other elements. Carbon has four valence electrons that can participate in the formation of chemical bonds allowing carbon atoms to form long chains, with each link leaving two potential bonds free to join with other atoms. Carbon bonds particularly easily with oxygen, hydrogen and nitrogen. Carbon is the major part of all living organisms on Earth.
For this reason, it is assumed that if life exists somewhere else in the universe, it will also be carbon-based. Carbon is the simple building block that organisms need to form organic compounds such as proteins, carbohydrates and fats. It is also lightweight and relatively small in size. Carbon molecules are strong and stable. Hence, they are perfect to build bodies like ours. In one form or another, the average adult human body contains about 16 kg of carbon. Te origin of the name ‘carbon’ comes from the Latin word
carbo, for charcoal. Carbon has been known and used for thousands of years as the black soot and charcoal left over after a fire. Carbon is also the most important part of gasoline. Carbon is the basis for technological wonders such as graphene, which is a material stronger than steel and more flexible than rubber.
9.3.3 Nitrogen
Figure 9.39: An artist’s concept of a plume of water vapour ejected off the icy surface of the Jovian moon Europa to an altitude of 200 km and then raining frost back onto the moon’s surface. It is believed that under Europa’s icy crust there is a subsurface ocean.
9.3.1 Water (and Temperature)
Te temperature must be in a range that allows for water in liquid form – this is what defines the ‘habitable zone’, also called the Goldilocks zone, after the children’s fairy tale of Goldilocks and the Tree Bears, in which the little girl chooses from sets of three items, ignoring the ones that are too extreme (large or small, hot or cold, etc.), and settling on the one in the middle, which is ‘just right’. Te bounds of the habitable zone are based on Earth’s
position in the solar system and the amount of heat the Earth receives from the sun. It defines the range of orbits around a star within which a planet’s surface can support liquid water. To determine whether a planet does have water or has lost it, we need to have measurements of its atmosphere. Water is contributory to extra-terrestrial life and intelligence, so the presence of water has been vital in the search for other habitable planets and moons.
9.3.2 Carbon
Carbon is the fourth most common element in the universe. It forms the basis of older stars: as they run out of hydrogen, they fuse helium into heavier elements – and this is how many of the other elements are made: carbon, nitrogen, oxygen, silicon, iron, sulphur, and so on up to iron. Complex molecules are composed of carbon bonded with
322
Nitrogen is the other important building block of life. It is the sixth most common element in the universe and is essential for all plants and animals to survive. Although nitrogen makes up almost 80% of our atmosphere, it is in an unreactive form that is not accessible to us. Plants rely on ammonium and nitrate created by bacteria in the soil and water, and animals obtain it through their food. Terefore, a big clue for biological activity on another planet is to find biochemically formed nitrogen. Nitrogen is essential because life is almost certainly going
to require amino acids – simple organic compounds that contain nitrogen – which are used in every cell of our bodies
Figure 9.40: Structure and contents of the first form of life on Earth: single-celled bacteria, consisting of an envelope of chemicals including DNA. Later, multi- function cells evolved into the animal cells from which we are constructed. Your body has more than 200 different types of cells. Each cell has a different job to help your body to function. There are blood cells, bone cells, and cells that make your muscles.
