A low-mass planet candidate orbiting Proxima Centauri
advances.sciencemag.org
advances.sciencemag.org
Neat to find a planet, but it doesn't sound like one humans would want to have much to do with.
Still, there may be life that's happy with slow and heavy.
e.g. Wasn't Mars 'warm' for quite a long time and only became really cold once it lost most of its atmosphere due to its small mass?
Someone in the know correct me if I'm wrong, but I believe this is no longer the main theory, as solar wind ablation is too slow to make such a huge impact. I believe the popular explanation now is that geological reactions, i.e. gas reacting with rocks and being sequestered, played a larger part.
https://www.nasa.gov/press-release/nasas-maven-reveals-most-... "The new result reveals that solar wind and radiation were responsible for most of the atmospheric loss on Mars, and the depletion was enough to transform the Martian climate."
I looked through the paper and didn't see anything about the radius of the planet candidate. I suppose it's quite difficult to determine it from so far away. Is a value known? If so, that would obviously give a good idea about the local g.
You can also possibly find it via imaging, but even then, since you can't directly resolve it better than a point light source, you're making assumptions about albedo that lead to a wide dispersion in possible radii. High resolution optical imaging would require a telescope roughly 1-2km in diameter. Pretty tough... and because of the glare of the star, would be nearly impossible to image with an interferometric (i.e. non-filled-aperture) telescope since the light gather power would be so low. However, astronomers are incredibly clever at pulling data out of tiny points of light, so there may be some way.
I have a friend who used to work in a lab doing super-resolution microscopy (i.e. beating the diffraction limit by various means) for use with bio/medical applications. Some of the techniques he told me about have to do with more or less taking lots of data from many images and assembling it all into something meaningful. I suppose what you're describing as "pulling data out of tiny points of light" is kind of the same thing. It's just that the scale is different.
https://en.wikipedia.org/wiki/Proxima_Centauri_b
> The host star, with about an eighth of the mass of the Sun, has a habitable zone between ∼0.0423–0.0816 AU.
Set around a star that alternates between bright and dim, with a species that hibernates during the dim periods.
As to Venus... it is CLOSER to the Sun than Earth is, not farther.
https://en.wikipedia.org/wiki/Large_Ultraviolet_Optical_Infr...
The planet is ~10,000 times further away. Back of envelope puts the resolution at 250,000km. The earth is 12,000km in diameter. At 5.8x Earth mass and assuming similar density it would be a bit more than twice as wide and 25,000km diameter is easy to work with giving the planet a width of 1/10th of a "pixel". That's not nothing. In fact it's quite a lot relative to nothing. But it's still a long way from a well resolved image.
Oops. Forgot to apply the inverse square law. 10,000x further means resolving features of 10^10 greater area.
https://www.airspacemag.com/space/hibernation-for-space-voya...
An unmanned mission would probably have to go even faster, and probably has to be a bigger craft with better on-board power supply (with backups) and a big communications array. Maybe it would even need similar craft following it after a while to form a chain of communications relays on their way out.
Whats more likely to happen, is ~500 years of unmanned space exploration before we even think about sending people out there.
Luxury. Proxima Centauri is 40 trillion kilometers from here.
Sadly Proxima Centauri is 40,000 billion km away, so a bit further to go.
At 500m km/year our fastest probes would take 80,000 years to get there.
anyway given that their network was 100% switched, and "time to connect to a lightly-loaded remote host on a nearby network would actually largely be governed by the speed of light distance to the destination rather than by incidental router delays."
I'm thinking it doesn't apply to email delivery to Proxima Centauri or basically most places.
on edit: though with a long enough distance to the destination it would be pretty close to speed of light as the various times to respond etc. would be negligible.
Learn from Admiral Grace Hopper: https://www.youtube.com/watch?v=9eyFDBPk4Yw
The speed of light in fiber optic cable is about 2/3 the speed of light, which is why SpaceX's Starlink will have a potential latency advantage over oceanic fiber optics.
It also gives good perspective on what's being thrown away when you add a single ms of latency through a router or a display. 186 miles at the speed of light. Many on HN don't get this, but this is why cloud gaming is perfectly feasible if we're running with low latency displays and inputs, low distance to the edge compute, and few routing hops.