BlueCat Motors E-books > Astronomy > Burnham's Celestial Handbook: An Observer's Guide to the by Robert Burnham Jr.

Burnham's Celestial Handbook: An Observer's Guide to the by Robert Burnham Jr.

By Robert Burnham Jr.

This complete assurance of the millions of celestial items open air our sunlight method. quantity II of the three-volume paintings comprises entries from Chamaeleon to Orion.

Show description

Read or Download Burnham's Celestial Handbook: An Observer's Guide to the Universe beyond the Solar System (1 PDF

Best astronomy books

Deep-Sky Wonders

Highlights from Sky & Telescope's Deep-Sky Wonders column demonstrate the independence of idea and devotion to craft that made author "Scotty" Houston a favourite between readers for nearly 50 years. Sky & Telescope journal contributing editor Stephen James O'Meara has chosen and organized the simplest of Scotty's paintings right into a year-round consultant to the superstar clusters, nebulae, and galaxies that trap skygazers into their backyards on transparent, darkish nights.

Chemical Evolution of Galaxies

The time period “chemical evolution of galaxies” refers back to the evolution of abundances of chemical species in galaxies, that's because of nuclear methods taking place in stars and to fuel flows into and out of galaxies. This e-book bargains with the chemical evolution of galaxies of all morphological kinds (ellipticals, spirals and irregulars) and stresses the significance of the megastar formation histories in picking out the houses of stellar populations in several galaxies.

Twenty-Five Astronomical Observations That Changed the World: And How To Make Them Yourself

"Twenty-Five Astronomical Observations that modified the area" takes twenty-five trips via area, again in time and into human heritage. we start with the best sight of the Tycho Crater at the Moon, via a repeat of Galileo's observations of Jupiter's moons, after which movement out in the direction of the nebulae, stars, and galaxies.

StarGuides Plus: A World-Wide Directory of Organizations in Astronomy and Related Space Sciences

StarGuides Plus represents the main finished and appropriately tested choice of sensible info on enterprises curious about astronomy, comparable area sciences and different comparable fields. This useful reference resource (and its better half quantity, StarBriefsPlus) can be at the reference shelf of each library, association or person with any curiosity in those parts.

Extra resources for Burnham's Celestial Handbook: An Observer's Guide to the Universe beyond the Solar System (1

Sample text

An allowed transition is one in which an integral number of wavelengths can be completed in one electron orbit. Jn the simple Bohr model for hydrogen, in which the proton is orbited by an electron a given distance away, the angular momentum, L, is given by the equation: nh L — mvr = — 277 which specifies the allowed distances r for energy levels n; m is the mass of the atom, and h is Planck's constant (see Appendix 1). Electrons can move to different average distances from the nucleus when energy is exchanged, Collisions between the atom and another particle, or absorption of an incoming photon by the atom, can transfer energy and cause an electron to jump from one energy level to another.

We can detect planetary nebulae in other galaxies by their emission lines. Higher mass stars, in contrast, can fuse nuclei all the way up to the iron atom, : whose nucleus is the most stable of ail the elements. It takes energy to process iron, however, so at this stage core nucleosynthesis stops. In the absence of radiation pressure from nuclear fusion, the core of the high mass star collapses ? against gravitational forces. A shock wave is produced during the implosion, . which leads to an explosion outward at about 2000 km s ' 1 as the star becomes <, a supernova Th^.

They are usually elliptical galaxies. Their classification was not made by Hubble but is based on morphology studied by B. Vorontsov-VeTyanihiov and W. W. Morgan, Radio lobe galaxies are characterized by the strong radio emission coming from ends of jets 100 kpc (kiloparsec; 1000 pc) to 1 Mpc (megaparscc: 1000 kpc) across. The lobes typically are three or four times the size of the Milky Way. According to theory, they are the result of a strong jet associated with the central galaxy ejection of particles.

Download PDF sample

Rated 4.01 of 5 – based on 29 votes