This article was originally authored by Dr. Hugh Ross and is republished here with permission from Reasons to Believe, a ministry dedicated to integrating science and faith. All rights reserved by the original publisher. To explore more resources, visit their website Reasons to Believe.
One of the most common inquiries posed to Reasons to Believe scholars can be expressed by this pair of questions:
Producing a scientific date for the origin of human beings is not easy and is far from precise and reliable. All methods for dating human origins involve both large statistical and even larger systematic errors.
Statistical errors refer to imprecisions in measurements. Systematic errors refer to environmental and instrumental factors that can shift all values up or down.
In some cases, these factors are known and quantifiable. In others, they are known but not measurable, or entirely unknown.
In astronomy, physics, chemistry, and geophysics, the environmental and instrumental factors are often well understood. Researchers can publish with clear margins of error and certainty levels (67, 95, or 99 percent).
In the life sciences, complexity often prevents full identification of systematic effects. As a result, many studies report only statistical errors, leading readers to overestimate confidence in results.
Carbon 14 dating measures how long it has been since a living organism stopped taking in carbon from the atmosphere. Carbon 14’s half-life is 5,715 plus or minus 30 years.[1] Reliable results fall between roughly 800 and 40,000 years.
Carbon 14 is created when cosmic rays strike nitrogen 14. The flux of cosmic rays changes over time due to nearby supernovae. Four such events occurred within about 360 to 820 light years of Earth in the past 44,000 years,[2] enough to affect results by up to 10 percent.
Altitude and canopy coverage affect exposure. High altitude yields more exposure, while underground or forested environments yield less.
Uranium and thorium isotopes in the crust can transform nitrogen 14 into carbon 14. This explains why very old samples such as zircons and diamonds sometimes register apparent carbon 14 dates around 58,000 years.
Carbon 14 dating is still the preferred and most reliable method for samples younger than about 40,000 years.
These methods measure how long a sample has been isolated from heat or light. They track trapped electrons in crystals. Systematic effects include variable pre-burial exposure, delayed burial, and later disturbance.
The Jinmium Rock Shelter in Australia illustrates this. Early results suggested 60,000 years of human activity,[3] but later carbon 14 dating corrected the oldest artifacts to about 3,000 years.[4]
Electron spin resonance relies on measuring unpaired electrons and requires knowing past radiation levels, so it shares the same limitations as luminescence. Uranium thorium dating measures the ratio of thorium 230 to uranium 234 to estimate precipitation age, but only if the sample formed rapidly and remained uncontaminated.
Mitochondrial DNA and Y chromosomal analysis estimate the time back to a single common ancestor by measuring present diversity and assuming mutation rates and reproductive timing.
Supernovae and solar flares can alter mutation rates. In the past ten thousand years there have been no nearby supernovae,[7] but several occurred between 22,000 and 115,000 years ago.[8]
Reproductive ages vary greatly across history. Modern averages are longer due to lifestyle and social factors, which skews results toward older estimates.
For older remains, argon argon and paleomagnetic dating methods apply. These can measure up to several million years with smaller systematic effects compared to human-origin dating methods.
Awareness of these limitations encourages scientific humility. Determining precise dates for humanity’s origin remains an ongoing challenge.