NASA's New Horizons Discovered a Large Surprise in the Kuiper Belt
sciencealert.com
sciencealert.com
> Data from the New Horizons probe as it sails serenely through the Kuiper Belt hints at unexpected levels of particles where dust ought to be thinning out, suggesting the donut-shaped field extends significantly farther from the Sun than previous estimates suggest.
Isn't this -- finding out that what we didn't know is far greater than we realized -- typical in any field of science or even profession? When I was 5 years into my programming career I had the cocky feeling of knowing everything. 20 years later I feel more like I know nothing because every day I'm discovering more about my profession that I never even knew existed (thank you, HN!).
Yet even classical mechanics holds some surprising mysteries, such as how bicycles self-stabilize [1].
[1] https://www.aip.org/history-programs/niels-bohr-library/ex-l...
> But amazingly, even for a riderless bike science currently doesn't what it IS about the special combinations of variables that enables a bike to stay up on its own. We just know that some combinations work and others don't.
> Astronomers using the Webb telescope discovered complex organic molecules in a galaxy located over 12 billion light-years away.
https://edition.cnn.com/2023/06/06/world/webb-telescope-dist...
To me, this sort of claim is beyond embarrassing. How can we possibly reconcile knowing about organic molecules, and not know about our backyard.
The reason? Light.
Webb was able to detect the absorption characteristics of PAH (the organic molecules in question) from a distance because there was light from behind illuminating it (and it was absorbing only parts of that light). We know roughly what the light being emitted "looks like" so we are able to extrapolate based on what light isn't present what is in that region. And it wasn't as if individual particles were being seen but rather there is a sufficient density of these molecules spread out in the regions where they were detected that when the light passed through them, it was noticeable from a distance. Kinda like how you can't see the air but you can see the sky.
I'm probably not explaining it super well but it's the phenomenon where you can see the gaps in between up close but from far away it looks like one big blob.
But point being Webb was able to make that discovery because those molecules basically had a giant lamp shining on them from behind and we the observer are at such a distance that we can see all the little bits of information that would otherwise be indistinguishable from noise all together at once.
Now comparatively, the stuff out in the far reaches of our solar system have a lamp shining on them (our sun) but we are on the wrong side to be able to see the shadows that are cast. So unfortunately that means if we want to learn about this blindspot of ours we have to physically go out there to see it.
In general I would expect this to be a case where we didn't expect something but once we look closer we discover it fits with our current known physics - this is the majority of "interesting" discoveries. However once in a while we discover something unknown.
And we'd know if there was another gas giant in the kuiper belt. I couldn't find estimates on how much mass is in the oort cloud, but probably not enough to form a orbit with enough mass to make a gas giant.
Edit: Just found the wikipedia section on the mass of the oort cloud. Roughly estimated at 5 earth masses. Neptune, which isn't quite massive enough to be a gaseous planet, is 17 earth masses. Saturn, our smaller gas giant is 95 earth masses
The temperature is not related to holding on to the helium, but to its density for higher efficiency farming.
It probably has a better title too, considering the more clickbaity title above.
> New data (Figure 3) at larger heliocentric distances show that the SDC-reported dust f l uxes, out to 55 au, remained higher than current models expected. Each of the three physical phenomena: optical properties and radiation pressure (Arnold et al. 2019); compositional variation between silicates and ice (Grigorieva et al. 2007); and a further reaching than currently identif i ed distribution of dust-producing bodies in the solar system (Fraser et al. 2023), may contribute to the data/model deviation.