ASA/ESA/
K.Retherford/SWRI
Ali Zifan
Page 1 |
Page 2 |
Page 3 |
Page 4 |
Page 5 |
Page 6 |
Page 7 |
Page 8 |
Page 9 |
Page 10 |
Page 11 |
Page 12 |
Page 13 |
Page 14 |
Page 15 |
Page 16 |
Page 17 |
Page 18 |
Page 19 |
Page 20 |
Page 21 |
Page 22 |
Page 23 |
Page 24 |
Page 25 |
Page 26 |
Page 27 |
Page 28 |
Page 29 |
Page 30 |
Page 31 |
Page 32 |
Page 33 |
Page 34 |
Page 35 |
Page 36 |
Page 37 |
Page 38 |
Page 39 |
Page 40 |
Page 41 |
Page 42 |
Page 43 |
Page 44 |
Page 45 |
Page 46 |
Page 47 |
Page 48 |
Page 49 |
Page 50 |
Page 51 |
Page 52 |
Page 53 |
Page 54 |
Page 55 |
Page 56 |
Page 57 |
Page 58 |
Page 59 |
Page 60 |
Page 61 |
Page 62 |
Page 63 |
Page 64 |
Page 65 |
Page 66 |
Page 67 |
Page 68 |
Page 69 |
Page 70 |
Page 71 |
Page 72 |
Page 73 |
Page 74 |
Page 75 |
Page 76 |
Page 77 |
Page 78 |
Page 79 |
Page 80 |
Page 81 |
Page 82 |
Page 83 |
Page 84 |
Page 85 |
Page 86 |
Page 87 |
Page 88 |
Page 89 |
Page 90 |
Page 91 |
Page 92 |
Page 93 |
Page 94 |
Page 95 |
Page 96 |
Page 97 |
Page 98 |
Page 99 |
Page 100 |
Page 101 |
Page 102 |
Page 103 |
Page 104 |
Page 105 |
Page 106 |
Page 107 |
Page 108 |
Page 109 |
Page 110 |
Page 111 |
Page 112 |
Page 113 |
Page 114 |
Page 115 |
Page 116 |
Page 117 |
Page 118 |
Page 119 |
Page 120 |
Page 121 |
Page 122 |
Page 123 |
Page 124 |
Page 125 |
Page 126 |
Page 127 |
Page 128 |
Page 129 |
Page 130 |
Page 131 |
Page 132 |
Page 133 |
Page 134 |
Page 135 |
Page 136 |
Page 137 |
Page 138 |
Page 139 |
Page 140 |
Page 141 |
Page 142 |
Page 143 |
Page 144 |
Page 145 |
Page 146 |
Page 147 |
Page 148 |
Page 149 |
Page 150 |
Page 151 |
Page 152 |
Page 153 |
Page 154 |
Page 155 |
Page 156 |
Page 157 |
Page 158 |
Page 159 |
Page 160 |
Page 161 |
Page 162 |
Page 163 |
Page 164 |
Page 165 |
Page 166 |
Page 167 |
Page 168 |
Page 169 |
Page 170 |
Page 171 |
Page 172 |
Page 173 |
Page 174 |
Page 175 |
Page 176 |
Page 177 |
Page 178 |
Page 179 |
Page 180 |
Page 181 |
Page 182 |
Page 183 |
Page 184 |
Page 185 |
Page 186 |
Page 187 |
Page 188 |
Page 189 |
Page 190 |
Page 191 |
Page 192 |
Page 193 |
Page 194 |
Page 195 |
Page 196 |
Page 197 |
Page 198 |
Page 199 |
Page 200 |
Page 201 |
Page 202 |
Page 203 |
Page 204 |
Page 205 |
Page 206 |
Page 207 |
Page 208 |
Page 209 |
Page 210 |
Page 211 |
Page 212 |
Page 213 |
Page 214 |
Page 215 |
Page 216 |
Page 217 |
Page 218 |
Page 219 |
Page 220 |
Page 221 |
Page 222 |
Page 223 |
Page 224 |
Page 225 |
Page 226 |
Page 227 |
Page 228 |
Page 229 |
Page 230 |
Page 231 |
Page 232 |
Page 233 |
Page 234 |
Page 235 |
Page 236 |
Page 237 |
Page 238 |
Page 239 |
Page 240 |
Page 241 |
Page 242 |
Page 243 |
Page 244 |
Page 245 |
Page 246 |
Page 247 |
Page 248 |
Page 249 |
Page 250 |
Page 251 |
Page 252 |
Page 253 |
Page 254 |
Page 255 |
Page 256 |
Page 257 |
Page 258 |
Page 259 |
Page 260 |
Page 261 |
Page 262 |
Page 263 |
Page 264 |
Page 265 |
Page 266 |
Page 267 |
Page 268 |
Page 269 |
Page 270 |
Page 271 |
Page 272 |
Page 273 |
Page 274 |
Page 275 |
Page 276 |
Page 277 |
Page 278 |
Page 279 |
Page 280 |
Page 281 |
Page 282 |
Page 283 |
Page 284 |
Page 285 |
Page 286 |
Page 287 |
Page 288 |
Page 289 |
Page 290 |
Page 291 |
Page 292 |
Page 293 |
Page 294 |
Page 295 |
Page 296 |
Page 297 |
Page 298 |
Page 299 |
Page 300 |
Page 301 |
Page 302 |
Page 303 |
Page 304 |
Page 305 |
Page 306 |
Page 307 |
Page 308 |
Page 309 |
Page 310 |
Page 311 |
Page 312 |
Page 313 |
Page 314 |
Page 315 |
Page 316 |
Page 317 |
Page 318 |
Page 319 |
Page 320 |
Page 321 |
Page 322 |
Page 323 |
Page 324 |
Page 325 |
Page 326 |
Page 327 |
Page 328 |
Page 329 |
Page 330 |
Page 331 |
Page 332 |
Page 333 |
Page 334 |
Page 335 |
Page 336 |
Page 337 |
Page 338 |
Page 339 |
Page 340 |
Page 341 |
Page 342 |
Page 343 |
Page 344 |
Page 345 |
Page 346 |
Page 347 |
Page 348 |
Page 349 |
Page 350 |
Page 351 |
Page 352
