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[历年真题] 托福阅读历年真题精选37

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发表于 2012-8-14 22:34:35 | 显示全部楼层 |阅读模式
Questions 1-9:
9 z( W4 ?. S+ O0 N9 lEuropa is the smallest of planet Jupiter’s four largest moons and the second moon
; H/ q5 p3 L. Dout from Jupiter. Until 1979, it was just another astronomy textbook statistic. Then 2 b" `+ f: @. a
came the close-up images obtained by the exploratory spacecraft Voyager 2, and within % Z9 y) E" {! p* a9 O
days, Europa was transformed-in our perception, at least-into one of the solar system’s 6 R' ^* p! J6 [
(5)most intriguing worlds. The biggest initial surprise was the almost total lack of detail,
/ b% \& c  q! O: f9 Z6 Zespecially from far away. Even at close range, the only visible features are thin, kinked! O2 p9 M  j% Z  t5 Q
brown lines resembling cracks in an eggshell. And this analogy is not far off the mark.
* X5 v# k8 [, K9 fThe surface of Europa is almost pure water ice, but a nearly complete absence of
7 c% i0 h- B& o3 J1 c* }: K  craters indicates that Europa’s surface ice resembles Earth’s Antarctic ice cap. The$ n% ~$ G* N) D' s3 ^1 Q4 v: l+ g
(10) eggshell analogy may be quite accurate since the ice could be as little as a few kilometers # X8 B4 Z1 m! G6 [- R
thick –a true shell around what is likely a subsurface liquid ocean that , in turn, encases
7 i: n! A; q: u& U2 n  a rocky core. The interior of Europa has been kept warm over the eons by tidal forces
6 v$ v; l0 b3 Y& k9 ^  generated by the varying gravitational tugs of the other big moons as they wheel around
/ `3 `4 u+ s. i- |' M  Jupiter. The tides on Europa pull and relax in an endless cycle. The resulting internal heat ) R8 P. J: O% @3 b6 }3 j
(15) keeps what would otherwise be ice melted almost to the surface. The cracklike marks on5 ]" _$ s. U2 C" ?
  Europa’s icy face appear to be fractures where water or slush oozes from below.
& b: b1 @1 c- J! F1 Q9 p9 t9 s. h0 d) A0 f       Soon after Voyager 2’s encounter with Jupiter in 1979, when the best images of1 Y5 o2 B- _& k; n% N* G% V
    Europa were obtained, researchers advanced the startling idea that Europa’s subsurface& z: q* e2 @5 m2 {# Z8 P
    ocean might harbor life. Life processes could have begun when Jupiter was releasing a
" z- X) z* K% _$ A(20 )vast store of internal heat. Jupiter’s early heat was produced by the compression of the3 y" g" L2 C$ r/ F
    material forming the giant planet. Just as the Sun is far less radiant today than the primal0 G$ G" h9 ~: k- D' F
    Sun, so the internal heat generated by Jupiter is minor compared to its former intensity.
" B; x0 D7 C6 F    During this warm phase, some 4.6 billion years ago, Europa’s ocean may have been liquid! j! E8 c' R) K7 Y# j. I5 o1 N
    right to the surface, making it a crucible for life. 9 _. o# ^4 d, l& K0 \/ a7 ]5 h
$ K3 l8 j5 [) Y4 Y! P
What does the passage mainly discuss?
( \% X; M/ _' e4 u2 T! _( yThe effect of the tides on Europa’s interior
# W$ ^* a0 ?9 |4 ~Temperature variations on Jupiter’s moons+ O4 f1 z1 q8 n& y0 k% F
Discoveries leading to a theory about one of Jupiter’s moons# H$ G0 \  E  C
Techniques used by Voyager 2 to obtain close-up images.
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 楼主| 发表于 2012-8-14 22:34:36 | 显示全部楼层

托福阅读历年真题精选37

The word “intriguing” in line 5 is closest in meaning to</p>changing6 u5 Z: X+ I3 P8 D4 P$ O
perfect
, ^9 C1 w' F, ^* qvisible
. D( u. H; J* R! Ufascinating  , ?! o) U3 P/ v) L4 k, Q
In line 7, the another mentions “cracks in an eggshell” in order to help readers
. _6 K0 z. X5 W- ?$ @' P: fvisualize Europa as scientists saw it in the Voyager 2 images
, w4 M5 z! ]  B4 l( T- Nappreciate the extensive and detailed information available by viewing Europa from far away* j. M1 }' O( A, E% @+ V
understand the relationship of Europa to the solar system
# f. A3 O4 N- Q/ o7 R9 p6 jrecognize the similarity of Europa to Jupiter’s other moons
9 M% |7 \9 j, t* d3 B+ A" ~% U3 U4.  It can be inferred from the passage that astronomy textbooks prior to 1979 5 n; X' e2 B) B( ^
(A)  provided many contradictory statistics about Europa$ c  v! K7 L7 [8 \
(B)  considered Europa the most important of Jupiter’s moons
, s9 w0 o. d/ \' S) G(C)  did not emphasize Europa because little information of interest was available, p3 x# n; P) C4 k  `, X
(D)  did nor mention Europa because it had not yet been discovered , U# B2 e  ?; z+ _/ N+ ^; `
5.  what does the author mean by stating in line 7 that “this analogy is not far off the mark”?
: s* j1 t- u# S, b* Q6 d(A)   The definition is not precise.
& D3 ?4 q! {* f2 O(B)   The discussion lacks necessary information.
2 M* @! u7 [! k7 y( B/ n5 g(C)   The differences are probably significant.
. s8 [. w9 M8 x( C* ~% q(D)   The comparison is quite appropriate.
8 `1 J  _# W% J: z% @. t! B/ _0 l6.   IT can be inferred from the passage that Europa and Antarctica have in common which of the following?. N& u( N3 ]& @9 c* N' A, \6 ]
    (A)   Both appear to have a surface with many craters.
1 `8 V( e2 e+ s! _8 D, M    (B)   Both may have water beneath a thin, hard surface.
* l/ D. G2 l5 F; W1 g, V    (C)   Both have an ice can that is melting rapidly.
, d' f0 O) N! F) d- w( Z    (D)   Both have areas encased by a rocky exterior.
$ Y7 ^& C; ?8 ^/ M7.  The word “endless” in line 14 is closest in meaning to $ i; H' a5 P5 i7 L
(A)   new. Y, c6 I& L- d0 ~4 U( {- h
(B)   final6 t$ P8 H' h6 E4 E3 t* r* x
(C)   temporary
. _' @: W; e  L7 _: F% u(D)   continuous8 [) y* ?3 l/ t" l' G7 \4 N
8.  According to the passage, what is the effect of Jupiter’s other large moons on Europa?9 ^0 `: _. P1 B4 v) m& \
(A) They prevent Europa’s subsurface waters from freezing.+ x1 B. T" Y! Z2 C& F
(B) They prevent tides that could damage Europa’s surface.5 X* Y  E& Q- J! c
(C) They produce the very hard layer of ice that characterizes Europa.2 G, E+ U* i, M
(D) They assure that the gravitational pull on Europa is maintained at a steady level.
) y, \# n) K; f) k+ T8 V  G1 p9   According to the passage, what is believed to cause the thin lines seen on Europa’s surface?5 u5 `1 O! v% I+ I) e
(A) A long period of extremely high tides
) g" L0 v2 G2 K: o0 D. M- l(B) Water breaking through from beneath the surface ice
, W$ ~2 \' v- Y9 o* O(C) The continuous pressure of slush on top of the ice
& p9 a4 s0 z+ l7 m(D) Heat generated by the hot rocky core
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