Egg balancing

Last updated • 3 min readFrom Wikipedia, The Free Encyclopedia
Eggs balanced on a flat surface Balanced eggs.jpg
Eggs balanced on a flat surface

Egg balancing is a traditional Chinese practice of standing eggs on their ends that has also been popularized in the United States. Although the irregular shape of eggs makes this somewhat difficult, eggshells typically have many imperfections such that the vast majority can be balanced on their broad ends with minimal effort. [1]

Contents

Folklore holds that eggs can only be balanced in this way at a particular time of year: the lunar new year in China, the Dragon Boat Festival in Taiwan, [2] or the vernal equinox in the United States. It is also said that eggs can be balanced on the heads of nails at the equator. [3] In reality, eggs will balance anywhere at any time of year, and the practice has no connection to the gravitational force of the moon or sun.

History

Lichun egg

Egg balancing has been connected with Lichun, the solar term beginning Chinese spring ( ) on February 4 or 5 when the sun is at the celestial longitude of 315°. On this day, fresh chicken eggs were balanced on their broad end. In Taiwan, the practice is sometimes connected with the Dragon Boat Festival instead, on the fifth day of the fifth lunar month. [4]

United States

A 1945 Life article reported on "an egg-balancing craze" among the population of Chongqing (the interim capital of China during World War II) on that year's Lichun. [5] That article and subsequent followings-up started a similar egg-balancing craze in the United States, but transposed to the vernal equinox beginning Western spring on March 20 or 21 when the sun is at the celestial longitude of 0°. The idea that an egg is easier to balance on the spring equinox has since become an American urban legend, and egg-balancing events are sometimes held on that date. [6] In 1976, New York artist Donna Henes started organizing egg-balancing ceremonies with the stated goal of bringing about world peace and international harmony. [7] These events, which often drew thousands of people, are still held annually by Henes in New York City.

Science

The balancing of most eggs on their broad ends is not particularly difficult at any time of the year. [1] No physical influence of other celestial bodies on the egg can affect its balance to the extent required by the folk belief. Gravitational and electromagnetic forces, in particular, are considerably weaker and steadier than the disturbances created by the person's breathing and heartbeat.

In 1947, after Japanese newspapers picked up the story, the physicist Ukichiro Nakaya verified experimentally that eggs can be balanced with ease at any time of the year. He noticed that an eggshell usually has many small bumps and dimples so that, by turning the egg in different directions, it can be made to touch a flat surface on three points at the same time in many ways. It is not hard to find an orientation such that the egg's center of mass is contained within the triangle spanned by the three contact points, which is the condition for balancing any object. [1] His findings were replicated by astronomer Frank D. Ghigo of the University of Minnesota in 1984. [8] [9]

Writing on the subject, Martin Gardner speculated that the folk beliefs inspired people to "try a little harder, be more patient, and use steadier hands" and possibly even to subconsciously sabotage attempts on other days. He compared the self-reinforcing delusion to a "ouija-board phenomenon". [6]

See also

Related Research Articles

<span class="mw-page-title-main">Ecliptic</span> Apparent path of the Sun on the celestial sphere

The ecliptic or ecliptic plane is the orbital plane of Earth around the Sun. From the perspective of an observer on Earth, the Sun's movement around the celestial sphere over the course of a year traces out a path along the ecliptic against the background of stars. The ecliptic is an important reference plane and is the basis of the ecliptic coordinate system.

A solar equinox is a moment in time when the Sun crosses the Earth's equator, which is to say, appears directly above the equator, rather than north or south of the equator. On the day of the equinox, the Sun appears to rise "due east" and set "due west". This occurs twice each year, around 20 March and 23 September.

<span class="mw-page-title-main">Right ascension</span> Astronomical equivalent of longitude

Right ascension is the angular distance of a particular point measured eastward along the celestial equator from the Sun at the March equinox to the point in question above the Earth. When paired with declination, these astronomical coordinates specify the location of a point on the celestial sphere in the equatorial coordinate system.

A solstice is the time when the Sun reaches its most northerly or southerly excursion relative to the celestial equator on the celestial sphere. Two solstices occur annually, around 20-22 June and 20-22 December. In many countries, the seasons of the year are defined by reference to the solstices and the equinoxes.

