Today in History - August 28
Curious about what happened today in history? Discover highlights from August 28th, including important events and defining moments from around the world.
Kudos365
Interesting Facts • Thoughts • Ideas
Curious about what happened today in history? Discover highlights from August 28th, including important events and defining moments from around the world.
Albert Einstein (March 14, 1879, - April 18, 1955) German-born theoretical physicist whose ideas fundamentally changed humanity’s understanding of space, time, gravity, light, and energy.
Albert Einstein
Physicist Who Transformed Our Understanding of the Universe
Albert Einstein was a German-born theoretical physicist whose ideas fundamentally changed humanity’s understanding of space, time, gravity, light, and energy. Best known for the theories of special and general relativity, he also made essential contributions to quantum physics and statistical mechanics. His work reshaped modern science and made him one of the most recognizable intellectual figures of the twentieth century.
Einstein was born on March 14, 1879, in Ulm, in the German Empire. His family soon moved to Munich, where his father and uncle operated an electrical engineering business. As a child, Einstein was thoughtful and independent, showing a strong interest in mathematics and the natural world. He later recalled being deeply impressed by a compass shown to him when he was young. The unseen force moving its needle suggested that reality contained structures and forces hidden from ordinary observation.
Contrary to the popular story that he performed poorly in mathematics, Einstein demonstrated considerable mathematical ability from an early age. His difficulties were primarily with rigid teaching methods and unquestioned authority. He preferred to understand ideas through personal investigation rather than memorization.
Education and Early Independence
When the family business encountered difficulties, Einstein’s parents moved to Italy. He eventually left his Munich school and joined them, renouncing his German citizenship in 1896. For several years he was officially stateless.
After completing preparatory studies in Aarau, Switzerland, Einstein entered the Swiss Federal Polytechnic in Zurich, later known as ETH Zurich. He trained as a teacher of mathematics and physics and graduated in 1900. In 1901, he became a Swiss citizen, a nationality he retained for the rest of his life.
Einstein struggled to obtain a university position after graduation. In 1902, he began working as a technical examiner at the Swiss Patent Office in Bern. His job required him to evaluate inventions involving electrical and mechanical devices. Although the work was not academic, it provided financial stability and encouraged the habit of reducing complicated proposals to their essential principles.
During his years in Bern, Einstein married Mileva Marić, a former classmate at the Polytechnic. They had two sons, Hans Albert and Eduard. The marriage later deteriorated, and they divorced in 1919. Einstein subsequently married his cousin Elsa Löwenthal.
The Extraordinary Year
In 1905, while still employed by the patent office, Einstein published four papers that changed the direction of physics. This period became known as his annus mirabilis, or “miracle year.”
One paper explained the photoelectric effect by proposing that light could behave as discrete packets of energy, later called photons. This idea supported the emerging quantum theory and challenged the conventional understanding of light as exclusively wave-like.
A second paper explained Brownian motion—the irregular movement of tiny particles suspended in a liquid. Einstein showed how the motion could result from collisions with molecules. His analysis offered powerful evidence that atoms and molecules were physically real at a time when some scientists still questioned their existence.
A third paper introduced the special theory of relativity. Einstein began with two principles: the laws of physics are the same for observers moving at constant speeds, and the speed of light in a vacuum remains constant regardless of the motion of its source or observer. From these principles came remarkable consequences. Measurements of time and distance are not absolute but depend on the relative motion of the observer.
A fourth paper explored the relationship between mass and energy. Its central result was later expressed through the equation:
E=mc2
The equation showed that mass is a concentrated form of energy. Because the speed of light squared is an enormous quantity, even a small amount of mass corresponds to a tremendous amount of energy.
A New Theory of Gravity
Special relativity applied to motion at constant velocity, but Einstein wanted to extend its principles to acceleration and gravity. After years of work, he completed the general theory of relativity in 1915.
Isaac Newton had described gravity as a force acting between masses. Einstein proposed a more fundamental interpretation: matter and energy curve the structure of spacetime, and objects move along paths determined by that curvature. In this view, Earth travels around the Sun because the Sun’s mass alters the geometry of the surrounding spacetime.
General relativity explained a previously unresolved irregularity in the orbit of Mercury and predicted that gravity would bend light. During a solar eclipse in 1919, two British expeditions measured the apparent positions of stars near the Sun. Their findings were reported as supporting Einstein’s prediction.
The results made Einstein internationally famous. Newspapers presented him as the scientist who had overturned Newton’s universe. Although later measurements achieved far greater precision, the eclipse observations played an important role in bringing general relativity to worldwide attention.
General relativity eventually became essential to the study of black holes, gravitational waves, and the evolution of the universe. It also acquired practical importance: satellite navigation systems must account for relativistic effects to provide accurate positions on Earth.
