- #1
Ken G
Gold Member
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TL;DR Summary: It seems inevitable that internet searches to answer astronomy questions will someday involve AI assistance. Is ChatGPT reliable enough yet for that, or still nowhere close?
The issue for me at this point is how to distinguish the errors ChatGPT currently makes, versus the errors that are widespread on the internet that an unwary user could fall victim to even without AI assistance. Has anyone experimented with ChatGPT to see if it is better than simply using search engines to answer astronomy questions? Personally, I've only tested questions that I know regular internet searches will likely give wrong answers, and ChatGPT gives all those same wrong answers (questions like if fusion is necessary for hydrostatic equilibrium, or why are higher mass main-sequence stars more luminous, ChatGPT would have no hope of getting those right given all the misinformation out there). What happens if ChatGPT is used instead of, say, posting to a forum like this? I'll start with an example, using a question on this forum:
Me:
Could a brown dwarf ever have been a T Tauri star in its past?
ChatGPT:
Yes, a brown dwarf could have been a T Tauri star in its past.
T Tauri stars are young, pre-main-sequence stars that are still undergoing gravitational contraction and have not yet reached the point of sustained fusion in their cores. Brown dwarfs, on the other hand, are objects that are too small to sustain fusion in their cores, and they emit most of their energy as heat from their contracting cores.
However, T Tauri stars and brown dwarfs are thought to be similar objects in the early stages of their formation, and they may share many of the same physical characteristics. In fact, some brown dwarfs have been observed to have disks of gas and dust around them, similar to those seen around T Tauri stars, which suggests that they may have formed through a similar process.
Therefore, it's possible that a brown dwarf could have been a T Tauri star in its past, when it was still undergoing gravitational contraction and had not yet reached the point of sustained fusion in its core. Over time, as the brown dwarf continued to contract, it would have become denser and hotter, until it reached a stable state where it could no longer sustain fusion in its core.
So a decent answer in some ways, though technically wrong, and with a very weird ending!
The issue for me at this point is how to distinguish the errors ChatGPT currently makes, versus the errors that are widespread on the internet that an unwary user could fall victim to even without AI assistance. Has anyone experimented with ChatGPT to see if it is better than simply using search engines to answer astronomy questions? Personally, I've only tested questions that I know regular internet searches will likely give wrong answers, and ChatGPT gives all those same wrong answers (questions like if fusion is necessary for hydrostatic equilibrium, or why are higher mass main-sequence stars more luminous, ChatGPT would have no hope of getting those right given all the misinformation out there). What happens if ChatGPT is used instead of, say, posting to a forum like this? I'll start with an example, using a question on this forum:
Me:
Could a brown dwarf ever have been a T Tauri star in its past?
ChatGPT:
Yes, a brown dwarf could have been a T Tauri star in its past.
T Tauri stars are young, pre-main-sequence stars that are still undergoing gravitational contraction and have not yet reached the point of sustained fusion in their cores. Brown dwarfs, on the other hand, are objects that are too small to sustain fusion in their cores, and they emit most of their energy as heat from their contracting cores.
However, T Tauri stars and brown dwarfs are thought to be similar objects in the early stages of their formation, and they may share many of the same physical characteristics. In fact, some brown dwarfs have been observed to have disks of gas and dust around them, similar to those seen around T Tauri stars, which suggests that they may have formed through a similar process.
Therefore, it's possible that a brown dwarf could have been a T Tauri star in its past, when it was still undergoing gravitational contraction and had not yet reached the point of sustained fusion in its core. Over time, as the brown dwarf continued to contract, it would have become denser and hotter, until it reached a stable state where it could no longer sustain fusion in its core.
So a decent answer in some ways, though technically wrong, and with a very weird ending!