Nautilus coven.
Allegedly 876 (a suspicious number) ft - a bit less than 300m - down in the Pacific near Palau.
Lighting is suspiciously bright.
Original pic
My reading.
Somewhere to write my notes and comments. Typically, these are bits of science news that tickle my fancy.
It has been a while since I posted anything, and the potential submissions have been piling up.
Arxiv Ref |
Title |
Comments |
2108.09868 |
The Orbit of Planet Nine |
Probably the most interesting to the general reader. |
2108.07207 |
(216) Kleopatra, a low density critically rotating M-type asteroid |
Partly the “M-class” (no, not Star Trek), but in itself interesting because quite large asteroids can get spun up to the point of shedding matter from their extremities. |
2108.03343 |
On the Need for a Classification System for Consistent Characterization of the Composition of Planetary Bodies |
An actual planet classification. |
2108.03323 |
Warm terrestrial planet with half the mass of Venus transiting a nearby star |
New competitor for lightest planet known – check on Exoplanets.org |
2108.05321 |
Ross 19B: An Extremely Cold Companion Discovered via the Backyard Worlds: Planet 9 Citizen Science Project |
Its the citizen science that is most interesting. |
2108.01422 |
The interior of hairy black holes in standard model physics |
Funny phrase – save it for next time someone is whinging about Uranus. |
2108.01471 |
What’s inside a hairy black hole in massive gravity |
ditto |
2108.01783 |
Comment on “Observation of a Neutrino Burst from the Supernova SN1987A” |
There was a 7.3 second gap during the records of neutrinos from SN1987A at Kamiokande. This is suggested to be a hardware eror, when the tape staging recorder experiences a write error and performs a rewind-reset, which takes about this period of time. |
Ever since the demotion of Jupiter, any mention of "Planet Nine" invariably attracts a swarm of comments about how, for some people, "Planet Nine will always be 134340 Pluto. Well, that battle has been fought and lost, and @plutokiller (Professor Mike Brown of Caltech, USA) himself has moved on to trying to find a new Planet Nine. In 2016 an analysis of the orbits of the largest, most distant "minor bodies" of the Solar system suggested that there may be a large planet "out there", controlling the distribution of these (relatively) large, distant bodies orbits, and from that inferring where they think their suggested planet would be seen on the sky.
Such efforts have a patchy history. Certainly LeVerrier is famous for predicting the position of Neptune from irregularities in the orbit of Uranus (cue whooping from the peanut gallery), but equally certainly he was working with an inaccurate data for the masses of solar system bodies (Uranus, particularly), and his result was correct by luck, not judgement. Similarly, the calculations which led to the discovery of 134340 Pluto were also based on inaccurate mass data leaving the mass of 134340 Pluto uncertain between the mass of Earth and "very small". The fly-by of a spacecraft - Voyager 2 - greatly improved the measurement of Uranus's mass, which is crucial to understanding the motions of the rest of the Solar system.
Since Brown (and others) started discovering multiple bodies of mass comparable to that of 134340 Pluto, orbiting in the same region of space, the identity of 134340 Pluto as a planet has been challenged, resulting in it's demotion to a "dwarf planet" in 2006. But since then, the discovery of more, and more distant, dwarf planets (including by Brown) has led to suggestions that they may hint at the presence of something big, "out there". Which Brown and colleagues have been looking for for several years, securing observing time on very large telescopes to carry out this work.
Their current best estimate of properties for Planet Nine is mass 6.2 (average: spread 8.4 - 4.9) Earth masses ; semi-major axis 380 (520- 300) AU ; inclination 16 (21 - 11) degrees and an argument of perihelion of 300 (440 - 240) degrees (centred on Capricorn, but with a wide spread).
Hopefully they'll find it soon, because not finding it would only prove that they were looking in the wrong place at the wrong times, not that it doesn't exist.
This one posted 2021-09-02
A paper just published on Arxiv, the astronomy/ physics/ computing/ mathematics preprint service, describes studies into old astronomical data sets, to prepare the ground for the "transient" phenomena which will be discovered by new "repeated survey" telescopes. These will photograph the whole sky every few days, capturing novae and supernovae, many new Solar system bodies, the new "mega-constellations" of thousands of satellites, and other, more surprising "transient" phenomena.
In the early 1950s the then-new "200 inch" Hale telescope at Mt Palomar was employed in performing a sky survey. They would take a plate (literally, a glass plate ; this was long before electronic image capture) with a blue-sensitive emulsion, then a plate with a red-sensitive emulsion ; six days later, another red plate covered the same area (by planned overlap). The middle red plate showed a cluster of 9 objects, covering about a tenth of the full Moon's apparent size, which weren't visible in the previous blue plate, nor in the subsequent red plate. The simplest astronomical explanation is that 9 objects of red colour appeared and disappeared in that time interval.
As astronomers get more short-interval surveying of the sky, they get a better idea of how often such "transients" occur. Individual transients (novae, unidentified Solar system bodies, etc) are not, themselves, rare. But nine, in such a small area, in such a short time period - that is rare.
