Morning

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Morning on a farm in Namibia, just after sunrise Morning, just after sunrise, Namibia.jpg
Morning on a farm in Namibia, just after sunrise

Morning is the period from sunrise to noon. It is preceded by the twilight period of dawn. There are no exact times for when morning begins (also true of evening and night) because it can vary according to one's lifestyle, latitude, and the hours of daylight at each time of year. [1] However, morning strictly ends at noon, when afternoon starts.

Contents

Morning precedes afternoon, evening, and night in the sequence of a day. Originally, the term referred to sunrise. [2]

Etymology

The Modern English words "morning" and "tomorrow" began in Middle English as morwening, developing into morwen, then morwe, and eventually morrow. English, unlike some other languages, has separate terms for "morning" and "tomorrow", despite their common root. Other languages, like Dutch, Scots and German, may use a single word morgen to signify both "morning" and "tomorrow". [3] [4]

Significance

Cultural implications

Morning prayer is a common practice in several religions. The morning period includes specific phases of the Liturgy of the Hours of Christianity.

Some languages that use the time of day in greeting have a special greeting for morning, such as the English good morning. The appropriate time to use such greetings, such as whether it may be used between midnight and dawn, depends on the culture's or speaker's concept of morning. [5] The use of 'good morning' is ambiguous, usually depending on when the person woke up. As a general rule, the greeting is normally used from 3:00 a.m. to around noon.

Many people greet someone with the shortened 'morning' rather than 'good morning'. It is used as a greeting, never a farewell, unlike 'good night' which is used as the latter. To show respect, one can add the addressee's last name after the salutation: Good morning, Mr. Smith.

For some, the word morning may refer to the period immediately following waking up, irrespective of the current time of day. This modern sense of morning is due largely to the worldwide spread of electricity, and the independence from natural light sources. [6]

Astronomy

Comet Ison at dawn, with Mercury at left Comet ison.jpg
Comet Ison at dawn, with Mercury at left

When a star first appears in the east just prior to sunrise, it is referred to as a heliacal rising. [7] Despite the less favorable lighting conditions for optical astronomy, dawn and morning can be useful for observing objects orbiting close to the Sun. Morning (and evening) serves as the optimum time period for viewing the inferior planets Venus and Mercury. [8] Venus and sometimes Mercury may be referred to as a morning star when they appear in the east prior to sunrise. It is a popular time to hunt for comets, as their tails grow more prominent as these objects draw closer to the Sun. [9] The morning (and evening) twilight is used to search for near-Earth asteroids that orbit inside the orbit of the Earth. [10] In mid-latitudes, the mornings near the autumnal equinox are a favorable time period for viewing the zodiacal light. [11]

Genetics

For people, the morning period may be a period of enhanced or reduced energy and productivity. The ability of a person to wake up effectively in the morning may be influenced by a gene called "Period 3". This gene comes in two forms, a "long" and a "short" variant. It seems to affect the person's preference for mornings or evenings. People who carry the long variant were over-represented as morning people, while the ones carrying the short variant were evening preference people. [12]

See also

Related Research Articles

A day is the time period of a full rotation of the Earth with respect to the Sun. On average, this is 24 hours. As a day passes at a given location it experiences morning, noon, afternoon, evening, and night. This daily cycle drives circadian rhythms in many organisms, which are vital to many life processes.

<span class="mw-page-title-main">Solar System</span> The Sun and objects orbiting it

The Solar System is the gravitationally bound system of the Sun and the objects that orbit it. It formed about 4.6 billion years ago when a dense region of a molecular cloud collapsed, forming the Sun and a protoplanetary disc. The Sun is a typical star that maintains a balanced equilibrium by the fusion of hydrogen into helium at its core, releasing this energy from its outer photosphere. Astronomers classify it as a G-type main-sequence star.

