is F. If the masses are moved to ...
Patterns in the Sky - Plano Independent School District
Patterns in the Sky - Plano Independent School District

... stars that make up the pan or dipper and the 3 stars in the tail. You use the 2 stars on the end of the pan as the pointing stars to find Polaris the North Star in the tail of the Little Dipper. The 2 stars that are the pointers are Dubhe—the top star and Merak—the bottom star in the pan. The handle ...
Chapter 4 The Solar System
Chapter 4 The Solar System

... 4.1 An Inventory of the Solar System Early astronomers knew Moon, stars, Mercury, Venus, Mars, Jupiter, Saturn, comets, and meteors Now known: Solar system has 135 moons, one star, nine planets (added Uranus, Neptune, and Pluto), asteroids, comets, and meteoroids ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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