2. 职称英语
  3. COMETS (1) Comets are among

COMETS (1) Comets are among

游客2024-01-02  9
问题                                                 COMETS
    (1) Comets are among the most interesting and unpredictable bodies in the solar system. They are made of frozen gases (water vapor, ammonia, methane, carbon dioxide, and carbon monoxide) that hold together small pieces of rocky and metallic materials. Many comets travel in very elongated orbits that carry them far beyond Pluto. These long-period comets take hundreds of thousands of years to complete a single orbit around the Sun. However, a few short-period comets (those having an orbital period of less than 200 years), such as Halley’s Comet, make a regular encounter with the inner solar system.
    (2) When a comet first becomes visible from Earth, it appears very small, but as it approaches the Sun, solar energy begins to vaporize the frozen gases, producing a glowing head called the coma. The size of the coma varies greatly from one comet to another. Extremely rare ones exceed the size of the Sun, but most approximate the size of Jupiter. Within the coma, a small glowing nucleus with a diameter of only a few kilometers can sometimes be detected. As comets approach the Sun, some develop a tail that extends for millions of kilometers. Despite the enormous size of their tails and comas, comets are relatively small members of the solar system.
    (3) The observation that the tail of a comet points away from the Sun in a slightly curved manner led early astronomers to propose that the Sun has a repulsive force that, pushes the particles of the coma away, thereby forming the tail. Today, two solar forces are known to contribute to this formation. One, radiation pressure, pushes dust particles away from the coma. The second, known as solar wind, is responsible for moving the ionized gases, particularly carbon monoxide. Sometimes a single tail composed of both dust and ionized gases is produced, but often two tails—one of dust, the other, a blue streak of ionized gases—are observed.
    (4) As a comet moves away from the Sun, the gases forming the coma recondense, the tail disappears, and the comet returns to distant space. Material that was blown from the coma to form the tail is lost from the comet forever. Consequently, it is believed that most comets cannot survive more than a few hundred close orbits of the Sun. Once all the gases are expelled, the remaining materials—a swarm of tiny metallic and stony particles—continue the orbit without a coma or a tail.
    (5) Comets apparently originate in two regions of the outer solar system. Most short-period comets are thought to orbit beyond Neptune in a region called the Kuiper belt, in honor of the astronomer Gerald Kuiper. During the past decade over a hundred of these icy bodies have been discovered. Most Kuiper belt comets move in nearly circular orbits that lie roughly in the same plane as the planets. A chance collision between two comets, or the gravitational influence of one of the Jovian planets—Jupiter, Saturn, Uranus, and Neptune—may occasionally alter the orbit of a comet in these regions enough to send it to the inner solar system and into our view.
    (6) Unlike short-period comets, long-period comets have elliptical orbits that are not confined to the plane of the solar system. These comets appear to be distributed in all directions from the Sun, forming a spherical shell around the solar system, called the Oort cloud, after the Dutch astronomer Jan Oort. Millions of comets are believed to orbit the Sun at distances greater than 10,000 times the Earth-Sun distance. The gravitational effect of a distant passing star is thought to send an occasional Oort cloud comet into a highly eccentric orbit that carries it toward the Sun. However, only a tiny portion of the Oort cloud comets have orbits that bring them into the inner solar system.
    (7) The most famous short-period comet is Halley’s Comet, named after English astronomer Edmond Halley. [A] Its orbital period averages 76 years, and every one of its 30 appearances since 240 B.C. has been recorded by Chinese astronomers. [B] When seen in 1910, Halley’s Comet had developed a tail nearly 1.6 million kilometers (I million miles) long and was visible during daylight hours. [C] Its most recent approach occurred in 1986. [D] [br] According to paragraph 3, what is true about comets’ tails?
选项 A、Their shapes led early astronomers to draw false conclusions about the Sun.
B、They consist mostly of ionized gases that had been blown out of the Sun.
C、Radiation pressure and solar wind both play a role in their formation.
D、Their dust content decreases as a comet nears the Sun.
答案 C
解析 本题属于事实信息题，题干要求根据第3段来选出有关彗尾的正确说法。原文第3段第2—4句提到，人们普遍认为有两股太阳力促使彗尾的形成：其一是辐射压力；其二是太阳风。C项“辐射压力和太阳风都对彗尾的形成起作用”符合表述，故选。A项“彗尾的形状导致早期天文学家得出有关太阳的错误结论”可定位到第3段第1句，但此处说的是早期天文学家得小了关于彗尾是如何形成的错误结论，而不是关于太阳的错误结论。B项“彗尾主要是由被吹出太阳的电离气体组成”，根据第3段最后一句可知，彗尾不仅由尘埃组成，还由电离气体组成。D项“当彗星接近太阳时，彗尾的尘埃含量减少”没有依据。
转载请注明原文地址:https://www.tihaiku.com/zcyy/3327435.html
相关试题推荐
随机试题
最新回复(0)