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black hole
black hole

...  The core of helium ash cannot generate nuclear energy.  Nevertheless, it can grow hotter—because it contracts and converts gravitational energy into thermal energy.  The rising temperature heats the unprocessed hydrogen just outside the core—hydrogen that was never previously hot enough to fuse. ...
Astrophysical explosions: from solar flares to cosmic gamma
Astrophysical explosions: from solar flares to cosmic gamma

PC3692: Physics of Stellar Structure (and Evolution)
PC3692: Physics of Stellar Structure (and Evolution)

... 2. Stars provide extreme conditions for studying physics. The high density, high temperature and high pressure are usually not found on Earth. White dwarfs, neutron stars are extremely dense and are a good testing ground for theories such as general relativity. 3. Stars are fascinating for yet anoth ...
Dust formation in the winds of AGBs: the contribution at low
Dust formation in the winds of AGBs: the contribution at low

... At lower stellar masses (<8 M ) grain condensation occurs during the AGB and super-AGB phases and the resulting dust mass depends on the progenitor stellar mass and metallicity through complex processes which affect the chemical composition and physical conditions in the stellar atmospheres. Previo ...
astronomy advisory panel strategy
astronomy advisory panel strategy

... Understanding the birth of stars is fundamental to astrophysics. Any realistic explanation of the formation and evolution of galaxies requires us to know what determines the rate of star formation, what determines any variation in the mass distribution of stars formed, and what determines the charac ...
Standard Four: Earth in Space
Standard Four: Earth in Space

... Essential Question: What predictable, observable patterns occur as a result of the interaction between the Earth, Moon, and Sun? Essential Question: How has technology expanded our knowledge of the Earth, Moon, and Sun System.? Enduring Understanding: There are observable, predictable patterns of mo ...
P7 Further Physics : Observing the Universe
P7 Further Physics : Observing the Universe

A Very Dense Low-Mass Molecular Condensation in Taurus
A Very Dense Low-Mass Molecular Condensation in Taurus

... a protostellar core within a time scale of ~ 104 yr. This starless condensation, named MC 27 in complete surveyed molecular condensations in Taurus, is ~ 0.1 pc in size and ~ 3M® in mass. It exhibits fairly strong and narrow H 1 3 CO + emission of the J = 4-3, 3-2, and 1-0 transitions, as well as se ...
Globular Clusters
Globular Clusters

... place. The nuclear energy production slows down and eventually stops the contraction. The star reaches a nice equilibrium, balancing energy production and transfer and global brightness, and enters into the main sequence (MS). This equilibrium holds on the MS for more than 70% of the total stellar l ...
Bayesian mass and age estimates for transiting exoplanet host stars⋆
Bayesian mass and age estimates for transiting exoplanet host stars⋆

2 Galaxy morphology and classification
2 Galaxy morphology and classification

... The dark halo is the dark matter component that envelopes all galaxies. It extends well beyond the visible extents of the galaxy. The ,mass density decreases with radius roughly as where measurable. The nature of the particles that comprise this component is not known, but there is strong evidence t ...
suggested
suggested

... space: H, O, C, and N. He assumed these atoms combined on a surface of some kind to form frozen saturated molecules. The surface was left as ‘to be determined’ (TBD). This is what later became known as the ‘dirty ice’ model and was the first application of surface physics to interstellar dust. The di ...
docx - STAO
docx - STAO

... is accomplished by drawing the sky (star patterns) on the astrolabe with moveable parts to adjust for the date and time. The traditional sky map astrolabe allowed people to locate celestial objects in the sky similar to how a place is located using a map. A mariner’s astrolabe is different in that i ...
Student Activity: Using a Mariner`s Astrolabe
Student Activity: Using a Mariner`s Astrolabe

... is accomplished by drawing the sky (star patterns) on the astrolabe with moveable parts to adjust for the date and time. The traditional sky map astrolabe allowed people to locate celestial objects in the sky similar to how a place is located using a map. A mariner’s astrolabe is different in that i ...
Stars
Stars

... (but less if AGS09 replaces AGS05). OP opacities give a better fit than OPAL. However in that region, there is no way to change the OP opacity by a sufficient amount to compensate the effects of mixture (Badnell et al. 2005) ...
Examiners` Report June 2012 GCSE Astronomy 5AS01 01
Examiners` Report June 2012 GCSE Astronomy 5AS01 01

Evolution of Warm Debris Around Sun-like Stars: Clues to Terrestrial
Evolution of Warm Debris Around Sun-like Stars: Clues to Terrestrial

... Our main result is that 10-100 Myr appears to be the preferred epoch for the generation of 24 micron debris excess around sun-like stars. Studies of extinct radio-active nuclides suggest that the Earth-Moon system was formed about 30 Myr after the formation of the Sun. This is also consistent with n ...
Century-Long Monitoring of Solar Irradiance and Earth`s Albedo
Century-Long Monitoring of Solar Irradiance and Earth`s Albedo

The Sun`s journey through the local interstellar medium: the
The Sun`s journey through the local interstellar medium: the

Inner Solar System Material Discovered in the Oort Cloud
Inner Solar System Material Discovered in the Oort Cloud

... must   be   measured   and   compared   with   the   predictions   from   early   solar   system   formation   models,   some   of   which   predict   significant   reshuffling   of   material   throughout   the   solar   system.     Ground-­‐ ...
INTERSTELLAR MedLab
INTERSTELLAR MedLab

... These regions were called nebulae, which means “clouds.” As study of the interstellar medium progressed, these nebulae were divided into categories: Emission – a gas cloud that receives energy from a hot star(s), allowing the nebula to give off radiation in emission. Reflection – dust clouds that re ...
The Role of Radioactive Isotopes in Astrophysics
The Role of Radioactive Isotopes in Astrophysics

... had been created in previous massive stars, thereby seeding the interstellar matter with primary elements. These seed nuclei are required in order that secondary nuclei be produced from them in stars. He emphasized especially 14 N, 18 O, 19 F and 22 Ne in that regard, each of which depends on initia ...
The surface composition of Beta Pictoris
The surface composition of Beta Pictoris

... inferred by Paresce (1991) from Geneva photometry, a result that has prompted King and Patten (1992) to suggest that β Pic is a λ Boo star. We note that the HST GHRS data analyzed by Lanz and Hubeny (1995) also rule out a low metallicity, and that their own evaluation of Geneva indices leads to a no ...
LESSON 8: STARS
LESSON 8: STARS

AN ATTEMPT To prove the MOTION OF THE EARTH FROM
AN ATTEMPT To prove the MOTION OF THE EARTH FROM

... removed. Next the bending and warping of an Instrument by its own weight, will make a very considerable alteration. And thirdly, the common way of Division is also lyable to many inconveniencies: And 'tis hardly possible to ascertain all the subdivisions of Degrees into minutes for the whole Quadran ...
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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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