Wasp-76b is a planet where it rains iron

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    Iron Planet
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Discussion Overview

The discussion revolves around the exoplanet Wasp-76b, particularly its extreme weather phenomena where it is suggested to rain iron due to high temperatures on its dayside and cooler conditions on its nightside. Participants explore the implications of this phenomenon, including atmospheric composition and the physical characteristics of the planet.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants note that Wasp-76b's dayside temperatures exceed 2,400°C, which could vaporize metals, while the nightside is significantly cooler, allowing for condensation and precipitation of iron.
  • There is speculation about the existence of a ring of iron at the boundary between the daylight and darkside, and how this rain might manifest as fog or drizzle.
  • Questions arise regarding the potential atmospheric composition of Wasp-76b, with some suggesting it could be rich in noble gases due to the extreme temperatures.
  • Participants discuss the distances of Wasp-76b from Earth, with conflicting information about its distance in light-years and parsecs, leading to confusion about its exact location.
  • Some participants humorously reference other fictional planets with extreme weather, such as "Sol-3," where it rains molten hydrogen ash, drawing parallels to the exotic nature of Wasp-76b's conditions.
  • There are discussions about the implications of tidal locking on Wasp-76b and whether iron would accumulate on the cold side or be transported back to the hot side.
  • Concerns are raised about the availability of oxygen in the atmosphere and how it could be detected through spectroscopy.

Areas of Agreement / Disagreement

Participants express a range of views on the atmospheric conditions and physical characteristics of Wasp-76b, with no clear consensus on the specifics of its environment or the implications of its weather phenomena. Multiple competing ideas and uncertainties remain present throughout the discussion.

Contextual Notes

There are unresolved questions regarding the atmospheric composition, the mechanisms of iron transport, and the exact distances of Wasp-76b from Earth, which depend on various sources and may contain errors or differing interpretations.

  • #31
TaurusSteve said:
Summary:: A planet where it rains iron!

https://www.bbc.co.uk/news/science-environment-51828871
"Wasp-76b, as it's known, orbits so close into its host star, its dayside temperatures exceed 2,400C - hot enough to vaporise metals.

Can we really be sure this is the case? In other words, is the result ironclad?

Because,
BBC article said:
Using the Espresso spectrometer, the scientists detected a strong iron vapour signature at the evening frontier, or terminator, where the day on Wasp-76b transitions to night.

My critique:

Using a spectrometer designed to measure the components of caffeine does seem suspect.
There could have been caffeine residual in the spectrometer.
And espresso is strong, so the person doing the measurements could have had shaky hands.
 
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  • #33
Ian J Miller said:
Weird! If it rained iron on the cold side, one might expect sooner or later all the iron would be there if the planet is tidally locked, so maybe despite its closeness, it isn't. Alternatively, deep down, there must be some means of transporting it back to the hot side. As an aside, deep down, the pressure is immense and iron might be expected to be solid. I suspect there is a lot we don't know about this world.
The same neutral iron signatures were detected in WASP-121b too, therefore occurrence must be pretty common. Interesting, both WASP-76b and WASP-121b are orbiting F-class stars. It may be coincidence or consequence of neutral iron circulation requiring abundant ultraviolet irradiation.
Regarding transport of iron, i suspect both WASP-121b and WASP-76b could have rapidly super-rotating atmospheres with complex clouds, similar to Venus. In this case, ultraviolet-rich sunlight will result in strong temperature inversion at subsolar point (tropopause at pretty high pressure). And strong wind at high enough pressure may prevent a layer of "iron clouds" from settling. If my hypothesis is correct, these planets will not have iron rain - only iron haze/fog will be present.
 
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  • #34
Gosh! A planet that rains nuts, bolts, washers and nails!
 
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  • #35
sysprog said:
maybe it's raining aluminum on one side and aluminium on the other
Ian J Miller said:
Aluminium is sufficiently active that it would only exist as the oxide. Iron oxide would be reduced to iron by the hot hydrogen, but aluminium should remain as an oxide
If there would be oxidized aluminium falling from the sky. Would it not be more accurate to describe it as snowing? Oxidized aluminium is alumina a fine white powder.
 
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  • #36
Nick-stg said:
If there would be oxidized aluminium falling from the sky. Would it not be more accurate to describe it as snowing? Oxidized aluminium is alumina a fine white powder.
I imagine that you know that what we in the US call aluminum oxide (as distinguished from what the Brits call 'aluminium' oxide -- same stuff; different spelling), is used as a pigment in some white paints, so maybe yes, 'snowing' might be more apropos than 'raining'. I was joking about a small difference between US English and Brit English regarding the orthography of the term for the element.

I think that it's not entirely Humphrey Davy's fault, although apparently he vacillated on the spelling of the name for the element that he had identified; it was the people pushing the agenda of 'ium' ending for names of elements instead of acceding to the wishes of the person who had isolated and characterized the element -- their fault too -- from https://www.thoughtco.com/aluminum-or-aluminium-3980635:
In 1808, Sir Humphry Davy identified the existence of the metal in alum, which he at first named "alumium" and later "aluminum." Davy proposed the name aluminum when referring to the element in his 1812 book Elements of Chemical Philosophy, despite his previous use of "alumium." The official name "aluminium" was adopted to conform with the -ium names of most other elements. The 1828 Webster's Dictionary used the "aluminum" spelling, which it maintained in later editions. In 1925, the American Chemical Society (ACS) decided to go from aluminium back to the original aluminum, putting the United States in the "aluminum" group. In recent years, the IUPAC had identified "aluminium" as the proper spelling, but it didn't catch on in North America, since the ACS used aluminum. The IUPAC periodic table presently lists both spellings and says both words are perfectly acceptable.​

I suppose that if ##\rm {Al_2O_3}## is descending from the sky, whether to call it rain or snow should depend at least in part on the temperature.
 
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  • #37
sysprog said:
I suppose that if Al2O3Al2O3\rm {Al_2O_3} is descending from the sky, whether to cal it rain or snow should depend at least in part on the temperature.

TaurusSteve said:
its dayside temperatures exceed 2,400C

According to wikipedia alumina has a melting temp 2072C. Darn! I missed by 300C.

I knew the melting point was high. I guess the strategy of post first, check facts later has failed me again.
 
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  • #38
Nick-stg said:
I guess the strategy of post first, check facts later has failed me again.
No way man 'ready; fire; aim' always works for me . . .
 
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  • #39
This will be Earth's fate about 6 billion years hence.
 
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  • #41
sysprog said:
I think that @russ_watters, if he's not too busy stargazing :wink: , might be able to answer that question better than I am able to answer it.
Isn't that Russ_dihydrogen_monoxide (with t added to make it a better drink) ?
 
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  • #42
trurle said:
Warning! The "iron rain" on WASP-76 b is now refuted. Seems the confusion happened due light pollution from nearby star.
https://arxiv.org/pdf/2005.02374.pdf
Reading this through it hasn't been refuted per say since refuted is a strong word. Here there still seems to be a signal but it is just below the threshold for detection using the given spectrometer and telescope without the contamination of the systems K type companion star. There also is still strong signals of TiO and water but the Vanadium oxide signature has disappeared. I feel we need to be careful not to over-sensationalize or make preemptive claims. This is the sort of things that leads to confusion among the general public and results in their errosion of confidence in science as it "contradicts itself" I feel the uncertainty of observations need to be better conveyed so that things in that grey area are described as such.
 
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