﻿ What is the speed of Earth? Discover How Fast it Moves

What is the speed of Earth? Discover How Fast it Moves

The answer to how fast the earth moves is: it depends. Check out why.

Like many of you, I've wondered how fast the Earth moves through space. But, in order to answer this, we must first ask: How quick in comparison to what?

Only when evaluated against something else does speed make sense—this is referred to as a frame of reference. We'll examine the Earth's motion from several perspectives, from its spin on its axis to the lingering glow of the Universe's blazing beginnings. Each depicts our world moving at dizzying speeds.

Join me on this exciting voyage to understand the mechanics of our planet's movement!

Spin Speed

The Earth is our most intimate frame of reference. It rotates eastward at the pace of one full turn every 23 hours and 56 minutes. At the equator, this spin causes the surface to spin at around 1,600 kilometres per hour! That's the speed of a bullet discharged! Of course, when you move north or south, this spins slower and slower until it reaches zero speed at the poles.

Orbit Velocity

Next, we consider the Earth’s path circling the Sun each year. From this frame of reference, our home planet travels at 30 kilometres per second on average. In one full orbit, it journeys 940 million kilometres! Picture that gigantic racetrack! Cruising around at over 100,000 kilometres per hour, no wonder it takes 365 days to complete the circuit. The actual speed varies a bit due to the elliptical orbit shape.

Within the Galaxy

We can see the complete solar system circle the Milky Way galaxy every 250 million years by expanding our vision. From this vantage point, the Earth travels through space at 220 kilometres per second—nearly 500,000 miles per hour! The Sun, accompanied by its planets, navigates up and down the galaxy's pancake structure.

The Great Attractor

To comprehend the most massive motions, we must broaden our perspective to encompass millions of galaxies travelling within the universe. Within our Local Group of galaxies, the Milky Way and its nearby Andromeda spiral at 1,000 kilometres per second towards a gravitational focal point known as the Great Attractor. This unfathomably vast nexus of tens of thousands of galaxies spans 500 million light years and 100 quadrillion star masses.

Its total bulk could comprise 90% undiscovered dark matter that outweighs all visible stars. Though the galaxies appear luminous, the bulk of attraction comes from invisible material sheathing each system. What immense grasp must this gravitational giant exert to tug our Local Group within its inexorable pull?

Can we, however, establish an ultimate reference frame for measuring the flow of matter and energy in our universe?

Measurements from the Cosmic Background Explorer spacecraft indicate that the faint microwave light that pervades all of space—the cosmic microwave background radiation (CMB)—approaches such a backdrop. This pervasive thin photon fog formed approximately 400,000 years after the Universe's catastrophic start.

Photons can finally travel freely through space once electrons combine with protons to produce stable hydrogen. Previously, matter and light interacted so intensively that photons couldn't move without colliding with a particle.

That early hot dense plasma roared like our Sun today. Eventually, expansion allowed cooling—imagine the steam evaporating from an immense pot! After which photons propagated outward in all directions, redshifting into the microwave band as the Universe continued inflating. Remarkably, the CMB structure retains traces of tiny temperature ripples in the infant cosmos. Later density patches eventually collapsed under their gravity to ignite stars and galaxies.

But in those early eras, spots merely hotter and cooler by thousandths of degrees dictated where matter later congregated. By gauging patterns in this primordial glow, satellites reveal the Earth’s vector of travel relative to the timeworn CMB sky at 390 kilometres per second towards the zodiac constellation Leo.

What truths are yet to be revealed by this surviving relic of cosmic formative stages? So, by gradually expanding our frame, we expose and calculate ever-greater velocities for our gently rotating terrestrial home. I hope that visualising Earth's diverse motions through these various backdrops inspires astonishment at both the fragility and endurance of life as we all ride this cosmic carousel together!