So I'm not so sure yet why you think any of this means what you think it means. Best I can figure is that our galaxy has a higher mass than about 85% of all known galaxies. And it also has a metallicity thats higher than about 85% of known galaxies. This has been known for some time now. So of course, to find more galaxies, we have to look farther out into space. And almost all of the new galaxies we find will have less mass and less metal than the milky way.Rumraket wrote: ↑Aug 03, 2024 12:10 pm
That looks like a clear downward trend to me, yes.
There's a lot of uncertainty due to different methods, and another problem is the mass class also strongly affects metallicity. Ideally we'd want to tr ack metallicity with redshift for a specific galaxy mass class. They do this in Zahid et al. 2021:
Skærmbillede 2024-08-03 135747.png
Notice the mass-metallicity relation decreases obviously with redshift. The blue curve is redshift z=0.08, yellow curve (which is below blue) z=0.29, and so on, with the red curve (highest redshift) also showing lowest metallicities. So yes, there's a clear and obvious correlation when controlling for the mass-metallicity relation.
Yes, there's a mass-metallicity relation too, in addition to a redshift-metallicity relation. You need to control for mass, which the website you linked doesn't do.
I would say there's an obvious correlation for specific mass classes, yes.Johnny Blade wrote: ↑Aug 02, 2024 5:13 pm Do you still believe metallicity is a good way to determine age?
So considering we have observed at the most, 5% of the knowable universe (I don't know where they get that number from. Maybe you can help me.) and further considering the morphology of galaxies we find (galaxy bars ect), It looks like the trend is that we will just find all kinds of different galaxies, everywhere, relative to our own high mass and high metal galaxy.