Gardening on Worlds with Two Suns

Life on Other Worlds Could Well Look VERY Different

Black plants on a world with two Suns. Courtesy Jack O' Malley, University of St. Andrews.

Imagine if Earth had two Suns in its sky, similar to the otherworldly scenes we recall from movies like Star Wars. What would our gardens look like as we whirled around in a binary star system?

According to Jack O’Malley, a scientist at the University of St. Andrews in Scotland, it’s very possible that our gardens would NOT be the colorful delights we know today. They might very well be teeming with plants that are distinctly black or grey. He presented his ideas to the National Astronomy meeting of the Royal Astronomical Society this week.

How could strange darkened plants happen?  To understand the idea behind these science-fiction type blackish-grey plants that could flourish under the light of binary stars, we have to look at the process that makes green plants here on Earth: photosynthesis.  It provides the main energy source for plants, and of course for the animals that eat them. Photosynthesis is what a plant does to convert sunlight into energy.  On Earth, our plants are attuned to sunlight for their photosynthetic activities — and in particular, the color of the light streaming from our nearest star.

However, if those plants had evolved on an Earth with TWO Suns, they’d have twice as many light sources to choose from.  It’s entirely possible that they could use the light from both stars, or, perhaps some plants might evolve with a preference for the light from only one of the stars, particularly if they are exposed mostly to one of the stars for longer periods of time.

Think about this:  the temperature of a star determines its color, which is the color that photosynthesis relies on to do its job.  The star colors could then also affect the colors of the plants that are using photosythesis for their energy sources.  So, star color, availability of light, and the chance to utilize multiple star sources are big factors in the colors of the plants that could evolve on worlds blessed with more than one star.

This is an interesting thought experiment — and one that O’Malley and his PhD supervisors — are doing to figure out the potential for finding photosynthetic life on planets around other stars.  In particular, they are looking at the factors for such life in multi-star systems with different combinations of Sun-like stars and red dwarfs. Sun-like stars are known to host exoplanets and red dwarfs are the most common type of star in the Milky Way Galaxy. They are often found in multi-star systems, and are old and stable enough for life to have evolved.

In M star radiation habitats, vegetation may have more photosynthetic pigments in order to make use of a fuller range of wavelengths, giving them a ‘black’ appearance. These are terrestrial examples of a dark plants (and flowers).

O’Malley and his team are running simulations that consider Earth-like planets orbiting two stars close together or maybe are in orbit around one of two widely separated stars. Their simulations seem to show that planets in multi-star systems may host exotic forms of the more familiar plants we see on Earth.  If this is true, then they would look much different from what we grow here.

For example, explorers collecting plants growing in the light of dim red dwarf suns would find black-looking leaves and strange-colored flowers. Those plants would be absorbing light from across the entire visible wavelength range.  They’d have to use as much of the available light as possible in order to keep the photosynthesis process going.

It’s also possible that they could use infrared or ultraviolet radiation to drive photosynthesis. For planets orbiting two stars that are like our own, harmful radiation from intense stellar flares could lead to plants that develop their own ultraviolet-blocking sun-screens, or photosynthesizing microorganisms that could move in response to a sudden flare.

Someday, astronomers will find the chemical signatures of plants in the atmospheres of distant planets.  From the light output of their stars and the chemistry lesson we get from those worlds, perhaps we’ll finally be able to “see”  what gardens on the surfaces of faraway worlds will be like.  Maybe we’ll find out that the worlds we imagine in our science fiction movies are not even half as “weird” and different as the real worlds that lie out there around nearby stars.

From Starbirth to Stardeath…

… and Back Again

This picture of the star formation region NGC 3582 was taken using the Wide Field Imager at ESO's La Silla Observatory in Chile. The image reveals giant loops of gas ejected by dying stars that bear a striking resemblance to solar prominences. Courtesy ESO, Digitized Sky Survey 2 and Joe DePasquale

The process of stardeath is one of those events that is not just the end of a star’s life, but possibly the beginning of another one’s existence.  In some regions of our galaxy (and in many other galaxies), the explosion of a massive star in an event called a supernova, not only ejects material from the star that will eventually be recycled into other stars. It also sends shock waves through space that can compress nearby nebulae (clouds of gas and dust). That “ripple effect” starts the nebula down the path to star formation as the material begins to coalesce, heat up, and eventually “turn on” in the process of star birth. If the birth cloud has enough heavy elements to form planets, and the conditions are right, the stellar babies could also be born with worlds of their own.  This is what happened to create our Sun and planets, more than 4.5 billion years ago.

The image above is a scene of violent stellar destruction, lit up by strong ionizing radiation (UV light) from nearby newborn stars. It’s a star-forming region in the Milky Way called RCW 57, and the nebula itself (the glowing, loop-filled cloud of gas and dust) is called NGC 3582.  Some of the stars forming in regions like NGC 3582 are much heavier than the Sun. These monster stars emit energy at prodigious rates and have very short lives that end in supernova explosions. The material ejected from these dramatic events creates bubbles in the surrounding gas and dust. This is the probable cause of the loops visible in this picture. When the stellar beacons that are heating up this cloud start to die they will also send out clouds of gas and dust like these, and the forces of their deaths may well send the clouds back through a cycle of star birth, creating new stars that will light up the death-clouds of their forebears.

The image was processed by the European Southern Observatory (ESO),  using observational data identified by Joe DePasquale, from the United States, who participated in ESO’s Hidden Treasures 2010 astrophotography competition. The activity was organised by ESO in October–November 2010, for everyone who enjoys making beautiful images of the night sky using astronomical data obtained using professional telescopes.