Quantum Theory and the Nobel Prize
Einstein is closely associated with relativity, but his work on quantum physics was equally important. His explanation of the photoelectric effect demonstrated that light could exchange energy in individual quantities. This insight helped establish the foundations of quantum mechanics and later made possible technologies including photoelectric sensors and aspects of modern electronics.
Einstein received the 1921 Nobel Prize in Physics, awarded in 1922. The citation emphasized his services to theoretical physics and especially his discovery of the law of the photoelectric effect. The prize did not specifically recognize relativity, which remained controversial among some scientists at the time.
Although Einstein helped launch quantum theory, he became uncomfortable with the probabilistic interpretation developed by later physicists. He accepted the theory’s experimental success but believed it was incomplete. His long debates with Niels Bohr concerned whether nature was fundamentally governed by probabilities or whether a deeper, more complete description remained undiscovered.
These disagreements helped clarify the philosophical and scientific implications of quantum mechanics. Several thought experiments proposed by Einstein and his colleagues became central to later research into entanglement and the foundations of quantum physics.
Exile and Life in the United States
Einstein held academic positions in Zurich and Prague before moving to Berlin in 1914. There he became a member of the Prussian Academy of Sciences and director of the Kaiser Wilhelm Institute for Physics.
The rise of Adolf Hitler transformed his circumstances. Einstein was Jewish, internationally prominent, and outspoken in support of democratic and humanitarian causes. When the Nazis came to power in 1933, he was traveling outside Germany. He renounced his German citizenship and never returned to live there.
Einstein settled in the United States and joined the Institute for Advanced Study in Princeton, New Jersey. He became an American citizen in 1940 while retaining his Swiss citizenship.
In 1939, physicists Leo Szilard and Eugene Wigner visited Einstein and explained the possibility that Nazi Germany might develop an atomic bomb. Einstein signed a letter to President Franklin D. Roosevelt warning that nuclear chain reactions could lead to extraordinarily powerful weapons. The letter helped draw the American government’s attention to uranium research.
Einstein did not participate in the Manhattan Project and did not work on the atomic bomb. His relationship to nuclear weapons was indirect, arising from both the mass-energy relationship and the warning letter bearing his signature. After the war, he supported international control of nuclear technology and warned about the dangers of the arms race.
Public Life and Moral Concerns
Einstein used his fame to speak about matters beyond physics. He supported civil liberties, opposed racism, advocated cooperation among nations, and maintained a strong connection to Jewish cultural and educational causes. He supported the establishment of the Hebrew University of Jerusalem and helped raise funds for it.
His political views evolved in response to events. Although he was strongly inclined toward pacifism, the threat posed by Nazi Germany persuaded him that force could sometimes be necessary. After the Second World War, he again emphasized disarmament and international government as safeguards against catastrophic war.
Einstein also spoke against racial discrimination in the United States. He formed a friendship with the African American singer and civil-rights advocate Paul Robeson and supported organizations working for racial equality.
In 1952, after the death of Israel’s first president, Chaim Weizmann, Einstein was offered the presidency of Israel. He declined, explaining that he lacked the experience and aptitude required for official leadership.
Final Years and Legacy
Einstein spent his later years seeking a unified field theory that would bring gravity and electromagnetism within a single mathematical framework. He did not complete such a theory, and the growing importance of quantum mechanics left him increasingly separated from the main direction of theoretical physics. Nevertheless, the search for a unified description of nature continued to influence subsequent generations of scientists.
Albert Einstein died in Princeton on April 18, 1955, at the age of seventy-six, after an abdominal aortic aneurysm ruptured.
Einstein’s legacy reaches far beyond a single equation. Special relativity transformed the concepts of space, time, mass, and energy. General relativity redefined gravity and provided a foundation for modern cosmology. His work on light quanta helped establish quantum physics, while his study of Brownian motion strengthened the scientific case for the atomic structure of matter.
He also became a lasting symbol of intellectual independence. Einstein’s willingness to question assumptions allowed him to see familiar problems in entirely new ways. By demonstrating that space and time are interconnected, that matter and energy are equivalent, and that gravity reflects the geometry of the universe, he permanently changed humanity’s understanding of physical reality.
