There is also the shroud of turin, which verifies Jesus in a new way than other evidences.
I've seen with my own eyes all the criminal idiocy being perpetrated by the chump and his henchmen. I have some real schadenfreude watching the MAGAts when they complain about the face-eating leopards coming for them.Quote from: Icarus on February 24, 2026, 11:17:32 PMI stumbled across this video that tells it like it is. We Americans, with our heads up our collective asses, have failed to pay attention. Our fearless leader with his imbecilic behavior has cost us dearly.
This is a 20 minute video that is realistic with bad news for us all.
QuoteEverybody knows that galaxies are large structures made of stars. That's a simple definition, and ignores the fact that galaxies also contain gas, dust, planets, moons, comets, asteroids, etc., and of course, dark matter. But one type of galaxy is mostly made of dark matter, and they're difficult to detect.
They're called dark galaxies, and they contain no stars, or only very few stars. Scientists have long theorized about their existence, which has remained hypothetical; they've found galaxies with low surface brightness, and they've found dark galaxy candidates. But new research has found the strongest candidate yet.
[. . .]
The candidate galaxy has been dubbed CDG-2, for Candidate Dark Galaxy 2. (CDG-1 is explained here.) CDG-2 is in the Perseus galaxy cluster about 300 million light-years away. The obvious question is, if it's so dark how was it detected?
It comes down to globular clusters (GC). Most galaxies have GCs. They're spherical groups of stars that are bound together gravitationally and can contain millions of stars. Around spiral galaxies like ours, they're mostly found in the galactic halo. Their origins are unclear, as is the role they play in the evolution of galaxies.
In this work, the researchers used the Hubble, the ESA's Euclid space telescope, and Japan's Subaru telescope. They searched for tight groupings of GCs that could indicate the presence of a galaxy. The Hubble found four closely-connected GCs in the Perseus cluster. The researchers then applied advanced statistical methods on data from the three telescopes that revealed a faint glow around the GCs. This glow is a strong indication that there's an underlying galaxy whose individual stars are too dim to resolve.
"This is the first galaxy detected solely through its globular cluster population," lead author Li said in a press release. "Under conservative assumptions, the four clusters represent the entire globular cluster population of CDG-2."
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QuoteAbstract:
Candidate Dark Galaxy-2 (CDG-2) is a potential dark galaxy consisting of four globular clusters (GCs) in the Perseus cluster, first identified in D. Li et al. through a sophisticated statistical method. The method searched for overdensities of GCs from a Hubble Space Telescope (HST) survey targeting Perseus.
Using the same HST images and new imaging data from the Euclid survey, we report the detection of extremely faint but significant diffuse emission around the four GCs of CDG-2. We thus have exceptionally strong evidence that CDG-2 is a galaxy.
This is the first galaxy detected purely through its GC population. Under the conservative assumption that the four GCs make up the entire GC population, preliminary analysis shows that CDG-2 has a total luminosity of LV,gal = 6.2 ± 3.0 × 106 L⊙ and a minimum GC luminosity of LV,GC = 1.03 ± 0.2 × 106 L⊙.
Our results indicate that CDG-2 is one of the faintest galaxies having associated GCs, while at least ∼16.6% of its light is contained in its GC population. This ratio is likely to be much higher (∼33%) if CDG-2 has a canonical GC luminosity function (GCLF). In addition, if the previously observed GC-to-halo mass relations apply to CDG-2, it would have a minimum dark matter halo mass fraction of 99.94% to 99.98%. If it has a canonical GCLF, then the dark matter halo mass fraction is ≳99.99%. Therefore, CDG-2 may be the most GC dominated galaxy and potentially one of the most dark matter dominated galaxies ever discovered.