<span class="mw-page-title-main">Zodiac</span> Area of the sky divided into twelve signs

The zodiac is a belt-shaped region of the sky that extends approximately 8° north and south of the ecliptic, the apparent path of the Sun across the celestial sphere over the course of the year. Also within this zodiac belt appear the Moon and the brightest planets, along their orbital planes. The zodiac is divided along the ecliptic into 12 equal parts ("signs"), each occupying 30° of celestial longitude. These signs roughly correspond to the astronomical constellations with the following modern names: Aries, Taurus, Gemini, Cancer, Leo, Virgo, Libra, Scorpio, Sagittarius, Capricorn, Aquarius, and Pisces.

<span class="mw-page-title-main">Ecliptic coordinate system</span> Celestial coordinate system used to describe Solar System objects

In astronomy, the ecliptic coordinate system is a celestial coordinate system commonly used for representing the apparent positions, orbits, and pole orientations of Solar System objects. Because most planets and many small Solar System bodies have orbits with only slight inclinations to the ecliptic, using it as the fundamental plane is convenient. The system's origin can be the center of either the Sun or Earth, its primary direction is towards the March equinox, and it has a right-hand convention. It may be implemented in spherical or rectangular coordinates.

<span class="mw-page-title-main">Sidereal time</span> Timekeeping system on Earth relative to the celestial sphere

Sidereal time is a system of timekeeping used especially by astronomers. Using sidereal time and the celestial coordinate system, it is easy to locate the positions of celestial objects in the night sky. Sidereal time is a "time scale that is based on Earth's rate of rotation measured relative to the fixed stars".

<span class="mw-page-title-main">Axial precession</span> Change of rotational axis in an astronomical body

In astronomy, axial precession is a gravity-induced, slow, and continuous change in the orientation of an astronomical body's rotational axis. In the absence of precession, the astronomical body's orbit would show axial parallelism. In particular, axial precession can refer to the gradual shift in the orientation of Earth's axis of rotation in a cycle of approximately 26,000 years. This is similar to the precession of a spinning top, with the axis tracing out a pair of cones joined at their apices. The term "precession" typically refers only to this largest part of the motion; other changes in the alignment of Earth's axis—nutation and polar motion—are much smaller in magnitude.

A solar calendar is a calendar whose dates indicate the season or almost equivalently the apparent position of the Sun relative to the stars. The Gregorian calendar, widely accepted as a standard in the world, is an example of a solar calendar. The main other types of calendar are lunar calendar and lunisolar calendar, whose months correspond to cycles of Moon phases. The months of the Gregorian calendar do not correspond to cycles of the Moon phase.

In astronomy, an epoch or reference epoch is a moment in time used as a reference point for some time-varying astronomical quantity. It is useful for the celestial coordinates or orbital elements of a celestial body, as they are subject to perturbations and vary with time. These time-varying astronomical quantities might include, for example, the mean longitude or mean anomaly of a body, the node of its orbit relative to a reference plane, the direction of the apogee or aphelion of its orbit, or the size of the major axis of its orbit.

<span class="mw-page-title-main">Lunar node</span> Where the orbit of the Moon intersects the Earths ecliptic

A lunar node is either of the two orbital nodes of the Moon, that is, the two points at which the orbit of the Moon intersects the ecliptic. The ascending node is where the Moon moves into the northern ecliptic hemisphere, while the descending node is where the Moon enters the southern ecliptic hemisphere.

<span class="mw-page-title-main">September equinox</span> When sun appears directly over equator

The September equinox is the moment when the Sun appears to cross the celestial equator, heading southward. Because of differences between the calendar year and the tropical year, the September equinox may occur from September 21 to 24.

<span class="mw-page-title-main">March equinox</span> When sun appears directly over equator

The March equinox or northward equinox is the equinox on the Earth when the subsolar point appears to leave the Southern Hemisphere and cross the celestial equator, heading northward as seen from Earth. The March equinox is known as the vernal equinox in the Northern Hemisphere and as the autumnal equinox in the Southern Hemisphere.