The zodiacal light is a faint glow of diffuse sunlight scattered by interplanetary dust. Brighter around the Sun, it appears in a particularly dark night sky to extend from the Sun's direction in a roughly triangular shape along the zodiac, and appears with less intensity and visibility along the whole ecliptic as the zodiacal band. Zodiacal light spans the entire sky and contributes to the natural light of a clear and moonless night sky. A related phenomenon is gegenschein, sunlight backscattered from the interplanetary dust, which appears directly opposite to the Sun as a faint but slightly brighter oval glow.

<span class="mw-page-title-main">2 Pallas</span> Third-largest asteroid

Pallas is the third-largest asteroid in the Solar System by volume and mass. It is the second asteroid to have been discovered, after Ceres, and is likely a remnant protoplanet. Like Ceres, it is believed to have a mineral composition similar to carbonaceous chondrite meteorites, though significantly less hydrated than Ceres. It is 79% the mass of Vesta and 22% the mass of Ceres, constituting an estimated 7% of the mass of the asteroid belt. Its estimated volume is equivalent to a sphere 507 to 515 kilometers in diameter, 90–95% the volume of Vesta.

The heliacal rising of a star or a planet occurs annually when it becomes visible above the eastern horizon at dawn just before sunrise. A heliacal rising marks the time when a star or planet becomes visible for the first time again in the night sky after having set with the Sun at the western horizon in a previous sunset, having since been in the sky only during daytime, obscured by sunlight.

<span class="mw-page-title-main">Sunrise</span> Time of day when the sun appears above the horizon

Sunrise is the moment when the upper rim of the Sun appears on the horizon in the morning, at the start of the Sun path. The term can also refer to the entire process of the solar disk crossing the horizon.

<span class="mw-page-title-main">Dawn</span> Time that marks the beginning of the twilight before sunrise

Dawn is the time that marks the beginning of twilight before sunrise. It is recognized by the appearance of indirect sunlight being scattered in Earth's atmosphere, when the centre of the Sun's disc has reached 18° below the observer's horizon. This morning twilight period will last until sunrise, when direct sunlight outshines the diffused light.

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">Regulus</span> Brightest star in the constellation Leo

Regulus is the brightest object in the constellation Leo and one of the brightest stars in the night sky. It has the Bayer designation designated α Leonis, which is Latinized to Alpha Leonis, and abbreviated Alpha Leo or α Leo. Regulus appears singular, but is actually a quadruple star system composed of four stars that are organized into two pairs. The spectroscopic binary Regulus A consists of a blue-white main-sequence star and its companion, which has not yet been directly observed, but is probably a white dwarf. The system lies approximately 79 light years from the Sun.

<span class="mw-page-title-main">Vulcanoid</span> Hypothetical asteroids orbiting the Sun

The vulcanoids are a hypothetical population of asteroids that orbit the Sun in a dynamically stable zone inside the orbit of the planet Mercury. They are named after the hypothetical planet Vulcan, which was proposed on the basis of irregularities in Mercury's orbit that were later found to be explained by general relativity. So far, no vulcanoids have been discovered, and it is not yet clear whether any exist.

<span class="mw-page-title-main">Twilight</span> Atmospheric illumination by the Sun below the horizon

Twilight is sunlight illumination produced by diffuse sky radiation when the Sun is below the horizon as sunlight from the upper atmosphere is scattered in a way that illuminates both the Earth's lower atmosphere and also the Earth's surface. Twilight also is any period when this illumination occurs.

<span class="mw-page-title-main">1566 Icarus</span> Asteroid

1566 Icarus is a large near-Earth object of the Apollo group and the lowest numbered potentially hazardous asteroid. It has an extremely eccentric orbit (0.83) and measures approximately 1.4 km (0.87 mi) in diameter. In 1968, it became the first asteroid ever observed by radar. Its orbit brings it closer to the Sun than Mercury and further out than the orbit of Mars, which also makes it a Mercury-, Venus-, and Mars-crossing asteroid. This stony asteroid and relatively fast rotator with a period of 2.27 hours was discovered on 27 June 1949, by German astronomer Walter Baade at the Palomar Observatory in California. It was named after the mythological Icarus.

