First ever recorded planetary engulfment

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SUMMARY

The discussion centers on NASA's James Webb Space Telescope's observations of the first recorded planetary engulfment event, revealing a hot accretion disk and a cooler dust cloud surrounding a star. The star, which is in the Sun's mass range but cooler and dimmer, did not expand to engulf the planet; instead, the planet's orbit decayed over time. The planet, approximately Jupiter-sized, experienced significant disruption due to grazing impacts with the stellar atmosphere, leading to ejecta formation and a ring structure. The findings are detailed in a journal article that emphasizes the model-dependent nature of the observations.

PREREQUISITES
  • NASA James Webb Space Telescope observations
  • Planetary engulfment phenomena
  • Stellar atmosphere interactions
  • Orbital decay mechanics
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  • Research the implications of hot accretion disks in stellar evolution
  • Study the mechanics of orbital decay in exoplanetary systems
  • Examine the modeling techniques used in astrophysical simulations
  • Explore the significance of stellar mass and temperature in planetary engulfment events
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Astronomers, astrophysicists, and researchers interested in planetary formation and stellar interactions will benefit from this discussion.

Tom.G
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"NASA’s James Webb Space Telescope’s observations of what is thought to be the first ever recorded planetary engulfment event revealed a hot accretion disk surrounding the star, with an expanding cloud of cooler dust enveloping the scene. Webb also revealed that the star did not swell to swallow the planet, but the planet’s orbit actually slowly decayed over time."

https://webbtelescope.org/contents/media/images/2025/117/01JR8HQ5MZTSG07EBWNBPYJADH

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1744519752098.png

Cheers,
Tom
 
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Can you talk us through in a bit more detail what is going on in #3 and #4?
 
More detail here. The planet was roughly Jupiter sized and heavily disrupted by repeated grazing impacts with the stellar atmosphere, which is what's supposed to be depicted in (3). The final impact flung ejecta into space, some of which settled into a ring (4).

Note that the images are artists' impressions, not Webb photos.

Original journal article (which I haven't read yet) here: https://iopscience.iop.org/article/10.3847/1538-4357/adb429
 
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The journal article says the star was in the Sun's mass range and the planet was probably less than ten times Jupiter's mass. The star appears to be cooler and dimmer than the Sun, so unlikely to have engulfed the planet as part of an expansion into a red giant. Hence it was probably orbital decay.

The rest of the paper seems to be a lot of modelling talk. There seem to be a good few assumptions feeding into the model, so I suspect the details are rather more model-dependent than the NASA article would suggest. Figure 9 (in section 4) is a less arty version of what their best fit says things look like pre- and post- event.
 
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