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NASA Astronomy Picture of the Day:
At the latitude of ESO's Paranal Observatory in Chile, about 25 degrees south, Earth's rotation moves the planet's surface eastward at over 1,500 kilometers per hour. And while that's faster than the speed of sound at sea level, the motion is imperceptible. Still, that motion can be revealed in the apparent rotation of the night sky by photographing star trails. This star trail image was composed from a digital stack of 300 consecutive 25-second exposures made with a camera fixed to a tripod to trace the star trail arcs. The graceful arcs are concentric and centered at the south celestial pole, the southern hemisphere extension of Earth's axis of rotation into space. One of the observatory's operating 1.8 meter auxiliary telescopes, AT 3, appears beneath the south celestial pole, faintly illuminated in the foreground of this well-planned scene from a rotating planet. Growing Gallery: Lunar Eclipse of 2026 August 28 APOD's main NASA site is moving: From apod.nasa.gov to science.nasa.gov/apod
Photo by Osvaldo Castillo
Circaetus gallicus (Short-toed snake eagle) in Bhigwan, Maharashtra, India.
Tisha Mukherjee, CC BY-SA 4.0, via Wikimedia Commons. View source.
Aldous Leonard Huxley ~ (1894 -1963) Prolific English writer, novelist, philosopher, poet and pacifist.
He authored nearly 50 books, including Brave New World (1932) and his final novel, Island (1962). When he was 16, he suffered an eye infection that left him nearly blind for almost two years. His sight was so compromised that he learned to read in Braille. He was nominated for the Nobel Prize in Literature nine times. As a pacifist, he renounced all war and refused to fight in any war a decision which caused him not to be able to become a United States citizen after living in California for 14 years with his wife. More
NASA Astronomy Picture of the Day:
What a sight to behold, when a night sky became filled with colors that appeared to rain over the Skógafoss waterfall in Iceland. This image was taken in a single 5 second exposure by the photographer in April 2025. Seeing an aurora is on many people's bucket lists. But it is not easy. It requires high solar activity, dark and clear skies, and usually a viewing location at high latitude. That makes the northern lights more easily seen than the corresponding southern lights, simply because there is less landmass in the Southern Hemisphere, especially around the Antarctic Circle. Auroras are caused by charged particles from the solar wind that are captured by the Earth's magnetosphere and guided by the magnetic field to a region close to one of the poles, where they collide with gas particles in the atmosphere. Different colors indicate interactions with different gases at different altitudes, like oxygen (red and green) and nitrogen (blue and pink). APOD's main NASA site is moving : From apod.nasa.gov to science.nasa.gov/apod
Photo by Victor Lima Text: Cecilia Chirenti (NASA GSFC, UMCP, CRESST II)
Lake Coldai, an alpine lake beneath the Dolomites near village Alleghe, Italy. Today is World Lake Day, designated by the United Nations to raise awareness about the importance of lakes and to promote their sustainable management.
kallerna, CC BY-SA 4.0, via Wikimedia Commons. View source.
Always at dusk, the same tearless experience,
The same dragging of feet up the same well-worn path
To the same well-worn rock;
The same crimson or gold dropping away of the sun
The same tints—rose, saffron, violet, lavender, grey
Meeting, mingling, mixing mistily;
Before me the same blue black cedar rising jaggedly to a point;
Over it, the same slow unlidding of twin stars,
Two eyes, unfathomable, soul-searing,
Watching, watching—watching me;
The same two eyes that draw me forth, against my will dusk after dusk;
The same two eyes that keep me sitting late into the night, chin on knees
Keep me there lonely, rigid, tearless, numbly miserable,
The eyes of my Regret.
This poem was published in 1927, it is in the public domain.
Angelina Weld Grimké (1880 – 1958) was an American journalist, teacher, playwright, and poet. "Race" was a major issue in her life; she was the daughter of a white mother and a half-white father. She attended the best preparatory schools in Massachusetts. She was one of the first American women of color to have a play publicly performed.
NASA Astronomy Picture of the Day:
Are we looking at the future of our Sun? The James Webb Space Telescope captured today’s composite image of the Lion’s Head Nebula (NGC 2392) with its NIRCam and MIRI instruments. The Lion’s Head Nebula is the remnant of a Sun-like star. This star was unable to sustain the nuclear fusion in its core needed to remain stable. It began to shed layers of gas and dust into space, forming this planetary nebula. A hot stellar core, called a white dwarf, is left behind within the lion’s nose. Do not boop this nose! Intense radiation from the white dwarf is ionizing the gas as it expands, creating the irregular bubble that makes up the lion’s face. Dust clumps that have survived the white dwarf’s radiation and a cloud of ionized gas make up the lion’s mane. This new and more detailed view of the nebula will help humanity learn more about how the gas and dust interact with each other and the white dwarf radiation.
"The Accidental Burning of the USS Missouri in Gibraltar", lithograph, published by Ackermann & Co. The fire started on this day in 1843. In four hours, the steam frigate was reduced to a blackened and sinking hulk and finally at 03:20 in the morning of 27 August, the forward powder magazine exploded, destroying the burning ship.
Thomas Goldsworthy Dutton / Edward Duncan / George Pechell Mends / Adam Cuerden, Public domain, via Wikimedia Commons. View source.