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SEPTEMBER-OCTOBER 2017

that this chemical make-up is similar

to Earth’s primordial atmosphere.

The conditions on Titan, however,

are not conducive to the formation

of life as we know it; it’s simply too

cold. At ten times the distance from

the Earth to the Sun, Titan is so cold

that liquid methane rains onto its

solid icy surface, forming rivers, lakes,

and seas. These pools of hydrocar-

bons, however, create a unique envi-

ronment that may help molecules of

by ALMA Observatory

S

aturn’s largest moon, Titan, is

one of our solar system’s most

intriguing object and Earth-like

bodies. It is nearly as large as Mars

and has a hazy atmosphere made up

mostly of nitrogen with a smattering

of organic, carbon-based molecules,

including methane (CH

4

) and ethane

(C

2

H

6

). Planetary scientists theorize

ALMA confirms

complex chemistry in

Titan’s atmosphere

N

ASA’s Cassini spacecraft sees

bright methane clouds drifting in

the summer skies of Saturn’s moon

Titan, along with dark hydrocarbon

lakes and seas clustered around the

north pole. [NASA/JPL-Caltech/Space

Science Institute]

vinyl cyanide (C

2

H

3

CN) link together

to form membranes, features resem-

bling the lipid-based cell membranes

of living organisms on Earth.