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DIO 15 - DIO, The International Journal of Scientific History
DIO 15 - DIO, The International Journal of Scientific History

... the same descriptions that we find in Aratus, plus some additional material – principally lists of constellations on the colures and arctic circles – that we know only through Hipparchus.2 We therefore know that Eudoxus had a fully developed conception of the celestial sphere. He understood the impo ...
Pulsating Variable Stars and The Hertzsprung - Chandra X
Pulsating Variable Stars and The Hertzsprung - Chandra X

... the absolute magnitude (MV) – intrinsic brightness – of stars is plotted against their temperature (stellar classification) the stars are not randomly distributed on the graph but are mostly restricted to a few well-defined regions. The stars within the same regions share a common set of characteris ...
DIO vol. 15 - DIO, The International Journal of Scientific History
DIO vol. 15 - DIO, The International Journal of Scientific History

... these successes, I started a full-scale survey of the ecliptic region in 1977. This promptly led to my discovery of the object Chiron in November of that year. In the back of my mind during this survey, was the possibility of discovering a new planet. The only evidence that such a planet might exist ...
Homologous Stellar Models and Polytropes Main Sequence Stars
Homologous Stellar Models and Polytropes Main Sequence Stars

... must still be on the Main Sequence, even if they are as old as the Universe. • Low-Mass Stars (0.7 6 M 6 2M ) in most cases end up losing most of their mass to become planetary nebulae before evolving on to the white dwarf cooling track. • Intermediate-Mass Stars (2 6 M 6 8M ) have evolution tracks ...
Outer Space 2 - World of Teaching
Outer Space 2 - World of Teaching

... Green = hydrogen Blue = oxygen Red = nitrogen ...
View the sky`s greatest nebula
View the sky`s greatest nebula

... M42. This section features a hot, bright star (center) that is ionizing the gas near it. This creates a sphere of glowing hydrogen, which appears pink. This image was shot through a 20-inch RC Optical Systems RitcheyChrétien telescope at ...
Purpose The student will explore parallax, a primary distance
Purpose The student will explore parallax, a primary distance

... pencil stops moving relative to even more distant objects? b. What can you determine about the usefulness of parallax at different distances? 4. To measure a parallax, you use a baseline: the distance between observation points. In the exercise above, the "baseline" is equal to the distance between ...
astronomy of the korku tribe of india
astronomy of the korku tribe of india

The Astrobiology Primer - Mary Ann Liebert, Inc. publishers
The Astrobiology Primer - Mary Ann Liebert, Inc. publishers

... The Astrobiology Primer has been created as a reference tool for those who are interested in the interdisciplinary field of astrobiology. The field incorporates many diverse research endeavors, but it is our hope that this slim volume will present the reader with all he or she needs to know to becom ...
Abstracts - Physics of Evolved Stars 2015
Abstracts - Physics of Evolved Stars 2015

... OH/IR stars are believed to be the final stage on the asymptotic giant branch (AGB) of intermediate main-sequence mass (5-8 solar masses) stars before they evolve into the post-AGB and planetary-nebula stages. AGB stars lose most of their stellar envelope in the form of a gaseous and dusty stellar w ...
Option D – Astrophysics
Option D – Astrophysics

... a star and it is very similar to billions of other stars in the universe. It has many objects orbiting around it that are held in their orbits by gravity. The solar system is an example of a planetary system. Most of the planets have one or more objects orbiting around them. These are called moons. ...
December - Rose City Astronomers
December - Rose City Astronomers

... 205, a quasar near the galaxy NGC 4319. The Seven Dwarfs were a collection of nearby dwarf galaxies, but this article will focus on Markarian 205, which at the time I observed it was a fascinating and highly enjoyable object. It’s become even more compelling as I learned about its physical character ...
The Physics and Chemistry of Nebular Evolution
The Physics and Chemistry of Nebular Evolution

Celestial Navitation - National University of Singapore
Celestial Navitation - National University of Singapore

... celestial navigation was created, sailors navigated by deduced (dead) reckoning. This method was used by Columbus in his voyages and most other sailors of his era. Dead reckoning enables a navigator to plot the location of the ship at any given time. As a result, the journey is already planned out e ...
Close Double Stars from Video
Close Double Stars from Video

