Missing low-metalicity Red Dwarves

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In summary, the conversation discusses the absence of low metallicity Red Dwarves in our part of the universe and their potential impact on the age of the universe. It is noted that these red dwarves do not produce any metals themselves and must have acquired them from earlier generations of stars. However, due to their long lifespans, there is no visual confirmation of red dwarves reaching the later stages of their evolution.
  • #1
RCopernicus
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Our local part of the universe is apparently missing Red Dwarves that have low metallicity. As near as I understand it, if the universe began 13.8 Billion years ago, there should still be plenty of these critters still around. Does anyone know how long it takes to make the heavier metals in Red Dwarves? I understand these misers can live to be trillions of years old, so could the absence of low metal Red Dwarves place a lower limit on the age of the universe (much like the way they do in globular clusters)?
 
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  • #2
It's not that metal-poor red dwarfs are missing, they are not. The missing ones are the metal-free ones.

Red dwarfs never pass into helium burning stage. Their fully convective interiors mix hydrogen and helium well, never forming a dense core. Even when the energy production stops after hydrogen is exhausted, the contracting core never reaches temperatures high enough to fuse helium.
So, they never fuse any metals themselves. All metal content must have come from earlier generations of more massive stars.
Note that the later stages of red dwarf evolution is a model without visual confirmation - red dwarfs have too long lifespans for any of them to have passed the hydrogen burning stage.
 

What are missing low-metalicity Red Dwarves?

Missing low-metalicity Red Dwarves are a type of star that is believed to have a lower amount of heavy elements in their composition compared to other stars of the same type. This makes them appear redder and fainter than other Red Dwarves.

Why are scientists interested in studying these missing low-metalicity Red Dwarves?

Scientists are interested in studying these missing low-metalicity Red Dwarves because they can provide valuable insights into the early stages of star formation and the evolution of galaxies. They may also help us understand the conditions necessary for life to develop on other planets.

How do scientists search for missing low-metalicity Red Dwarves?

Scientists use various methods to search for missing low-metalicity Red Dwarves, such as spectroscopy and photometry. These techniques allow them to analyze the chemical composition and brightness of stars to identify those with lower levels of heavy elements.

What are some potential explanations for the absence of these low-metalicity Red Dwarves?

There are several potential explanations for the absence of low-metalicity Red Dwarves, including their fragility and tendency to fuse hydrogen and helium quickly, making them difficult to detect. It is also possible that they were formed differently or have evolved at a different rate than other Red Dwarves.

What implications could the discovery of missing low-metalicity Red Dwarves have?

The discovery of missing low-metalicity Red Dwarves could have significant implications for our understanding of the universe and the formation of stars and galaxies. It could also provide new insights into the possibility of habitable planets and the potential for life elsewhere in the universe.

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