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Option_E_Astrophysics_
Option_E_Astrophysics_

Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

... • acquire mass, if becomes > 1.4 M(Sun) SUPERNOVA (Ia). p + e  n + neutrino • Usually leaves neutron star For high mass stars • fusion continues beyond C,O to Iron • if Mass(core) > 1.4 M(Sun) core collapses in SUPERNOVA (II) • leaves either Neutron Star or Black Hole • Most SN are this type PHYS 1 ...
• This chapter concentrates on five goals:
• This chapter concentrates on five goals:

... • Two, in the surface layers of stars hotter than about 20,000 K, there are many violent collisions between atoms. • These excite electrons to high energy levels or knock the electrons completely out of most atoms—so they become ionized. – In this case, few hydrogen atoms will have electrons in the ...
GET WORKSHEETS FROM MY ASSIGNMENTS PAGE Mrs
GET WORKSHEETS FROM MY ASSIGNMENTS PAGE Mrs

... 1. What are the stages in a low-mass star’s life? 2. What are the stages in a high-mass star’s life? 3. What determines a star’s type? 4. What makes the Sun an ideal star for life? 5. Is the Sun a low-mass or high-mass star? 6. Looking at the H-R diagram, what are the: hottest, dimmest stars? cooles ...
Ay 112 Midterm review
Ay 112 Midterm review

Nucleosynthesis and the death of stars
Nucleosynthesis and the death of stars

... 4 H  He + energy + neutrinos Mass of 4 H > Mass of 1 He •In every second, 600 million tons of hydrogen converts into helium to power the Sun •At this rate, the Sun can continue hydrogen fusion for more than 6 billion years. ...
Lesson 3: Calculating distances to stars
Lesson 3: Calculating distances to stars

The star Betelgeuse is about 500 light years away from us. If this star
The star Betelgeuse is about 500 light years away from us. If this star

Lucas - WordPress.com
Lucas - WordPress.com

Powerpoint
Powerpoint

... (t = 0 defined by the neutrino burst) – Kirshner et al, ApJ, 320, 602, (1987), showed an emission temperature of 15,000 K that was already declining rapidly. Ultraviolet observations later (Fransson et al, ApJ, 336, 429 (1989) showed narrow emission lines of N III, N IV, N V, and C III (all in the 1 ...
Cosmic Dawn A Hunting for the First Stars in the Universe
Cosmic Dawn A Hunting for the First Stars in the Universe

... of these secondary elements backwards in time, we can infer the existence of generations of stars that have long since disappeared, in much the same way that an archeologist peels back geological strata to map the fossil record of extinct species. What astronomers call the “pollution” of the univer ...
V = 3 d3 = 4188.8 pc N = ρV = 0.1 pc χ 4188.8 pc = 419
V = 3 d3 = 4188.8 pc N = ρV = 0.1 pc χ 4188.8 pc = 419

Star Maps and Constellations (pdf 3.7 Megs)
Star Maps and Constellations (pdf 3.7 Megs)

PDF format
PDF format

... Why do protostars rotate rather fast and end up surrounded by disks of material? ...
1 Sun Stars Planets. Problem Sheet I
1 Sun Stars Planets. Problem Sheet I

... (d) By finding also how effective temperature Teff scales with mass for these stars, deduce a relation between log L and log Teff. 8. A main sequence star with the same radius as the Sun has a maximum energy output in visible light at a wavelength of 500 nm. If this star goes on to become a red gian ...
Contents ISP 205 Section 2 Study Guide for Test 3 28 March 2007
Contents ISP 205 Section 2 Study Guide for Test 3 28 March 2007

... White dwarfs are earth-sized, dead stars. Degenerate electrons produce the pressure. Neutron stars are Lansing-sized stars made of degenerate neutrons Black holes are so compact that light cannot escape from them. Exploding stars, supernovae, spew elements into space. Planets form near other stars. ...
Lecture
Lecture

... • First stage: all stars start fusing hydrogen (H) to make helium (He) • This stage is considered to be the longest stage in a star’s lifetime ( 90% of its total lifespan) • Second stage: Fusing of helium (He) to make carbon (C) • The life of some stars (like our Sun) stops after this stage, but ot ...
1. This question is about some of the properties of Barnard`s star
1. This question is about some of the properties of Barnard`s star

Question 1 The star Regulus, in the constellation Leo, appears
Question 1 The star Regulus, in the constellation Leo, appears

... . 2. elliptical galaxies with bright, starlike nuclei. ...
Chapter 13 Neutron Stars and Black Holes
Chapter 13 Neutron Stars and Black Holes

... The mass of a neutron star cannot exceed about 3 solar masses. If a core remnant is more massive than that, nothing will stop its collapse, and it will become smaller and smaller and denser and denser. Eventually the gravitational force is so intense that even light cannot escape. The remnant has be ...
Collapse of an unstable Neutron Star to a Black Hole
Collapse of an unstable Neutron Star to a Black Hole

N5128PNSydney
N5128PNSydney

... some higher values near centre (Field 42). Assuming most PN have similar stellar temperature and most of O in O++ => O/H abundance [Ne III]/[O III] very constant as found in other PN studies (MW, MC’s). Ne/O ratio ‘fixed’ by early high mass star evolution and marginal evidence for O enrichment by PN ...
Chapter 12
Chapter 12

Chapter 17 Measuring the Stars
Chapter 17 Measuring the Stars

Stellar Astrophysics: Introduction Q. Daniel Wang Astronomy Department University of Massachusetts
Stellar Astrophysics: Introduction Q. Daniel Wang Astronomy Department University of Massachusetts

... where M is any constant. We then obtain, for example, M αr −1 ...
< 1 ... 37 38 39 40 41 42 43 44 45 ... 167 >

Dyson sphere

A Dyson sphere is a hypothetical megastructure that completely encompasses a star and hence captures most or all of its power output. It was first described by Olaf Stapledon in his science fiction novel, ""Star Maker"". The concept was later popularly adopted by Freeman Dyson. Dyson speculated that such structures would be the logical consequence of the long-term survival and escalating energy needs of a technological civilization, and proposed that searching for evidence of the existence of such structures might lead to the detection of advanced intelligent extraterrestrial life. Different types of Dyson spheres correlate with information on the Kardashev scale.Since then, other variant designs involving building an artificial structure or series of structures to encompass a star have been proposed in exploratory engineering or described in science fiction under the name ""Dyson sphere"". These later proposals have not been limited to solar-power stations. Many involve habitation or industrial elements. Most fictional depictions describe a solid shell of matter enclosing a star, which is considered the least plausible variant of the idea (see below). In May 2013, at the Starship Century Symposium in San Diego, Dyson repeated his comments that he wished the concept had not been named after him.
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