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Starts With A Bang

Is Dark Matter required for life to exist?

It doesn’t interact with normal matter hardly at all, and yet it may be necessary for life itself.

“The privilege of a lifetime is being who you are.” –Joseph Campbell

Dark matter is the most mysterious, non-interacting substance in the Universe. Its gravitational effects are necessary to explain the rotation of galaxies, the motions of clusters, and the largest scale-structure in the entire Universe. But on smaller scales, it’s too sparse and diffuse to impact the motion of the Solar System, the matter here on Earth, or the origin and evolution of humans in any meaningful way. Yet the gravity that dark matter provides is an absolute necessity for allowing our galaxy to hold onto the raw ingredients that made life like us and planets like Earth possible at all. Without dark matter, the Universe would likely have no signs of life at all.

Image credit: M. Cappellari and the Sloan Digital Sky Survey.

Stars make up 100% of the light we observe in the Universe, but only 2% of the mass. When we look at the motions of galaxies, clusters and more, we find that the amount of gravitational mass outweighs the stellar mass by a factor of fifty. You might think, however, that other types of normal matter could account for this difference. After all, we’ve discovered lots of other types of matter in the Universe besides stars, including:

  • stellar remnants like white dwarfs, neutron stars and black holes,
  • asteroids, planets and other objects with masses too low (like brown dwarfs) to become stars,
  • neutral gas both within galaxies and in the space between them,
  • light-blocking dust and nebulous regions,
  • and ionized plasma, found mostly in the intergalactic medium.

All of these forms of normal matter — or matter originally made of the same things we are: protons, neutrons and electrons — do in fact contribute to what’s there, with gas and plasma in particular each contributing more than the sum total of all the stars in the Universe. But even adding all these components together only gets us up to about 15-to-17% of the total amount of matter we need to explain gravitation. For the rest of the motions that we see, we need a new form of matter that isn’t just different from protons, neutrons and electrons, but that doesn’t match up with any of the known particles in the Standard Model. We need some type of dark matter.

Images credit: X-ray: NASA/ CXC/UVic./A.Mahdavi et al. Optical/Lensing: CFHT/UVic./A.Mahdavi et al. (top left); X-ray: NASA/CXC/UCDavis/W.Dawson et al.; Optical: NASA/STScI/UCDavis/ W.Dawson et al. (top right); ESA/XMM-Newton/F. Gastaldello (INAF/IASF, Milano, Italy)/CFHTLS (bottom left); X-ray: NASA, ESA, CXC, M. Bradac (University of California, Santa Barbara), and S. Allen (Stanford University) (bottom right). These colliding galaxy clusters show a clear separation between the normal matter (in pink) and the gravitational effects (in blue).

A minority group of scientists favor not adding some unseen source of mass, but to rather modify the laws of gravitation instead. These models all have difficulties, including the inability to reproduce the full suite of observations, including individual galaxies moving within clusters, the cosmic microwave background, galaxy cluster collisions (above) the grand cosmic web or the patterns observed in the large-scale structure of the Universe. But there’s an important piece of evidence that points to the existence of dark matter that you might not expect: our very existence.

The Grand Canyon’s 23rd Annual Star Party in 2013. Image credit: NPS photo by Michael Quinn, under a cc by 2.0 generic license.

It might surprise you to learn that we don’t just need dark matter to explain astrophysical phenomena like galactic rotation, cluster motions and collisions, but to explain the origin of life itself!

To understand why, all you need to remember is that the Universe began from a hot, dense state — the hot Big Bang — where everything started off as a mostly uniform sea of individual, free, high-energy particles. As the Universe expands and cools, we can form protons, neutrons, and the lightest nuclei (hydrogen, deuterium, helium and a trace amount of lithium), but nothing else. It isn’t until tens or even hundreds of millions of years later that matter will collapse into dense enough regions to form stars and what will eventually become galaxies.

All of this will happen just fine, albeit differently in detail, whether there were plenty of dark matter or none at all. But in order to make the elements necessary for life in great abundance — elements like carbon, oxygen, nitrogen, phosphorous and sulphur — they need to be forged in the cores of the most massive stars in the Universe. They do us no good in there, though; in order to enable the creation of rocky planets, organic molecules and (eventually) life, they need to eject those heavier atoms back into the interstellar medium, where they can be recycled into future generations of stars. To do that, we need a supernova explosion.

Image credit: NASA / JPL-Caltech / O. Krause et al., combining Hubble (visible), Spitzer (IR) and Chandra (X-ray) data.

But we’ve observed these explosions in great detail, and in particular, we know how quickly this material gets ejected from the stars in their death throes: on the order of a thousand kilometers per second. (The Cas A supernova remnant has ejecta leaving it between a whopping 5,000 and 14,500 km/s!) While this may not sound like that big a number, especially compared to the speed of light, remember that our own star orbits the Milky Way at only some 220 km/s. In fact, if the Sun were to move even three times as fast as that, we’d find ourselves — today — escaping well beyond our galaxy’s gravitational pull.

A supernova remnant might see the fastest of its ejecta leave the luminous, star-based part of the galaxy, but combined with the intense gravitational pull of a diffuse, extended halo of dark matter, we’ll keep most of that mass inside our own galaxy. Over time, it will fall back towards the normal-matter-rich regions, form neutral, molecular clouds, and participate in subsequent generations of stars, planets, and more interesting,organic molecular combinations.

Image credit: ESO/L. Calçada, of the illustration of the dark matter halo surrounding the luminous disk of our galaxy.

But without the additional gravitation of a massive dark matter halo surrounding a galaxy, the overwhelming amount of material ejected from a supernova would escape from galaxies forever. It would wind up floating freely in the intergalactic medium, never to become incorporated into future generations of star systems. In a Universe without dark matter, we’d still have stars and galaxies, but the only planets would be gas giant worlds, with no rocky ones, no liquid water, and insufficient ingredients for life as we know it. Without the copious amounts of heavy elements provided by generations of massive stars, molecule-based life like us would never have come to be.

The Cigar Galaxy, M82, and its supergalactic winds that would drive all this matter out of the galaxy itself, were it not for dark matter. Image credit: NASA, ESA, The Hubble Heritage Team, (STScI / AURA); Acknowledgement: M. Mountain (STScI), P. Puxley (NSF), J. Gallagher (U. Wisconsin).

It’s only the presence of these massive dark matter halos, surrounding our galaxies, that allow the carbon-based life that took hold on Earth — or a planet like Earth, for that matter — to even be a possibility within our Universe. As we’ve come to understand what makes up our Universe and how it came to be the way it is, we’re left with one inescapable conclusion: dark matter is absolutely necessary for the origin of life. Without it, the chemistry that underlies it all — the heavy, complex elements, the ingredients necessary for biology in the first place, and the rocky planets that life takes hold on — could never have occurred at all.

This post first appeared at Forbes, and is brought to you ad-free by our Patreon supporters. Comment on our forum, & buy our first book: Beyond The Galaxy!


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