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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 b+ M, q* J  W9 mEuropa is the smallest of planet Jupiter’s four largest moons and the second moon
5 C. B  n. j$ c& n; V: y. Nout from Jupiter. Until 1979, it was just another astronomy textbook statistic. Then
+ }1 z  p& F2 [came the close-up images obtained by the exploratory spacecraft Voyager 2, and within
6 g' n' n. ?+ ?8 o  Ldays, Europa was transformed-in our perception, at least-into one of the solar system’s
0 [0 v# S9 R( w, f* z3 X(5)most intriguing worlds. The biggest initial surprise was the almost total lack of detail,- F9 G" f" r, l. v# w
especially from far away. Even at close range, the only visible features are thin, kinked( b  o3 R" D% L, `. @- j- x5 _
brown lines resembling cracks in an eggshell. And this analogy is not far off the mark.
* q0 E* S6 I/ OThe surface of Europa is almost pure water ice, but a nearly complete absence of* e- R: I: R7 ^+ b3 y
  craters indicates that Europa’s surface ice resembles Earth’s Antarctic ice cap. The
- z& g) b2 y$ L1 I( }: M/ B(10) eggshell analogy may be quite accurate since the ice could be as little as a few kilometers   ^! i8 B/ u& R8 Q- E6 U3 k
thick –a true shell around what is likely a subsurface liquid ocean that , in turn, encases
! W1 D, P2 r/ C$ f8 I/ Q  a rocky core. The interior of Europa has been kept warm over the eons by tidal forces! l5 W7 T' m+ I' ?3 k9 V
  generated by the varying gravitational tugs of the other big moons as they wheel around
7 v+ F" Z8 e4 J4 h0 ^; G  Jupiter. The tides on Europa pull and relax in an endless cycle. The resulting internal heat : b4 r! C& c" V$ |# `
(15) keeps what would otherwise be ice melted almost to the surface. The cracklike marks on- E* y; K6 e! }: ]
  Europa’s icy face appear to be fractures where water or slush oozes from below. 0 ?8 o  H- M: i0 @# }0 u
       Soon after Voyager 2’s encounter with Jupiter in 1979, when the best images of
) ?7 u2 q; d$ w; k0 h, _    Europa were obtained, researchers advanced the startling idea that Europa’s subsurface/ }: N. `) D* F$ g
    ocean might harbor life. Life processes could have begun when Jupiter was releasing a% ?0 h; t+ b( L$ I/ f& @" Y' {6 a
(20 )vast store of internal heat. Jupiter’s early heat was produced by the compression of the- M+ g# i; u1 N( d- M' r
    material forming the giant planet. Just as the Sun is far less radiant today than the primal
" K2 J/ u& l, K7 w, I# y    Sun, so the internal heat generated by Jupiter is minor compared to its former intensity.+ s, Q% ?! V2 A0 f8 S+ ?/ B% }2 ~( P: b
    During this warm phase, some 4.6 billion years ago, Europa’s ocean may have been liquid
9 ~1 i6 K- e; x! u4 |    right to the surface, making it a crucible for life. % {' ^3 C2 _6 U+ B

+ x5 Z' g7 v( _- c6 `What does the passage mainly discuss?
+ F; e( N: w# ~, r2 QThe effect of the tides on Europa’s interior: p( `1 r# z8 e* P) U  ~
Temperature variations on Jupiter’s moons  _) [5 h% u! F% \. j+ S* n
Discoveries leading to a theory about one of Jupiter’s moons% t. y" l# u" }; H
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>changing$ D1 s; q7 C3 V+ s, z
perfect# g- i. a  z8 W- x2 M0 Z
visible
' Y5 Q4 m8 w: h4 |: ^. m9 t9 Zfascinating  / R. ]0 r0 ~7 X6 ^7 o
In line 7, the another mentions “cracks in an eggshell” in order to help readers
9 q: Z! |2 e& U- n) A# }# Uvisualize Europa as scientists saw it in the Voyager 2 images& G$ {# K/ M/ ^4 Z; n
appreciate the extensive and detailed information available by viewing Europa from far away
" [  i5 O% p1 }7 D; V2 c$ Munderstand the relationship of Europa to the solar system
$ D0 S* e$ V$ r( Q% J% i2 o( Urecognize the similarity of Europa to Jupiter’s other moons
, k) l( i& E$ T4.  It can be inferred from the passage that astronomy textbooks prior to 1979 2 W- o# _$ D! [: h+ L
(A)  provided many contradictory statistics about Europa4 l& R5 c8 n" N% v/ I$ }
(B)  considered Europa the most important of Jupiter’s moons) ]$ ]5 ^$ X2 [' H& B1 w
(C)  did not emphasize Europa because little information of interest was available5 v' m$ t8 \: U4 J% l0 e$ F
(D)  did nor mention Europa because it had not yet been discovered
  w0 `8 v* B5 O4 f% R. q3 _7 A5.  what does the author mean by stating in line 7 that “this analogy is not far off the mark”?! A9 D( ?. S; ]( k
(A)   The definition is not precise.
2 h2 `" J+ j& x' S2 k! l; D(B)   The discussion lacks necessary information.
* t# f& m8 Z1 t# R" ?' |5 T$ s(C)   The differences are probably significant.. {$ L1 b9 R8 j8 X0 x
(D)   The comparison is quite appropriate.: I, j' _6 N/ o+ T4 A3 \  B% v# }
6.   IT can be inferred from the passage that Europa and Antarctica have in common which of the following?. _/ Y7 o9 R. K5 H7 @$ f
    (A)   Both appear to have a surface with many craters. ' u8 [- Z: J4 f( j4 b
    (B)   Both may have water beneath a thin, hard surface.: Y2 g5 A# s7 m" f0 m4 q
    (C)   Both have an ice can that is melting rapidly.4 I- d3 p/ C' u- ^
    (D)   Both have areas encased by a rocky exterior.
* L5 ]& i* z/ |/ d! O7 {7.  The word “endless” in line 14 is closest in meaning to
, `0 N) m& R$ `( Z& [3 h(A)   new
' I! O2 u! i* x% g(B)   final
- _5 p* L" j% p; P4 a) P5 N(C)   temporary6 U, y& I  U, ]) P3 h0 I
(D)   continuous7 K0 Z; ^8 P4 Y: {) l' L
8.  According to the passage, what is the effect of Jupiter’s other large moons on Europa?
7 p6 {' I- S$ b8 {- j6 ]) R- j(A) They prevent Europa’s subsurface waters from freezing., f- T- f  g* I! J1 k
(B) They prevent tides that could damage Europa’s surface.
/ ]' l( G3 m' `  z8 E! Z(C) They produce the very hard layer of ice that characterizes Europa.
" r- V( v* g% [. o" q7 Q9 {2 i) Z(D) They assure that the gravitational pull on Europa is maintained at a steady level. . ^3 h( A( c% j7 j. Q# H
9   According to the passage, what is believed to cause the thin lines seen on Europa’s surface?
/ ?. d6 ^! b# P(A) A long period of extremely high tides
. F3 S0 k; E( X3 g& H1 B: F; R(B) Water breaking through from beneath the surface ice; o# W4 @2 y  q. ~0 |, [* n
(C) The continuous pressure of slush on top of the ice
: h% j2 y( `( L2 y(D) Heat generated by the hot rocky core
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