Tag Archives: Kepler

Wishing and hoping doesn’t make it real

Credits: NASA/JPL-Caltech/T. Pyle

Credits: NASA/JPL-Caltech/T. Pyle

Look, I’m a space nut. It says so on the header up there. So when NASA announced the discovery of “Earth 2.0” I was as excited as the next space nut.

But let’s put this into context, people. What do we really KNOW about this planet, as FACT?

  • It’s in the constellation of Cygnus, 1,400 light years from Earth.
  • It orbits a star slightly larger than our sun, but of the same solar type.
  • The planet has an orbit of 385 Earth days.
  • It’s slightly larger than Earth.

And that’s it.

Let’s face it folks, astronomers have done a LOT of conjecturing on what amounts to a slight dip in the brightness of the star as the planet passes across its face. Science Alert has a rather good article about the discovery, with a little less hype.

We don’t know how long its day is. We don’t know the composition of its atmosphere. We might think it’s rocky but we can’t be certain. We certainly can’t suggest for a moment that its surface looks like the wonderful artist’s impression at top left. We should remember that Mars and Venus are in our sun’s habitable zone. Venus, in particular, could be seen as Earth’s twin – from a distance.

That said, (and to quote Captain Piett) it’s the best lead we’ve had. He was promoted to Admiral not long after that. Maybe we should send a star fleet to check Kepler 452b out. Maybe we’ll meet some Klingons.



What would you weigh on an exoplanet?

picture of an exoplanetI was reading an article from somebody, all enthusiastic about the exo-planets the Kepler probe keeps finding. They’re all many times larger than planet Earth even if they’re in the ‘Goldilocks’ zone. You know the one – not too close, not too far, just right. That is, a planet neither too close to its primary nor too far away, where liquid water could exist. My immediate reaction was ‘sure, but we’d weigh too much’.

Then I began to wonder how much more. I’m not a mathematician – never have been. In truth, I can’t add up to save my life. So I’m counting on you (ha ha) to correct me if I get this wrong.

I discovered this site http://www.exploratorium.edu/ronh/weight/ and learned that gravitational pull weakens by the radius squared. So let’s say you weighed 60kg on planet Earth. Planet Gliese 581g is estimated at 2.6 Earth masses and 1.4 Earth radii. So yes, you’re going to weigh more on Gliese 581g, but not 2.6 times as much. If I’ve got this right, the increased diameter of the planet means you’ll weigh about 1.3 times as much – so about 78kg. That’s certainly not a huge imposition. And all of a sudden, I’m bouncing in my chair, going oooh oooh.

Here’s some estimated figures about Gliese 581g, taken from this fascinating website http://phl.upr.edu/projects/habitable-exoplanets-catalog

Mass = 2.6 Earth Radius = 1.4 Earth  Temp = average surface temperature, so this place, at 10, is rather cooler than our 15 degrees (NASA’s figure from 2008), but the estimate of average temperature assumes an Earth-like atmosphere, which is a pretty big assumption. On the face of it the planet zips around its sun in a fraction of the time it takes ours, taking only 32 days as compared to 365. But that might not be the case, since the Gliesean day may be much longer than Earth’s. The figures don’t mention period of rotation, which I find a tad surprising. As a comparison, Venus’s ‘day” (the time it takes to rotate on its axis) is actually longer than its year (the time it takes to orbit the Sun.) (http://www.universetoday.com/14282/how-long-is-a-day-on-venus/)

So there you have it. I found out today that a candidate for Torreno (capital of the Coalition of Worlds in Morgan’s Choice) may be only 20.2 light years away. And with the shift drive of the future, that’ll be a place to add to your holiday plans.

Ain’t science grand?