... - Total occultations, both current and from published obs. - Spectroscopic binaries (including 1-line) were included to encourage observation of their occultations. • Too many dubious events were included; especially visual observers often reported “gradual” events more likely due to Fresnel diffrac ...
8 Comets: Potential Sources of Prebiotic Molecules for the
8 Comets: Potential Sources of Prebiotic Molecules for the

Hariprasad comes from well known Jyotish family in Andhrapradesh
Hariprasad comes from well known Jyotish family in Andhrapradesh

... Proceedings of 2nd Karnataka Astronomical Conference, Mysore - 1934 Vedanga Jyotisha, whose author is unknown, was transmitted for the benefit of mankind through Lagadha Mahamuni. (There is a view that it was authored by Lagadha Mahamuni. But upon close reading “Lagadhasya Mahatmanah” does not give ...
Examining the M67 Classification as an Open Cluster
Examining the M67 Classification as an Open Cluster

Eye in the sky - Academy of Science of South Africa
Eye in the sky - Academy of Science of South Africa

Metallicity, Age, and Mass of Star Forming Galaxies at z~3
Metallicity, Age, and Mass of Star Forming Galaxies at z~3

... If the star (or stellar population) is sufficiently young and massive to produce ionizing photons, a common method is to measure the deviation of hydrogen recombination line ratios from theoretical expectations. These have well established values, that vary typically less than 10%-15% for a large ra ...
How astero-seismology can help to infer properties of - IAG-Usp
How astero-seismology can help to infer properties of - IAG-Usp

... * surface Prot or a relation between Prot and stellar parameters * Seismic model : (is wanted by itself and wanted for rotation determination) better use slow rotators if possible otherwise must remove pollution by rotation ...
Facilitator`s Guide
Facilitator`s Guide

... the only measurements that can be made, involve the detection of the energy they emit (typically the visible light energy) to determine: position, movement in time, brightness and color. The initial “rung” on the distance ladder (parallax) involves measuring the position of a star from two different ...
FILE
FILE

... In the SNAPP model, the volume each SN would process times the number of SNe occurring in the lifetime of a “giant molecular cloud”, in which complex molecules are thought to be made, is <<< the size of the cloud. But once created, the molecules will replicate, possibly on warmed (more than 20 K) du ...
Pluto Challenge - Cedar Amateur Astronomers
Pluto Challenge - Cedar Amateur Astronomers

... of a Plutonian day to be 6.4 Earth days. Pluto’s orbit around the sun takes 248.5 Earth years. These days Pluto traverses an area of the night sky that it hasn’t visited since 20 years prior to signing of the United States Declaration of Independence! NASA has plans to send a science mission to Plut ...
Project 1. CCD image analysis
Project 1. CCD image analysis

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Theoretical astronomy

Theoretical astronomy is the use of the analytical models of physics and chemistry to describe astronomical objects and astronomical phenomena.Ptolemy's Almagest, although a brilliant treatise on theoretical astronomy combined with a practical handbook for computation, nevertheless includes many compromises to reconcile discordant observations. Theoretical astronomy is usually assumed to have begun with Johannes Kepler (1571–1630), and Kepler's laws. It is co-equal with observation. The general history of astronomy deals with the history of the descriptive and theoretical astronomy of the Solar System, from the late sixteenth century to the end of the nineteenth century. The major categories of works on the history of modern astronomy include general histories, national and institutional histories, instrumentation, descriptive astronomy, theoretical astronomy, positional astronomy, and astrophysics. Astronomy was early to adopt computational techniques to model stellar and galactic formation and celestial mechanics. From the point of view of theoretical astronomy, not only must the mathematical expression be reasonably accurate but it should preferably exist in a form which is amenable to further mathematical analysis when used in specific problems. Most of theoretical astronomy uses Newtonian theory of gravitation, considering that the effects of general relativity are weak for most celestial objects. The obvious fact is that theoretical astronomy cannot (and does not try) to predict the position, size and temperature of every star in the heavens. Theoretical astronomy by and large has concentrated upon analyzing the apparently complex but periodic motions of celestial objects.
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