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CONSTELLATIONS OF THE SOUTHERN SKY VOLANS
CONSTELLATIONS OF THE SOUTHERN SKY VOLANS

... Created by Bayer in 1603, this constellation used to be called PiscisVolans, the Flying Fish, before it was shortened to Volans. Volans was one of the 12 new constellations introduced at the end of the 16th century by the Dutch navigators Pieter Dirkszoon Keyser and Frederick de Houtman. Volans repr ...
STELLAR STRUCTURE AND EVOLUTION
STELLAR STRUCTURE AND EVOLUTION

... stellar surface, Rs the stellar radius. Energy may also be lost in the form of neutrinos or by direct mass loss (generally unobservable). Astronomers measure: f = (Rs/D)2 F ...
Word version of Episode 704
Word version of Episode 704

... External reference This activity is taken from Advancing Physics, chapter 12, 160O ...
Agenda - Relativity Group
Agenda - Relativity Group

... • As a high-mass star ages, carbon and heavier elements can fuse via helium capture and other processes to form ever heavier elements. Shells of increasingly heavy element fusion are created, like onion skins inside the star. However, since fusion of iron uses up energy instead of releasing energy, ...
Characteristics of Our Galaxy
Characteristics of Our Galaxy

... of gas, which in turn accumulated under mutual gravitational attraction to form many different galaxies as opposed to just one humongous structure. Some new galaxies form today out of collisions and interactions between existing galaxies.3 Our home, the planet Earth, orbits the Sun along with Mercu ...
Stars and Galaxies
Stars and Galaxies

...  Sine of the parallax (angle) x Earth’s distance to the Sun = Distance to the star  The angles involved for strellar observations are very small and difficult to measure. Proxima Centauri, has a parallax of 0.77 arcsec. This angle is approximately the angle subtended by an object about 2 centimete ...
NATS1311_082108_bw - The University of Texas at Dallas
NATS1311_082108_bw - The University of Texas at Dallas

... 2. Measurement and Prediction - Explore the necessity for accurate and reliable data from measurements in order to make predictions. Measure the density of several objects. 3. Conservation of Energy/Momentum - Study laws of conservation of momentum and energy. Determine speed of a ball by 2 differen ...
Enhanced lithium depletion in Sun-like stars with orbiting planets.
Enhanced lithium depletion in Sun-like stars with orbiting planets.

... from either the accretion of planets/planetesimals on to the star or the protostellar molecular cloud. This metallicity excess is also present in the solar analogue planet-bearing stars (see Fig. 2c). Can high metallicity be responsible for enhanced Li depletion in these stars? The increase of metal ...
AST 341 - Homework I - Solutions
AST 341 - Homework I - Solutions

Unit 5 – Creating and Understanding Spectra
Unit 5 – Creating and Understanding Spectra

... familiar objects in alternative ways. It is because certain objects can be detected and studied only at these other wavelengths. ...
Fomalhaut b
Fomalhaut b

... •  1984
:

IRAS
mission
finds
dust
grains
orbi)ng

Fomalhaut,
as
 well
as
other
stars
such
as
Epsilon
Eridani,
Vega,
and
Beta
 Pictoris
 •  Resolved
thermal
emission
shows
a
central
hole
(Holland
et
al.
1998)
 •  Fomalhaut
is
nearby
(7.7
pc).

High
proper
mo)on
(0.4”/yr).
 •  Fomalhaut
is
a
young,
ma ...
Measuring the mass of galaxies Luminous matter in a
Measuring the mass of galaxies Luminous matter in a

Powerpoint of lecture 14
Powerpoint of lecture 14

... Summary of basic picture ...
Physics 1114OL - Normandale Community College
Physics 1114OL - Normandale Community College

... Policy on Incompletes: Generally we assign an “I” grade when a student has extenuating circumstances that cause him or her to miss significant portions of a course. The “I” is an alternative to a “W” when the student has demonstrated a mastery of the material and only will miss a part of the course. ...


... Meteorites contain clear evidence that isotopes with short half lives (as short as 100,000 years) were present in the cloud of gas and dust (the called solar nebula) from which the Sun and planets formed. Supernovae, the powerful explosions of spent stars, produce elements, including short-lived rad ...
The Time of Perihelion Passage and the Longitude of Perihelion of
The Time of Perihelion Passage and the Longitude of Perihelion of

... perturbed the orbits of the planets substantially, especially near times of perihelion passage. Yet almost no such perturbations have been detected. This can be explained if Nemesis is comprised of two stars with complementary orbits such that their perturbing accelerations tend to cancel at the Sun ...
Solar Spectrum Birth of Spectroscopy Kirchhoff`s Laws Types of
Solar Spectrum Birth of Spectroscopy Kirchhoff`s Laws Types of

The loss of nitrogen-rich atmospheres from Earth-like
The loss of nitrogen-rich atmospheres from Earth-like

... gaseous envelope even if the planet orbits its parent M star within the habitable zone (HZ). However, as shown in Lammer et al. (2007), a high CO2 atmospheric mixing ratio will result in enhanced IR cooling in the thermosphere and inhibits its expansion and therefore leads to reduced non-thermal atm ...
Ch24-1 Powerpoint
Ch24-1 Powerpoint

... light is a basic tool to any modern astronomer. The main source of light in our solar system is our sun. This lesson will focus on the sun and the nature of light that comes from the sun; it’s form and function within our solar system. ...
Potential Meteorite Impact - Albert
Potential Meteorite Impact - Albert

... Shooting stars" or meteors are bits of material falling through Earth's atmosphere; they are heated to incandescence by the friction of the air. The bright trails that are coming through the Earth's atmosphere are termed meteors, and these chunks that are hurtling through space are called meteoroids ...
Earth Science 24.1 The Sun: Study of Light
Earth Science 24.1 The Sun: Study of Light

... light is a basic tool to any modern astronomer. The main source of light in our solar system is our sun. This lesson will focus on the sun and the nature of light that comes from the sun; it’s form and function within our solar system. ...
Potential meteorite impact - Albert
Potential meteorite impact - Albert

... are heated to incandescence by the friction of the air. The bright trails that are coming through the Earth's atmosphere are termed meteors, and these chunks that are hurtling through space are called meteoroids. Large pieces that do not vaporize completely and reach the surface of the Earth are ter ...
53.3 A New View of Gravity • What is gravity?
53.3 A New View of Gravity • What is gravity?

... "orbits" around the center of the bowl, while marbles rolled from farther away or at higher speeds could loop around the center on unbound parabolic or hyperbolic paths. By analogy, general relativity tells us that, depending on their speed and direction, planets or other objects moving freely in sp ...
Altitude and Azimuth 4 page
Altitude and Azimuth 4 page

... needs a coordinate system to find objects on the Earth. Navigators and geographers use latitude and longitude to find their way around on the surface of the Earth. Astronomers, though, have one problem that Earth-oriented people don't have. Objects in the sky appear to move over time with respect to ...
PSCI1030-CHAP016-The Solar System
PSCI1030-CHAP016-The Solar System

... • Mercury has the shortest period of revolution (88 days), and is the fastest moving • Mercury was named by the early Greeks after the swift messenger of the gods • Temperatures on Mercury range from about 473oC on the side facing the sun to about 173oC on the dark side • Due to its small size and c ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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