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Wednesday, December 10, 2025

Trail 31 - Betasso Preserve Canyon Loop

I've visited the Betasso Preserve Canyon Loop Trail a few times during late Spring and early Summer. I really like this trail. It has a variety of terrain with beautiful mountain scenery. The trail is shared by hikers, joggers and cyclists. The area is a good mix of brush and trees without heavily overgrown areas with wild bramble. Early Summer supports a wide variety of flowers.



You can also visit nearby Bummers Rock during the same drive. This trail is Hike #31 from 60 Hikes Within 60 Miles: Denver and Boulder. Within which, it's described at "a geological enthusiast's wonderland." Even though it has diverse terrain, the change in elevation is only about 400 feet. You'll have a chance to see some wildlife here as well. It's recommended to enjoy this trail on the weekday, as weekends can be crowded (at least in the parking lot).

Sunday, December 07, 2025

Ireland's First Script Ogham (with Converter tool)

The Ogham Alphabet

The Ogham alphabet (often pronounced "OH-um") is the earliest known form of writing used in Ireland and parts of Britain, appearing primarily in inscriptions between the 4th and 9th centuries AD. It's unique among world writing systems for its striking visual form and method of inscription.

Historical Context and Use

Ogham emerged during the period of Primitive Irish, the oldest attested form of the Gaelic language.

  1. Form and Structure: Unlike the Latin or Runic alphabets, Ogham consists entirely of a system of notches and parallel strokes etched along a central line, or "stemline." On monuments, the natural corner or edge of a standing stone served as this stemline, making Ogham essentially a three-dimensional script. It reads vertically, typically from bottom to top.
  2. Primary Function: The vast majority of surviving Ogham inscriptions are found on monumental stones (known as Ogham stones) scattered across Ireland and Wales. These stones functioned primarily as commemorative boundary markers or memorials, usually bearing the name of an individual and that person's lineage.
  3. The "Tree Alphabet" Tradition: Ogham is incorrectly known as the "Celtic Tree Alphabet." This association comes from medieval manuscript tradition, where each of the 20 original Ogham characters was given a name corresponding to a native Irish tree or plant (e.g., Beith = Birch, Dair = Oak). This tradition popularized the script but often overshadowed its true linguistic purpose.
  4. Decline: Ogham usage declined dramatically after the 7th century, largely being replaced by the Latin alphabet as Christianity spread and written language shifted from monumental inscriptions to manuscripts.

Transliteration for Modern English

The original Ogham alphabet had only 20 core characters (feda), which reflected the limited sound set of Primitive Irish. To adapt this ancient script for Modern English (which has 26 letters and many more sounds), a systematic approach is necessary.

This converter (below) uses a modern, mostly reversible transliteration method that maps the six missing English letters (J, K, P, V, W, X, Y, Z) to their closest existing Ogham phonetic or orthographic neighbors, ensuring every modern English word can be accurately rendered in Ogham. We also use the dedicated (Ogham space mark) for all word separation and punctuation to maintain the authenticity of the script's digital representation.

 

Ogham Bi-Directional Converter

Output (Click to Copy):

Note on Mapping: This converter uses the 20 core Ogham letters plus the later Forfeda for missing English sounds (P and CH). Punctuation is converted to the Ogham space mark ( ) for a more authentic output.

Latin Input Ogham Output Ogham Name Mapping Rationale
A, E, I, O, Uᚐ, ᚓ, ᛁ, ᚑ, ᚒAilm, Edad, Idad, Onn, UrDirect Ogham Vowels
BBeithDirect Ogham character.
PPeith**Uses the Forfid (supplementary letter).**
F, VFernV is voiced pair of F.
C, KCollK shares the hard C (/k/) sound.
CHEamhancholl**Uses the Forfid for the CH sound.**
GGortDirect Ogham character.
DDairDirect Ogham character.
TTinneDirect Ogham character.
HUathDirect Ogham character.
LLuisDirect Ogham character.
MMuinDirect Ogham character.
NNuinDirect Ogham character.
RRuisDirect Ogham character.
S, ZSailleZ is voiced pair of S.
JCollMapped to C/K as a functional default.
WUrMapped to the vowel U (closest to 'oo' sound).
YIdadMapped to the vowel I.
QQuertDirect Ogham character.
XᚉᚄColl + SailleMapped as the two-character phonetic sequence CS (/ks/).