A sceptic's first question would be - is the data good? Photographic plates are a mature technology - and were around a century old at the time of taking. Nobody knows of a similar "contamination" process. Millions of plates have been scanned into computers after the glassware was replaced with CCD detectors - again, nobody has found a similar set of contamination marks. Ideas such as grains of dust from the Alamagordo atomic tests getting onto the plates (and being washed off in the processing) were considered, but it is very unlikely that no other plates for the same manufacturer show similar defects. Human events (matches producing "flares" in spectroscopic observations ; the infamous "Fast Radio Burst" microwave oven) were considered, such as an astronomer with hayfever spraying the plate with snot droplets. But again, why haven't comparable artefacts been found on other plates - and people have looked, digitally, for them! Water drops and processing chemical streaks have characteristic sizes, which these images don't.
A fragmenting asteroid ("small body") was considered. But that would leave images substantially elongated by the Earth's motion - and only one of the 9 "transients" showed signs of elongation. Some astronomers used to refer to asteroids as "the vermin of the skies" referring to their common occurrence on the sky - invariably through the middle of what you were really trying to photograph. The term is being re-purposed for satellite megaconstellations.
What about a meteor fragmenting in the atmosphere above the telescope? They take too long, and produce even longer streaks than asteroids. They are photographed often enough to be well understood, and this image isn't one of those.
A satellite might produce a short enough "glint" of reflected sunlight. But ... the first satellite was launched 7 years after this image. Unless the launch records from Area 51 say differently.
One event, with 8 reflections from some nearby objects, could work. But with the plate exposure being 50 minutes, the maximum spacing of the reflecting objects is about 30 light minutes, and the size of the spread means the object is about 0.02 light years away. Comfortably beyond the Voyager probes, launched over 20 years later. Unless the launch records from Area 51 say differently.
The obvious next step is to look at existing images of the area taken with newer technology. That has been done. The Pan-STARRS survey (2010 to "continuing" ; to 3.4 magnitudes dimmer than the plates managed - a factor of about 23-fold in brightness) saw nothing there. The Sloan Digital Sky Survey (SDSS, 2000 to "continuing"), to 16-fold dimmer than the plates, saw nothing there.
To mis-quote Capt.Brody [no, Quint!], "We're gonna need a bigger telescope!" And that is what this report is about. Using the GTC (Gran Telescopio Canaria, 10.4m, ~409in) they photographed the region to a brightness (dimness) of 250-fold compared to the original plates. And they found a number of matches. That's not unexpected : the astronomers estimate the odds of getting such matches by chance as about 17% - far from impossible, but not terribly likely.
Still, nobody knows what there objects were (or even if the 1950 observation was real)
(The authors also consider the possibility that in the 70 years between observations, the original objects have drifted out of the field of study - in itself, that would mark them as likely outer Kuiper Belt objects, or Oort Cloud objects. In which case, the question of the simultaneous movement of 9 close objects remains a question. Cue the "I'm not saying it was aliens, but ..." video clip.)
This is a first draft. I'll post it to Slashdot after editing it down a bit.
G. Anglada-Escud ́e et al, https://arxiv.org/pdf/1406.0818.pdf with a small football team of co-authors.
I noticed the paper while searching for something else on Arxiv ; the title hooked me, but on second reading I'm realising it's old (2014) work.
Kapteyn's Star is one of the closest stars to the Solar system (well known) ; it's a red dwarf with a parallax of 0.25 arcsec (4 parsecs). It is considered a halo star - a star passing through the Milky Way's disc, but generally residing in the galaxy's halo). Proper motion just under 9 mas/year. Discovered about 1897 in compilation of the Cape photographic Durchmusterung. It has a low spectroscopic rotational speed (v.sin(i) <~3km/s) and low metallicity. It is considered a pretty ancient star, and possibly derived from the Omega Centaurus galaxy's halo into the Milky Way's halo, stripped off during the collision.
Located in Pictor, southern hemisphere. It moves, relatively quickly.
Between 1999 and 2013, using several devices, a sequence of spectra were taken and yield a periodic drift with two period peaks of 121 and 48.6 days.
With a low-mass primary, and relatively large planets (4.8 and 7.0 Msin(i)_earth) the orbits seem stable on the 10 Gyr timescale (appropriate for a merger star).
This work has been challenged several times, but seems to survive it reasonably well.
Yet another provocative paper emerges onto Arxiv from Harvard's Lingam and Loeb.
Today they estimate the volume of space occupied by habitable zones (regions where liquid water is stable) in brown dwarf not-quite stars. They find that it could be orders of magnitude greater than the volume in the atmospheres of Earth-size planets.
Brown dwarfs are masses of gas which are too small to sustain nuclear fusion (so, they're not stars), but can have a brief period of fusion of deuterium or lithium shortly after formation (so they're not planets ; the boundary size is under debate). After this burst of energy, they slowly cool, for billions of years. This leads to a large volume of the star's outer body — or atmosphere — with potentially attractive temperature and pressure. If the brown dwarf is orbiting with a larger star, there may be enough light to allow photosynthesis. Supply of chemicals is uncertain, but not impossible.
While this paper is speculative, the prospects for detecting such life by spectroscopy are plausible with observational instruments being designed at the moment.
Previous work on abiogenesis and the origin(s) of life has speculated that life could persist in the atmospheres of Venus and Jupiter, using comparable pressure-temperature arguments. In this respect, the proposal is more conventional.