Explore Natural Philosophy

Phil • Cr. Think • Science • Hist •

Human Ancestors

Pre-hominid human evolution all the way back to LUCA.

Hominin World Population: 2 Million (maybe)

When Homo sapiens first emerged, their population in Africa was likely just a few hundred thousand, while the total hominin population, including other species like Neanderthals and Homo heidelbergensis, may have ranged from 1.1 to 2.1 million. During this period, Homo sapiens were primarily found in Africa, while other hominins occupied broader ranges across Eurasia, […]

Hominin World Population: 2 Million (maybe) Read More »

World Population: 1.5 Million

Cognitive Revolution By 70,000 BCE. Population range: 500,000 to 2.5 million. Given the uncertainties and lack of direct data, the following are speculative estimates. Africa-Middle East: 50-60% or 600,000 to 1 million people Africa, being the origin of modern humans, likely had the highest population density at this time, particularly in Sub-Saharan regions which were

World Population: 1.5 Million Read More »

Mexico: Guilá Naquitz (Agrarian)

Earliest known agrarian society in the Americas zone: In Oaxaca, Mexico, the site of Guilá Naquitz provides evidence of early plant domestication, particularly of squash, around 8000 BCE, with subsequent developments including maize and beans. Imagined Image: An early agrarian society of Oaxaca, Mexico, circa 7900 BCE. It showcases small, temporary shelters, with indigenous people

Mexico: Guilá Naquitz (Agrarian) Read More »

Second Atmosphere: Carbon Dioxide & Nitrogen

Deep orange or reddish-brown atmosphere: The second atmosphere’s formation was crucial and occurred just before or alongside the formation of Earth’s oceans, which directly supported the evolution of organic molecules and prebiotic microenvironments. The second atmosphere began to develop around 4.5 to 4 billion years ago, as volcanic outgassing released gases trapped in the Earth’s

Second Atmosphere: Carbon Dioxide & Nitrogen Read More »

First Atmosphere: Hydrogen & Helium

Likely white or grayish atmosphere: The first atmosphere developed first but was not directly involved in the development of life. The first atmosphere formed shortly after Earth’s formation around 4.5 billion years ago. This initial atmosphere was primarily composed of hydrogen and helium, the lightest and most abundant elements in the universe, which were captured from

First Atmosphere: Hydrogen & Helium Read More »

Phenotype Variation: Eye Shape and the Epicanthic Fold

The feature of the epicanthic fold, particularly prevalent among East Asian populations descended from Haplogroup A, is an adaptation to cold, windy, and bright environments encountered as humans migrated northward from Africa. This phenotype likely developed to protect the eyes from frostbite and snow blindness, showcasing how genetic diversity within human lineages adapted to specific

Phenotype Variation: Eye Shape and the Epicanthic Fold Read More »

Emergence of Blood Type Variability in Primates

Blood type variations originated from common primate ancestors around 20 million years ago. While blood transfusions between species, such as between apes and humans, are not viable due to different and incompatible blood antigens, the development of blood type systems, including types similar to the human A, B, AB, and O, can be traced back

Emergence of Blood Type Variability in Primates Read More »

Francis Bacon

18 Generations Ago 30 Phil, Chapter 20: Francis Bacon and the Scientific Method Francis Bacon was born on January 22, 1561, in London to a prominent and influential family. The young Francis Bacon received a comprehensive education, attending the prestigious Trinity College, Cambridge, at the age of 12. Bacon is the Father of the Scientific

Francis Bacon Read More »

debris of a stellar explosion, 3d illustration

Interstellar Clouds: Organic Molecules

The synthesis of simple organic molecules such as formaldehyde (H₂CO), methanol (CH₃OH), and simple hydrocarbons in the dense molecular clouds of the interstellar medium occured once sufficient carbon was present. This process has been ongoing for billions of years but became more prevalent as the universe aged and more carbon became available. Big History Thresholds:

Interstellar Clouds: Organic Molecules Read More »

Inorganic Precursors to Organic Molecules

The chemical evolution from inorganic precursors to organic molecules is a fascinating story of transformation driven by Earth’s dynamic early conditions and possibly assisted by the input from space in the form of meteorites rich in organic compounds. During this period, the Earth witnessed a series of complex chemical reactions facilitated by its primordial atmosphere,

Inorganic Precursors to Organic Molecules Read More »

Scroll to Top