For information on other tools and topics:

Thursday, December 04, 2025

Trail 34-ish at El Dorado State Park

On the Fall Solstice or near-abouts in 2025, I visited Eldorado State Park.  This park has a trail that is listed in the 60 Hikes within 60 Miles: Denver and Boulder at #34. Like many Spanish-origin names in Colorado, the name "Eldorado" has an anglicized spelling, so it's not "El Dorado". Instead of hiking the Eldorado Canyon Trail, as suggested in the book, I hiked the loop called Rattlesnake Gulch Trail.





The trail is challenging, as there is significant uphill segments with several large cutbacks. I was able to visit on a day that was comfortably warm. Major portions of the hike are shaded. There are two uncommon points of interest on this trail too.

Crags Hotel Ruins is a location where a hotel once stood but long since burned down. The ruins of central fireplace still remain, along with a few other fleeting signs of some long-past structures.


Also on this loop, you'll find the Continental Divide Overlook.  This a great location for some awesome Rocky Mountain views (presumably including the Continental Divide).


I really enjoyed Eldorado Canyon State Park. This will be a location to which I'd love to return. Parking is $10 and is paid upon arrival. Reservations are required for weekends between May 1 and October 1.

Tuesday, December 02, 2025

Weight Calculation Tool based on Latitude

Your Weight Changes with Latitude

Your weight changes as you move further or closer to the Equator on Earth. This is true even if you typically measure your weight in kilograms.

Your mass is the amount of matter in your body. This remains constant.  However, your weight (the force of gravity acting on your mass) changes because the Earth's "falling" acceleration due to gravity (g) is not uniform. This variation is primarily due to two factors:

  1. The Earth's Spin (Centrifugal Force): As the Earth rotates, it creates an outward centrifugal force that partially counteracts gravity. This force is strongest at the Equator and drops to zero at the Poles, making you slightly lighter near the Equator.
  2. The Earth's Shape (Equatorial Bulge): The Earth is not a perfect sphere. It bulges around the Equator. This means you are physically farther from the planet's center when standing at 90° latitude than at the Poles. This distance also weakens the gravitational pull.

The combination of these two effects means you will exert the greatest gravitational force (be the heaviest) at the poles and the least at the Equator.

You can use Google Maps to find your current latitude and the latitude of your target or destination.


How to Use the Calculator

Use the calculator below to find your true constant mass and see how your weight (the force) would change if you moved to a new location:

  1. Your Scale Reading: Enter your weight and select your unit (lbs or kg). If you use kg, the tool will automatically adjust for the standard gravity value that your scale likely uses to calculate your true mass.
  2. Current Latitude: Enter the latitude where you took the measurement.
  3. Target Latitude: Enter the latitude of interest (90° for the Pole or 0° for the Equator).

The tool will then show you your True Constant Mass (in kg and slugs), your Current Weight (in lbs and Newtons) and your calculated Target Weight at the new latitude. One additional note is that I previous covered this topic with an Excel spreadsheet tool. This new tool (below) is more accurate than my original spreadsheet because this new tool takes Earth's shape into account.

Weight & Mass Calculator 🌍

Input your weight in either pounds (lbs) or kilograms (kg).

Enter your details and click 'Calculate'.


For information on other tools and topics:

Friday, November 28, 2025

Number Rounding Tool You Might Need

Everyone learns the "Schoolhouse Rule" of rounding. This is where you look at the next digit and if it's 5 or greater, round up. This method (Round Half Up, or 5 always rounds up) works for everyday math, but it introduces a hidden and cumulative problem that is often not considered: upward bias.

In financial, scientific, or engineering calculations involving hundreds of figures, the "5 always rounds up" rule causes you to round up more often than you round down. This subtle bias can compound into a significant error in the final result. Our tool provides professional rounding systems designed specifically to eliminate this problem.

Reducing Bias

These methods are used when the total sum of all figures must be as accurate as possible, minimizing accumulated error.

Mode What It Does Why You Use It
Round Half Even When a number is exactly halfway (e.g., 5.5 or 6.5), it rounds to the nearest even digit. This is Banker's Rounding. By rounding equally to even numbers, it eliminates the upward bias of the schoolhouse method. It's the standard for professional financial and scientific calculations.
Stochastic Rounding Uses random chance to decide whether to round up or down when exactly halfway. Used in high-precision scientific simulation and modeling to introduce statistical fairness and prevent bias in complex, non-linear calculations.

Strict Control Over Direction

These modes are used when your calculation must never exceed (or never fall short of) the true value.

