HOP ON HERE!

1

  • First, Produce a Plasma.
  • This plasma X

    WHAT'S PLASMA?

    Plasma is a kind of ionized gas. The sun, lightning and auroras are all plasma. X

    WHAT DOES "IONIZED" MEAN?

    An atom or molecule is ionized if it has a negative or positive charge.
    approximates the outer atmosphere of Titan, and includes the same ingredients that scientists believe make up the gas that gives that moon its characteristic orange haze.
  • Plasma-image
  • Credit: NASA

2

  • Fill ’er Up.
  • At a laboratory in Paris, scientists fill up a reactor mostly with nitrogen X

    NITROGEN?

    Nitrogen makes up about three-quarters of the Earth’s atmosphere. Normally, two atoms of the element bind to form dinitrogen (N2).
    Nitrogen-image
    gas, then add a little bit of methane. X

    METHANE?

    Methane molecules are made up of one carbon and four hydrogens (CH4). Like nitrogen, it’s a colorless, odorless gas.
    Methane-image

3

  • Let the Sun Shine In.
  • The molecules in the real Titan’s haze don’t exist in a reactor: They are constantly bombarded by the energy of the sun’s UV rays. So Maillard needs to simulate this energy and get the gases in his reactor to socialize. To do this, he adds another kind of energy to his system; it’s kind of like turning up the radio at a lackluster party. In fact, Maillard actually sends radio waves X

    WHAT ARE RADIO WAVES?

    They are a type of electromagnetic radiation with a relatively long wavelength.
    through the reactor. Suddenly, molecules that had been waltzing like couples in a ballroom begin thrashing like teens in a mosh pit, sending electrons flying, ionizing each other, and morphing from a gas into a plasma bearing the same lovely, pink tint as Titan.

4

  • A Monster Mosh.
  • With all this molecular moshing going on, molecules that bump into each other sometimes bond together into new, larger molecules.
  • monster-mosh-image

5

  • A Mega Mosh.
  • As time passes, more molecules combine into bigger and bigger structures.
  • mega-mosh-image

6

  • Powder Down.
  • After a few days, those growing gas molecules reach a point at which gravity kicks in, and they float down into a waiting beaker in the form of a brown powder that contains the tholins X

    WHAT'S A THOLIN?

    These organic molecules form when simple carbon-containing compounds like methane get energized by UV or cosmic rays, often in the presence of nitrogen or other compounds. The outer atmosphere of Titan is full of these tholins, which could be precursors to life in the presence of water.
    Maillard studies. The longer the process continues, the more complex the molecules become.

7

  • The Right Weigh.
  • Tholins come in all shapes and sizes, and Maillard’s job is to identify exactly which molecules he cooked up in his replica of Titan’s haze. So first, he puts the molecules inside a 12 - tesla X

    WHAT'S A TESLA?

    It’s a unit of magnetic field strength. A typical hospital MRI magnet generates a field of about 2 or 3 T.
    ion cyclotron resonance (ICR) X

    WHAT'S ICR?

    These magnets reveal the chemical composition of complex compounds by separating and weighing each of them. Every kind of molecule has a unique weight.
    magnet located in Rouen, France.

8

  • The Big Reveal.
  • This 12-T instrument identified 15,000 different molecules in Maillard’s powder, each represented by a different peak X

    PEAK?

    As shown here, each peak represents a unique molecular mass that corresponds to a unique molecule.
    Peak-image
    in his data. But the instrument could only detect molecules up to 800 daltons. X

    WHAT'S A DALTON?

    An atomic-scale unit of mass that scientists use to weigh atoms and molecules. A single proton weighs about one dalton.

9

  • Bring in the Big Guns.
  • So Maillard flew to Florida, where the world’s strongest ICR magnet is housed at the National MagLab. Thanks to its 21-tesla field, it could weigh molecules up to 1,200 daltons, more than doubling the number of molecular species Maillard could see. Also, because of the instrument’s higher resolution, X

    WHATS RESOLUTION?

    Thanks to the 21-T’s stronger field, it could see the molecules in greater detail, and therefore tell the difference between molecules that were very similar in atomic mass.
    Maillard learned that some molecules that the 12-T magnet had identified were actually several different kinds of molecules that had been inaccurately represented by one peak. These details gave Maillard fresh insight into the chemical diversity surrounding Titan.

10

  • To Pluto — and Beyond!
  • In true astronaut spirit, Maillard and his colleagues are not content to stop at Titan. Venturing to the edges of our solar system, they recently approximated the atmosphere of Pluto (believed to include methane, nitrogen and carbon monoxide) and examined those chemicals in the 21-T as well. What did they learn? That’s an outta-this-world story for another time ...
  • pluto-image
  • Credit: NASA