05.01.2015 Views

Hadiah Nobel - Akademi Sains Malaysia

Hadiah Nobel - Akademi Sains Malaysia

Hadiah Nobel - Akademi Sains Malaysia

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

ARS (Greek: Ares) is the god<br />

of War. The planet probabty<br />

got this name due to its red<br />

colour; Mars is sometimes<br />

relerred to as the Red Planet. (An<br />

interesting side note: the Roman ood<br />

Mars was a god ol agriculture bel-ore<br />

becoming associated with the Greek<br />

Ares; those in favor ot colonising and<br />

lerralorming Mars may prefer this<br />

symbolism.) The name of the month<br />

March derives from Mars.<br />

Mars has been kno$/n since prehisloric<br />

limes. lt is still a favourite of scignce<br />

ficlion writers as the most lavourable<br />

place in lhe Solar System (other than<br />

Earth!) for human habitation.<br />

The first spacecratt to visit Mars was<br />

Mariner 4 in 1965. Severat others<br />

followed including Mars 2, the first<br />

spacocratt to land on Mars and the two<br />

Viking landers in 1976 (tett). Ending a<br />

long 20 year hiatus, Mars Pathfinder<br />

landed successtully on Mars on 1997<br />

July 4 (right).<br />

Mars' orbit is significan y elliptical.<br />

One result of this is a temDerature<br />

variation of about 3CPC at the subsolar<br />

point between aphelion and perihetion.<br />

This has a maior influence on Mars'<br />

climate.<br />

While the average temp€rature on<br />

Mars is about 2t8oK (-550C, -6ZF),<br />

Marlian surlace temperatures range<br />

l. What ls another nane br Ma|B<br />

2. Whldl u{as thg flr8t sgac€crafr to<br />

vieit Mars<br />

3. Who thlnks ot Mars ae a<br />

fa\ourable plac€ ior habltataton<br />

,f. How ls Mats and Earth sarn€ or<br />

dfielgno<br />

widely from as little as 140oK (-133oC, - surface and the bulk statistics of the<br />

207'F) at the winter pole to almost planet The most likely scenario is a<br />

30CPK (27"C, 80oF) on the day side dense core aboul 1700 km in radius, a<br />

dunng summer.<br />

mollen rocky mantle somewhal denser<br />

Though Mars is much smaller than than the Eanh's and a thin crust.<br />

Earth, its sudace area is about the Dala from Mars Global Surveyor<br />

same as the land surface area ol Earth. indicates that Mars' crust is about 80<br />

Except for Earth, Mars has the most km thick in the southern hemisohere<br />

highly varisd and interesting terrain of but only about 35 km thick in the north.<br />

any of the lerrestrial planets, some ol it Mars' relatively low density<br />

qurte spectacular:-<br />

compared to the other terrestrial<br />

o Olympus Mons: the largest planets indicates that its core probabty<br />

mountain in lhe Solar System rising 24 contains a relatively large traction of<br />

km above lhe surrounding plain. lts sulphur in addition to iron (iron and iron<br />

base is mor€ than 500 km in diameler sulfide).<br />

d is rimmed by a clitf 6 km high. Like Mercury and the Moon, Mars<br />

Tharsis: a huge bulge on the appears to lack active plate tectonics at<br />

Martian surtace that is about 40OO km present; there is no evidence of recenr<br />

ross and 10 km hioh.<br />

horizontal motion ot the surlace sucn<br />

Valles Marineris: i system of as the folded mountains so common on<br />

canyons 4000 km long and from 2 to 7 Earth. Wilh no lateral plate<br />

deep (top ot page);<br />

motion, hot-spots under<br />

Hellas Planitia: an impact crater in the crust stay in a<br />

the southem hemisphere over 6 km fixed position<br />

deep and 2000 km in diameter. relative to the<br />

Much ol the Martian surface is verv surface.<br />

old and cratered, but there are also<br />

much youngeritt valleys,<br />

.<br />

ridges, hills<br />

This,<br />

along with E<br />

and Dlains.<br />

the lower .L<br />

The southern hemisDhere of Mars ts sudace<br />

predominanlly ancient cratered gravity,<br />

highlands somewhat similar to the may {f.+ ,<br />

Moon. In contrast, most of the norlhern accounl '5.-. . :!<br />

hemisphere consists of plains which for the<br />

are much younger, low€r in elevation Tharis<br />

and have a much more comDlex bu196 and<br />

hislory.<br />

its<br />

An abrupt elevation change ol enormous<br />

sev€ral kilometerseems to occur at volcanoes.<br />

the boundary The reasons tor this There is no<br />

global dicholomy and abrupt boundary €vidence of current<br />

are unknown (some speculate that they volcanic activity,<br />

are due to a very large impact shorfly nowever.<br />

atler Mars' accretion).<br />

But there is n€w evidenc€ from<br />

Mars Global Surveyor has produceo Mars Global Surveyor that Mars may<br />

a nice 3D map of Mars that clearly have had tectonic activity in its €arly<br />

sho$,is these features.<br />

history, making comparisons to Earth<br />

The interior of Mars is known onlv all the mor€ interestino!<br />

by inference from data about the<br />

esti8otmg ss

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!