Mode Rule Example Use Case
Round Floor Always rounds down (towards negative infinity). Resource Allocation: Calculating how many full containers, shipments, or packages you can create from a given amount, ensuring you never over-count.
Round Ceil Always rounds up (towards positive infinity). Safety Margins: Calculating how much material to order or capacity you need, ensuring you always have at least the required amount.

By using this tool, you move beyond simple arithmetic to achieve the precise, mandate-required accuracy necessary for serious data analysis and computation.

Multiple Methods Rounding Tool 🎯

Note: The rounding place is specified by its 10^N exponent, covering every single place value from 10^9 down to 10^-9.

For information on other topics and tools:

Thursday, November 20, 2025

Colonizing the Universe at Sub-Light Speed

The Ultimate Relativistic Sacrifice

Assuming Faster-Than-Light (FTL) travel is physically impossible and cryogenic hibernation is unavailable; humanity's expansion into the cosmos may rely on the extreme physics of time dilation from Special Relativity aboard some sort of colony ark. While time dilation will allow the crew to complete a voyage within their lifetime, the journey is an irreversible commitment that gambles the future of a civilization on a target millions of light-years away.


The Andromeda Challenge and the Irreversible Loss

The Andromeda Galaxy (M31) is our nearest major intergalactic target at approximately 2.5 million light-years distant. For the crew to complete this voyage in a human lifetime (e.g., 40 years of proper time), the ship must maintain a sustained average velocity of roughly 99.99999999995 c.

  • The Sacrifice: The travelers are not simply leaving home. They are permanently severing their connection to the Milky Way. When they arrive, 2.5 million years of cosmic, stellar, and biological evolution will have occurred in their home galaxy. Their families, their culture, and every trace of the civilization that launched them will be reduced to ancient memories.
  • A Temporal Gap: The voyagers exist in a tiny bubble of compressed time from which they will step into a universe that is unrecognizable to the one they left. They will have to pay millions of years of separation for their mere decades of travel.

The Existential Gamble

The greatest human impact lies in the uncertainty of the destination. The colony ark, having made the ultimate sacrifice, arrives 2.5 million years later. The pioneers will dependent on finding a habitable world.

  • Arrival on a Dead World: There is no guarantee of success. Target systems that looked promising via telescopes 2.5 million years ago may have undergone catastrophic changes. Target stars may have died, planetary orbits destabilized or life-bearing worlds may have been sterilized by a nearby supernova. The crew may be forced to settle a barely viable moon or asteroid, dedicating their compressed lives to the construction of a fragile habitat.
  • The Psychological Toll: Imagine emerging from a forty-year journey to find that the sacrifice of millions of years was in vain. Settlement options leave them desperate and even face slow extinction. The mental fortitude required for the crew to proceed with establishing a colony under such bleak conditions will be very a demanding for human endeavor.

Cosmic Expansion and the Event Horizon

The navigational challenge of intergalactic travel is a matter of pure survival, where failure means being permanently stranded in the dark void between galaxies.

1. The Super-Deep Space Trap

The massive target distance requires the ark to compensate for both the target galaxy’s movement and the expansion of the universe (Hubble flow) over millions of years.

  • Aiming for the Past: The crew must not aim for where Andromeda is now, but where cosmological models predict it will be millions of years in the future.
  • Gravitational Anchor: The ship must execute an instantaneous deceleration precisely within the gravitational well of the destination galaxy. If the deceleration occurs even slightly too far out, the surrounding spacetime expansion could accelerate the ship away from the galaxy before its local gravity can pull it in, stranding the crew in the empty, super-deep intergalactic void.

2. Reaching the Cosmological Edge

The concept of colonizing galaxies near the cosmological event horizon (currently 16 billion light-years away) highlights the final limit. Galaxies beyond this horizon are already receding faster than light due to accelerating cosmic expansion and are literally unreachable today, even at 0.999… c.

  • The Temporal Trap: To reach a galaxy near the horizon, the launch must occur almost instantaneously on the cosmic scale. If humanity delays too long, cosmic expansion will push that galaxy irrevocably beyond our reach, forever confining future generations to our local galactic neighborhood.

The Enduring Drive: A Galactic Legacy

Despite the risks and the terrifying finality of the journey, the impetus for expansion remains. We have an innate and evolutionary imperative to survive and propagate.

