- •Analysis (introduction)
- •I. Структура предложения
- •II. Явные сказуемые
- •III. Неявные сказуемые
- •1) Present Indefinite
- •2) Past Indefinite
- •Part I section 1 geology
- •Exercises
- •Word-Building
- •Grammar Exercises
- •Lexical Exercises
- •Analysis
- •Section 2 geology
- •Exercises
- •Word-Building
- •Word Study
- •Grammar Exercises
- •Lexical Exercises
- •Analysis
- •Section 3 historical geology
- •Exercises Word-Building
- •Word Study
- •Grammar Exercises
- •Analysis
- •Section 4 the earth and the solar system
- •Exercises
- •Word-Building
- •Grammar Exercises
- •Word Study
- •Lexical Exercises
- •Analysis
- •Section 5 the solar system
- •Exercises
- •Word-Building
- •Word Study
- •Grammar Exercises
- •Lexical Exercises
- •Analysis
- •Section 6 the great parts of the earth
- •Exercises
- •Word-Building
- •Word Study
- •Grammar Exercises
- •Lexical Exercises
- •Section 7 the earth's crust, rocks, minerals
- •Exercises
- •Word-Building
- •Grammar Exercises
- •Word Study
- •Lexical Exercises
- •Section 8 (revision of sections 1-7)
- •Supplementary texts and extracts (for reading, discussion, translation, analysis)
- •I. Geology (introduction)
- •II. Mineralogy in russia
- •III. Mineralogy and geochemistry in the ussr
- •V. I. Vernadsky (1863 - 1945)
- •A. E. Fersman (1883 - 1945)
- •IV. Our place in the universe
- •V. Soviet scientists study earth's weather and the sun
- •VI. The lithosphere
- •VII. Environments
- •VIII. Igneous rocks
- •IX. The occurrence of minerals
- •X. Sedimentary rocks
- •XI. Laws of sedimentary sequence
Analysis
XXIII. Analyse the sentences in the following way:
1. Найдите подлежащее, группу подлежащего и сказуемое. 2. Укажите левые и правые определения (если таковые есть) подлежащего. 3. Укажите слова, к которым относятся выделенные предлоги. 4. Определите функцию группы слов, которая предшествует подлежащему (если таковая есть).
a) Precipitation of these descending, oxidizing, acid waters comes about in various ways. b) All around the land masses the depth of the sea increases very gradually. c) In the bedrock areas small mountain masses rise abruptly from the smooth desert surface.
Section 5 the solar system
Mechanically the solar system has one controlling member, the sun. The sun contains almost 99.9% (per cent) of the total mass of the solar system and controls by gravitational attraction the planets which revolve about it.
The planets are nearly spherical in shape but they are all bulged at the equator and flattened at the poles. The nine planets of the solar system are of different sizes and at different distances from the sun. The planets fall into two groups, called the inner and outer planets. The four inner planets are small pla-nets (Earth is the largest of the group). With the exception ofl Pluto, the outer planets are very much larger than the inner ones. Among the nine planets Jupiter is the largest and Mercury is the smallest, having a radius of only 1,500 miles, which is about 2,500 miles less than that of the earth. The sun has a radius more than 80 times that of the earth. The sun is over one million times as great in vo-lume as the earth. The surface area of the earth is only about one twelve thousandth the area of the sun's great surface.
Two things about the planetary orbits are of particular interest2: (a) all the planets revolve around the sun in the same direction and (b) with the exception of Pluto they travel in elliptical orbits which lie relatively close to a common plane.
Moreover, the sun, the moon, and the planets all rotate about their axes in the same direction that the planets revolve around the sun, with the exception of Uranus, whose rotational axis lies almost in the plain of its orbit.
The planets travel along their orbits at different velocities. There is a relationship between the velocity of a planet and the size of its orbit. The size of the orbit governs (controls) the speed at which the planet moves: the nearer to the sun a planet is, the faster it moves.
Notes
1 with the exception of — за исключением
2 to be of particular interest — представлять особый интерес
|
Planets |
Average Distance from Sun (Millions of Miles) |
Mean Diameter (Miles) |
Mean Density (gm/cm3) |
Length of Time for One Trip Around the Sun (Earth Units) |
|
Pluto [ˊplu:tou] |
3,670 |
4,000 |
4 (?) |
248,4 years |
|
Neptune[ˊneptju:n] |
2,790 |
31,000 |
1.51 |
165 years |
|
Uranus [ˊjuərənəs] |
1,780 |
33,000 |
1.68 |
84 years |
|
Saturn [ˊsætən] |
886 |
75,000 |
0.68 |
29.5 years |
Jupiter [ˊʤu:pɪtə] |
483 |
89,000 |
1.22 |
11.0 years |
|
|
Mars [ma:s] |
142 |
4,270 |
2.97 |
1.9 уears |
|
Earth [ə:θ] |
93 |
7,930 |
5.52 |
365 days |
Moon [mu:n] |
93 |
2,160 |
3.36 |
— |
|
Venus [ˊvi:nəs] |
67 |
7,600 |
5.I |
225 days |
|
|
Mercury [ˊmə:kjurɪ] |
36 |
3,000 |
5.4 |
88 days |
|
Sun [sʌn] |
— |
864,327 |
1.42 |
— |
Fig. 1. The Solar System
The average distance from Earth to Sun, 92.6 million miles, is one astronomical unit.
Words
a) Familiar words:
gravitational [ˏgrævɪ:ˊtеɪʃənəl], mass [mæs], mechanically [mi:ˊkænikəli], orbit [ˊɔ:bɪt], total [ˊtoutəl]
b) area [ˊɛərɪə] n площадь (простран-ство, район, зона)
attract [əˊtrækt] v притягивать
attraction [əˊtrækʃən] n притяжение, тяготение
bulge [bʌlʤ] v выпячиваться, делаться выпуклым
close [klous] adv близко
close to (smth., smb.) = near (smth., smb.) близко от, рядом с
common [ˊkɔmən] a 1. общий; 2. обычный, распространенный
contain [kənˊteɪn] v содержать в себе, включать
direction [dɪˊrekʃən] n направление
exception [ɪkˊsepʃən] n исключение
govern [ˊgʌvən] v регулировать (управлять)
inner [ˊɪnə] а внутренний
nearly [ˊnɪəlɪ] adv почти, приблизительно, около
outer [ˊautə] а внешний, наружный
particular [pəˊtɪkjulə] а особый,
особенный (частный)
percent [pəˊsent] n процент
plane [pleɪn] n плоскость
relationship [rɪˊleɪʃənʃɪp] n связь, зависимость, отношение
relatively [ˊrelətɪvlɪ] adv относительно
size [saɪz] n размер
speed [spi:d] n скорость
velocity [vɪˊlɔsɪtɪ] n скорость
volume [ˊvɔljum] n объем