<i>Lichun</i> First solar term of East Asian calendars

The traditional Chinese calendar divides a year into 24 solar terms. The first one is known as lichun in Chinese, risshun in Japanese, ipchun in Korean, and lập xuân in Vietnamese. It begins when the Sun reaches the celestial longitude of 315° and ends when it reaches the longitude of 330°. It more often refers in particular to the day when the Sun is exactly at the celestial longitude of 315°. In the Gregorian calendar, it usually begins around February 4 and ends around February 18. It is also the beginning of a sexagenary cycle.

<span class="mw-page-title-main">Lunar standstill</span> Moon stops moving north or south

A lunar standstill or lunistice is when the Moon reaches its furthest north or furthest south point during the course of a month. The declination at lunar standstill varies in a cycle 18.6 years long between 18.134° and 28.725°, due to lunar precession. These extremes are called the minor and major lunar standstills.

<span class="mw-page-title-main">Orbit of the Moon</span> The Moons circuit around Earth

The Moon orbits Earth in the prograde direction and completes one revolution relative to the Vernal Equinox and the stars in about 27.32 days and one revolution relative to the Sun in about 29.53 days. Earth and the Moon orbit about their barycentre, which lies about 4,670 km from Earth's centre, forming a satellite system called the Earth–Moon system. On average, the distance to the Moon is about 385,000 km (239,000 mi) from Earth's centre, which corresponds to about 60 Earth radii or 1.282 light-seconds.

In astronomy, an equinox is either of two places on the celestial sphere at which the ecliptic intersects the celestial equator. Although there are two such intersections, the equinox associated with the Sun's ascending node is used as the conventional origin of celestial coordinate systems and referred to simply as "the equinox". In contrast to the common usage of spring/vernal and autumnal equinoxes, the celestial coordinate system equinox is a direction in space rather than a moment in time.

<span class="mw-page-title-main">Earth-centered inertial</span> Coordinate frames

Earth-centered inertial (ECI) coordinate frames have their origins at the center of mass of Earth and are fixed with respect to the stars. "I" in "ECI" stands for inertial, in contrast to the "Earth-centered – Earth-fixed" (ECEF) frames, which remains fixed with respect to Earth's surface in its rotation, and then rotates with respect to stars.

A tropical year or solar year is the time that the Sun takes to return to the same position in the sky – as viewed from the Earth or another celestial body of the Solar System – thus completing a full cycle of astronomical seasons. For example, it is the time from vernal equinox to the next vernal equinox, or from summer solstice to the next summer solstice. It is the type of year used by tropical solar calendars.

This glossary of astronomy is a list of definitions of terms and concepts relevant to astronomy and cosmology, their sub-disciplines, and related fields. Astronomy is concerned with the study of celestial objects and phenomena that originate outside the atmosphere of Earth. The field of astronomy features an extensive vocabulary and a significant amount of jargon.

References

  1. 1 2 3 Ukichiro Nakaya (February 2001) [1947]. "Egg of Li Chun". Essays (in Japanese). Vol. 5. Iwanami Shoten.
  2. 姜義鎮 (2002-06-03). 《台灣民俗與特產》 (in Chinese (Taiwan)). 臺灣: 武陵出版有限公司. ISBN   957351205X.
  3. "Busted! Top 3 equator line tricks debunked". 26 September 2016.
  4. Huang, Ottavia. Hmmm, This Is What I Think: "Dragon Boat Festival: Time to Balance an Egg". 24 June 2012. Accessed 3 November 2013.
  5. Annalee Jacoby (March 19, 1945). "Eggs Stand on End in Chungking". Life . pp. 36–37.
  6. 1 2 Martin Gardner (May–June 1996). "The great egg-balancing mystery". Skeptical Inquirer . 20 (3). Archived from the original on 2007-02-21.
  7. The New Yorker . 1983-04-04.{{cite magazine}}: Missing or empty |title= (help)
  8. Schmid, Randolph. "Equinox Returns and Eggs Keep Balancing". Associated Press, 20 September 1987. Accessed 3 November 2013.
  9. Mikkelson, David & al. Snopes.com: "Infernal Egguinox". 2012. Accessed 3 November 2013.