  • Successive Generations: If a colony succeeds in Andromeda, its primary goal is not to thrive, but to replicate the mission. The next generation of settlers will build their own relativistic arks, pushing further into the Laniakea Supercluster, driven by the knowledge that their future depends on finding and securing more footholds in the cosmos.
  • A Galactic Civilization: Each new colony, whether on an Earth-like world or in a sealed dome on a cold moon, becomes a new seed of humanity, creating a truly scattered, time-dilated galactic civilization whose survival is secured not by technology alone, but by the extraordinary sacrifice and unyielding courage of the original voyagers.

The Unavoidable Horizon and the Next Step

Such a relativistic colony ark would be more than just a ship. It will be a declaration of humanity's unyielding commitment to existence that must be secured regardless to possible costs. This colonization model, constrained by the immutable laws of physics (the speed of light and the accelerating expansion of the universe) forces us to recognize a sobering truth. Our window for becoming a truly galactic civilization is finite and closing.

The greatest challenge is not merely building the next ark, but cultivating the societal will to invest in such a millennia-spanning gamble. Before the first interstellar journey can even begin, we must achieve a few critical milestones:

  • Establish a Self-Sufficient Solar System: We must first master the art of survival away from Earth. Settling the Outer Solar System, as previously discussed, is the required engineering training ground, guaranteeing that the seed of humanity does not perish with the inevitable death of the Sun.
  • Achieve Kardashev Type II Capability: The energy requirements for a sustained 0.999… c voyage is so vast that they demand harnessing the power output of an entire star. This requires a civilization with an unprecedented scale of infrastructure and coordination.
  • Embrace the Temporal Sacrifice: The success of the journey rests on the psychological endurance of the travelers and the emotional maturity of the home world to accept the irreversible loss.

The final question for our species is no longer "Can we reach the stars?" but "Are we worthy of them?" Our willingness to make the ultimate sacrifice and to gamble millions of years of our history for the chance of a single new beginning will define whether humanity remains a fragile, single-star species or evolves into an enduring, time-scattered intergalactic legacy. The time to prepare for this final, defining endeavor begins now, before the accelerating expansion of the cosmos locks our future out of reach forever.


What Do We Do Now?

The path forward is clear. We need to Master our local region in order to plan for the galactic expanse. We should relentlessly pursue advances in fusion power, closed-loop life support and extreme deep-space navigation. We can act knowing that every technological victory at the solar scale moves us one step closer to making the ultimate and irreversible jump to the stars.

Also see:

Wednesday, November 12, 2025

Trail 60 - Great Views from Eagle Wind Trail of Rabbit Mountain

One spring morning in 2017, Allie and I hiked the Rabbit Mountain trail. It was a beautiful hike. The trail itself was damaged, apparently due to a combination of overuse and recent rains. As such, there were more than a few spots that required special navigation to avoid losing a shoe to the mud.  The trail itself is a fairly straightforward loop without connectors or spurs.  

Rabbit Mountain's trail, called Eagle Wind Trail, is Hike #60 mentioned in 60 Hikes within 60 Miles from Denver and Boulder.  It's a great location for open views of the Rocky Mountains, the foothills and the Great Plains beyond.



The day we visited was temperate with a clear sky. It was early Spring, so the scenery had not yet turned green with vibrate flowers. We had a clear view of Long's Peak for most of the hike. However, I'm not sure I would make the drive from Denver area back to this particular trail.

Tuesday, October 28, 2025

Interstellar Ark to Race to the Stars and Against Time

Our Sun, the source of all energy for life in our system, has a finite lifespan. In about 5 billion years, it will exhaust its core hydrogen, swell into a Red Giant and incinerate the inner Solar System, including Earth and eventually Mars. As such, Humanity's colonization efforts on Mars and the icy moons of the Outer Solar System are just temporary survival strategies. Even the fleeting habitability window on the moons of Jupiter and Saturn will close within a few hundred million years as the Sun's luminosity peaks.

To ensure the long-term survival of the species, humanity must master the ultimate engineering and emotional challenge of interstellar travel. Leveraging the relativistic properties of near-light-speed (c) travel is the only way for humans to reach other star systems within a single lifetime, transforming a journey spanning light-years into one that seems manageable to the travelers on interstellar arks.


A One-Way Ticket to the Stars

The decision to embark on an interstellar ark is not merely a scientific one; it's a profound, intensely personal act of sacrifice and hope. These are not round trips.

  • Leaving Everything Behind: The voyagers are pioneers, severing all ties with their home system, knowing they'll never return, and that everyone they ever knew will be long gone.

