The Hundred Greatest StarsSpringer Science & Business Media, 7. 5. 2006 - Počet stran: 211 I have always loved the stars. I watch them, photograph one. And you can hardly talk about Zubenelgenubi them, research them, write about them. Their wonder without bringing in Zubeneschamali, so they too are is that they are there not simply for scientists, but for treated within one story. The Sun is not included in the all of us, filling the night sky with their sparkling beauty. 100 list, but instead leads the pack as “Star Zero. ” There are as many different kinds as there are stars Before describing the glories of the 100 stars, an themselves, each an individual. The heavens give us introduction briefs the beginning stargazer on basic bright ones, dim ones, near ones, far ones, the aged, stellar properties and explains the astronomical the young, those that help tell our ancient stories, and terminology, without which we would be continuously those nearly invisible even with the greatest of our tongue-tied. A separate glossary provides a quick technologies. Taken together, they relate the tale of our reminder. Then we move on to the stars themselves. existence, of the birth, life, and death of the Sun on Each of my favorite stars is introduced by a short which we depend. |
Vyhledávání v knize
Výsledky 1-5 z 63
Strana xiii
... orbit, not unlike the planets of our Solar System. In the vastly bigger Galaxy, however, it takes 200 million years for the Sun to go all the way around. As a result of differing orbits, the stars slide past each other, the nearby (or ...
... orbit, not unlike the planets of our Solar System. In the vastly bigger Galaxy, however, it takes 200 million years for the Sun to go all the way around. As a result of differing orbits, the stars slide past each other, the nearby (or ...
Strana xix
... orbit not just of Earth, but of Mars. Toward hotter classes, the difference between giants and dwarfs becomes progressively less, and near class A the two more-or-less merge. Dramatically larger and brighter than giants are the ...
... orbit not just of Earth, but of Mars. Toward hotter classes, the difference between giants and dwarfs becomes progressively less, and near class A the two more-or-less merge. Dramatically larger and brighter than giants are the ...
Strana xxi
... orbits a closer double. Or two close doubles will orbit each other, and then maybe a fifth star (or another double) will orbit the double-double. True multiples, in which all the stars mutually orbit each other, do exist, but are not ...
... orbits a closer double. Or two close doubles will orbit each other, and then maybe a fifth star (or another double) will orbit the double-double. True multiples, in which all the stars mutually orbit each other, do exist, but are not ...
Strana xxii
... orbit. The shifts yield velocities, orbital characteristics, and, again, information on stellar masses. Unfortunately, there is no simple way of knowing how a spectroscopic binary's orbital plane may be tilted to the line of sight. As a ...
... orbit. The shifts yield velocities, orbital characteristics, and, again, information on stellar masses. Unfortunately, there is no simple way of knowing how a spectroscopic binary's orbital plane may be tilted to the line of sight. As a ...
Strana xxiv
... orbit of Mercury. At a temperature of 100 million K, the quiet helium in the core takes on new life. The conditions are so extreme that three helium atoms can combine to form carbon and gamma rays; adding another helium atom makes ...
... orbit of Mercury. At a temperature of 100 million K, the quiet helium in the core takes on new life. The conditions are so extreme that three helium atoms can combine to form carbon and gamma rays; adding another helium atom makes ...
Obsah
2 | |
14 | 30 |
16 | 34 |
18 | 38 |
104 | 39 |
20 | 42 |
22 | 46 |
110 | 48 |
67 | 136 |
68 | 138 |
69 | 140 |
70 | 142 |
71 | 144 |
72 | 146 |
73 | 148 |
74 | 150 |
24 | 50 |
26 | 54 |
28 | 58 |
130 | 61 |
30 | 62 |
32 | 66 |
34 | 70 |
140 | 73 |
36 | 74 |
38 | 78 |
40 | 82 |
42 | 86 |
44 | 90 |
46 | 94 |
150 | 97 |
48 | 98 |
50 | 102 |
51 | 104 |
52 | 106 |
53 | 108 |
54 | 110 |
55 | 112 |
56 | 114 |
57 | 116 |
58 | 118 |
59 | 120 |
60 | 122 |
61 | 124 |
62 | 126 |
63 | 128 |
64 | 130 |
65 | 132 |
66 | 134 |
HZ 21 | 152 |
Mizar and Alcor Mu Cephei Mu Columbae MXB 1730335 | 153 |
76 | 154 |
200 | 155 |
77 | 156 |
78 | 158 |
79 | 160 |
80 | 162 |
81 | 164 |
82 | 166 |
83 | 168 |
84 | 170 |
85 | 172 |
86 | 174 |
87 | 176 |
88 | 178 |
89 | 180 |
90 | 182 |
91 | 184 |
92 | 186 |
93 | 188 |
94 | 190 |
95 | 192 |
96 | 194 |
97 | 196 |
98 | 198 |
99 | 200 |
100 | 202 |
STAR | 203 |
Acrux Adhara AG Draconis Albireo Algol Alpha Centauri Alphard Antares Arcturus Barnards Star Beta Canis Majoris Beta Cassiopeiae Beta Lyrae B... | 204 |
RS Ophiuchi SGR 1900+14 Sigma Octantis Sirius 16 Cygni 61 Cygni Spica SS Cygni SS 433 | 205 |
HD 93129A | 207 |
Další vydání - Zobrazit všechny
Běžně se vyskytující výrazy a sousloví
Absolute visual magnitude absorptions accretion Alpha astronomers atoms Beta binary black hole bright brighter brightest brown dwarfs Capella carbon carbon stars Cassiopeiae celestial central stars Cephei cloud companion constellation cool core Cygni Cygnus Delta Delta Cephei disk distance double star dust Earth eclipse emissions energy Epsilon Eridani Eta Carinae fainter fusing fusion Galaxy Galaxy’s Gamma giant star gravity helium Hubble Space Telescope hydrogen infrared interstellar ionized J. B. Kaler kilometers per second light luminous Lyrae magnetic fields main sequence million Mira Mizar naked-eye neutron star nova Observatory Ophiuchi orbit Orionis pair percent period planetary nebula planets Polaris pole pulsar radiation radio radius Residence rotation second-ascent seconds of arc Sigma Octantis Significance Sirius solar luminosities solar masses spectral spectrum speed spin star’s stellar subgiant supergiant supernova surface surrounding Tauri temperature Thuban tion Tycho’s Ursa variable Vega visible wavelengths white dwarf wind X-ray