The Research Behind Elyria

Cosmic Perspectives:
Galaxies, Consciousness & Spirituality

A research reference on galaxy counts, JWST discoveries, fine-tuning, consciousness, divinity, indigenous star traditions, Elyrian doctrine, the epigenetic science of oxygen and breath, and the brain as a complex system.

Updated November 2026 12 Sections 147 Sources Section 1 free to read

Total Estimated Number of Galaxies

Astronomers estimate that the observable universe contains on the order of hundreds of billions to trillions of galaxies. Early Hubble Deep Field observations in the 1990s suggested roughly 100–200 billion galaxies. However, a landmark 2016 analysis of deep-sky surveys led by Christopher Conselice concluded this figure was at least ten times too low — implying on the order of 2 trillion galaxies in the observable universe.

Current Estimate Range

~100B
Low end of early
Hubble estimates
~200B
Original Hubble Deep
Field estimate
~2T
Conselice 2016
(modeled upper)
>Several T
Speculative (ultra-faint
dwarf galaxies)

The dramatic 2016 revision came from inferring many faint, distant galaxies that current telescopes cannot directly observe. The study estimated 90% of galaxies are too dim and far to be seen with present technology.

Nov 2026 A separate line of evidence comes from NASA's New Horizons probe, which can measure the faint background glow of the sky far from the scattered sunlight of the inner solar system. Its 2021 measurement was initially reported as being in tension with the 2-trillion figure, but NASA has since issued a correction: the New Horizons data do not constrain the total number of galaxies; they constrain the total amount of ultraviolet and optical light that all galaxies emit.51 A refined 2024 analysis (Postman et al., The Astrophysical Journal) measured this cosmic optical background at roughly 11 nW m⁻² sr⁻¹ and found it consistent with the light expected from the galaxies thought to have formed since the Big Bang, with no strong sign of an unknown extra light source.52 In other words, the background light is accounted for by known galaxy populations — but because faint dwarf galaxies contribute very little light, this measurement cannot by itself settle whether there are hundreds of billions or trillions of them.

Key Fact — Hubble Ultra Deep Field

The HUDF image, assembled from a ~1-million-second exposure in 2003–2004, revealed approximately 10,000 galaxies in a tiny patch of sky covering roughly 1/13,000,000th of the total sky area. Telescope surveys of such deep fields let astronomers count galaxies in a small sample area and extrapolate across the full sky — one of the primary tools for estimating the universe's total galaxy population.

Modern sources typically quote a wide range: "somewhere between 100 billion and 2 trillion" in the observable universe. Note also that the observable universe is only a fraction of the full universe, whose total extent is unknown.

Nov 2026 The next census is underway. Alongside JWST, three wide-area surveys designed to map galaxies by the billion are now operating. The Vera C. Rubin Observatory officially began its ten-year Legacy Survey of Space and Time on 30 June 2026.53 ESA's Euclid mission is scheduled to issue its first major data release (DR1-Foundation, about 1,900 square degrees of sky) in November 2026, with the full DR1 following in mid-2027.54 NASA's Nancy Grace Roman Space Telescope launched on 30 August 2026 and is due to begin science operations in early 2027.55,56 None of these will count every galaxy, but together they will sharply improve the deep-field statistics on which every total-count extrapolation rests.

Why the Number Keeps Changing

The count is not a single measurement — it is a model-dependent inference. When Conselice's team reached 2 trillion in 2016, they were not directly observing that many galaxies; they were extrapolating from what Hubble could see and modeling the dark, undetected population. Each revision in our cosmological models or observational tools produces a new number.

Nov 2026 JWST is already complicating things further: at z ≈ 10–14 it is finding far more luminous galaxies than pre-launch models predicted.13 But the effect on the total count should not be overstated. These bright objects are a tiny fraction of all galaxies, and the total is dominated by faint dwarfs that JWST still cannot fully census. A large 2026 search across more than 0.6 square degrees of JWST imaging (McLeod et al., preprint) also found that galaxy abundance falls off steeply beyond z ≈ 12, with a dearth of candidates beyond z ≈ 14.5 — suggesting the early excess has limits.57 Whether the early universe made more galaxies overall, or simply made some of them brighter sooner, remains open.

Nov 2026 Dark Energy Complication — DESI 2025–2026

The DESI (Dark Energy Spectroscopic Instrument) survey's March 2025 analysis used nearly 15 million galaxies and quasars spanning 11 billion years of cosmic history. It suggested dark energy may have been stronger in the past and is now weakening; depending on which external datasets (cosmic microwave background, supernovae, weak lensing) were combined, the preference ranged from 2.8 to 4.2 sigma — suggestive, but short of the 5-sigma discovery threshold.58 The picture remains unsettled: in April 2026 DESI finished mapping its entire planned survey area ahead of schedule (more than 47 million galaxies and quasars), with results from the full five-year dataset expected in 2027,59 and a July 2026 full-shape analysis of the Lyman-alpha forest produced a central value that shifted back toward the standard model.60 If evolving dark energy is confirmed, this would alter the standard Lambda-CDM cosmological model — the very framework used to count galaxies across cosmic time. A weakening dark energy changes how we model the universe's expansion history, which in turn changes how we extrapolate galaxy counts from what we observe to what we cannot see.

"The question of how many galaxies exist remains an active area where new observations can still shift the numbers — a frontier still in negotiation between measurement and model."

— Synthesis of current literature

Sections 2–12 · Sources

The rest of the research is for paid subscribers

You’ve just read the first section, and it’s free for everyone. The other eleven sections and all 147 sources are part of a paid subscription to my Substack, Let’s Talk About Anything and Everything. Paid subscriptions give me the time to keep reading, checking, and updating this work, and I’m grateful for every one.

Already a paid subscriber?

Your reader key is at the bottom of each paid post. Enter it once, and this device will remember it.

Not ready to subscribe? That’s completely fine. Section 1 stays open here, and the free newsletter is always open too. If you’d like to support the work later, the option will be waiting.

What’s inside

  • ✦2Methods of Estimation
  • ✦3JWST Latest Discoveries
  • ✦4Fine-Tuning & Multiverse
  • ✦5Consciousness & Cosmos
  • ✦6Divinity & the Cosmos
  • ✦7Native Traditions
  • ✦8Elyrian Convergence
  • ✦9The Epigenome
  • ✦10Hypoxia & the Epigenome
  • ✦11The Convergence
  • ✦12The Brain as Complex System
  • ✦·Sources & Further Reading (147)
Opening the research…