  • The Weight of Expectation: They carry the immense weight of humanity's future, a testament to the belief that life is meant to endure and explore. The "lifetime" they experience aboard the ark might be just years, but it's years spent in a cramped, artificial environment, with only the distant promise of a new home.

  • A Multi-Generational Endeavor: While time dilation makes the journey short for the crew, for the civilization that built and launched the ark, it's a multi-generational mission. The investment, the resources, and the hope stretch across centuries, a testament to collective foresight.


Relativistic Travel and Time Dilation

The core concept allowing interstellar travel in a human lifetime is time dilation, a consequence of Einstein's Special Relativity.

When a spacecraft approaches the speed of light, time for the travelers on board (the proper time) slows down dramatically relative to time observed by those remaining on Earth (the coordinate time).

  • The Effect: A trip to a star 50 light-years away would still take 50 years as measured by Earth observers. However, if the ship maintains an average speed of, for example, 99.999% of c, the time experienced by the crew could be compressed to just a few months or years.

  • The Challenge: Achieving and maintaining such high velocities requires an immense, continuous energy source, likely a form of matter-antimatter annihilation drive or an advanced fusion drive that provides high thrust over decades.



The Galactic Habitable Zone (GHZ) as a Guide

Since the vastness of space makes blindly searching for habitable worlds impossible, initial target selection is guided by the Galactic Habitable Zone (GHZ).

The GHZ is an annulus (ring) in the galactic disk where star systems are considered most likely to develop and sustain complex life. This zone is a balance between two main factors:

  1. Required Metallicity: The zone must be close enough to the galactic center to have a high concentration of heavy elements ("metals"—anything heavier than hydrogen and helium) needed to form rocky planets.

  2. Radiation and Density: The zone must be far enough from the galactic center to avoid the intense radiation and high frequency of supernovae that occur in the denser, inner regions, which could repeatedly sterilize planetary surfaces.

By targeting G-type, K-type, and even M-type stars within this GHZ ring, humanity maximizes the odds of finding an already existing, or at least a highly promising, habitable world upon arrival.


From Ark to Colony: Technologies and Unforeseen Challenges

To settle a new star system—especially one whose habitability is poorly characterized before arrival—the colonization ship must function as a comprehensive, self-contained factory and resource harvester.

Propulsion and Journey Survival

Requirement Technology Needed Purpose
Propulsion Fusion/Antimatter Drive Provides the sustained thrust necessary for near-c velocities and the huge deceleration upon arrival.
Collision Mitigation Magnetic Deflector Shields Creates a powerful magnetic field ahead of the ship to ionize and deflect interstellar dust and gas, which hit the ship like high-velocity shrapnel at relativistic speeds.
Life Support Closed-Loop Ecosystems Requires perfect, self-repairing biospheres to recycle all water, air, and nutrients for decades of travel without external resupply.

Settlement: Making a Home in the Unknown

The true test begins upon arrival. Unlike our well-studied Solar System, new systems will present unforeseen challenges. The ark must be equipped to establish a sustainable settlement on any plausible world it encounters, even if it's less than ideal.

  1. Mining and Manufacturing: The ship must carry Molecular Fabricators or advanced 3D printing systems to convert local raw materials (ice, rock, atmosphere) into necessary infrastructure, shielding, and repair components.

  2. Habitats and Shielding (Without Terraforming):

    • Subsurface Bases: On airless or radiation-exposed moons, settlers would immediately burrow underground to use rock and regolith as natural shielding against cosmic rays and local radiation.

    • Paraterraforming: Establishing large, modular, self-contained habitats or domes (paraterraforming) that maintain Earth-like conditions locally, independent of the external environment. This could be on a cold gas giant moon or a dry, thin-aired terrestrial planet.

  3. Full Terraforming Capabilities: For eventual planet-scale engineering, the ark must carry seed technology capable of:


The Enduring Drive: To Infinity, and Beyond

Even after successfully settling a new star system, the human spirit, honed by millennia of survival, will not rest. The drive to explore, to discover, and to secure humanity's future will continue.

  • Successive Waves of Expansion: Just as our ancestors ventured across continents and oceans, and as we plan to spread within our own Solar System, successive generations will likely feel the same urge to build new arks and push out even further into the galaxy.

  • The Legacy: Each new colony becomes a beacon, a new genesis point for life in the cosmos. The sacrifice of the initial voyagers, the struggles of the first settlers on an alien world, all contribute to a legacy that aims for a truly galactic civilization, a testament to humanity's unyielding will to live and thrive amongst the stars.