<span class="mw-page-title-main">Night sky</span> Appearance of the sky in a clear night

The night sky is the nighttime appearance of celestial objects like stars, planets, and the Moon, which are visible in a clear sky between sunset and sunrise, when the Sun is below the horizon.

<span class="mw-page-title-main">Evening</span> Period of the day

Evening is the period of a day that begins at the end of daylight and overlaps with the beginning of night. It generally indicates the period of time when the sun is close to the horizon and comprises the periods of civil, nautical and astronomical twilight. The exact times when evening begins and ends are subjective and depend on location and time of year. It may be used colloquially to include the last waning daytime shortly before sunset.

The interplanetary dust cloud, or zodiacal cloud, consists of cosmic dust that pervades the space between planets within planetary systems, such as the Solar System. This system of particles has been studied for many years in order to understand its nature, origin, and relationship to larger bodies. There are several methods to obtain space dust measurement.

<span class="mw-page-title-main">Discovery and exploration of the Solar System</span>

Discovery and exploration of the Solar System is observation, visitation, and increase in knowledge and understanding of Earth's "cosmic neighborhood". This includes the Sun, Earth and the Moon, the major planets Mercury, Venus, Mars, Jupiter, Saturn, Uranus, and Neptune, their satellites, as well as smaller bodies including comets, asteroids, and dust.

<span class="mw-page-title-main">Great Comet of 1901</span> Hyperbolic comet

The Great Comet of 1901, sometimes known as Comet Viscara, formally designated C/1901 G1, was a comet which became bright in the spring of 1901. Visible exclusively from the southern hemisphere, it was discovered on the morning of April 12, 1901 as a naked-eye object of second magnitude with a short tail. On the day of perihelion passage, the comet's head was reported as deep yellowish in color, trailing a 10-degree tail. It was last seen by the naked eye on May 23.

<span class="mw-page-title-main">C/2012 F6 (Lemmon)</span> Non-periodic comet

C/2012 F6 (Lemmon) is a long-period comet discovered in Leo on 23 March 2012, by A. R. Gibbs using the 1.5-m reflector at the Mt. Lemmon Survey, located at the summit of Mount Lemmon in the Santa Catalina Mountains north of Tucson, Arizona, USA. Initially, the object was considered to be of asteroidal nature before later observations confirmed its cometary appearance. Comet Lemmon has a highly eccentric orbit, bringing it as close to 0.73 AU from the Sun at perihelion and as far as 973 AU from the Sun at aphelion. This also leads to the comet's long-period nature with an orbital period of approximately 8,000 years based on epoch 2050. The comet last reached perihelion on 24 March 2013.

Maya astronomy is the study of the Moon, planets, Milky Way, Sun, and astronomical phenomena by the Precolumbian Maya civilization of Mesoamerica. The Classic Maya in particular developed some of the most accurate pre-telescope astronomy in the world, aided by their fully developed writing system and their positional numeral system, both of which are fully indigenous to Mesoamerica. The Classic Maya understood many astronomical phenomena: for example, their estimate of the length of the synodic month was more accurate than Ptolemy's, and their calculation of the length of the tropical solar year was more accurate than that of the Spanish when the latter first arrived. Many temples from the Maya architecture have features oriented to celestial events.

<span class="mw-page-title-main">594913 ꞌAylóꞌchaxnim</span> First known asteroid of the Vatira population

594913 ꞌAylóꞌchaxnim (provisional designation 2020 AV2) is a large near-Earth asteroid discovered by the Zwicky Transient Facility on 4 January 2020. It is the first asteroid discovered to have an orbit completely within Venus's orbit, and is thus the first and only known member of the eponymous ꞌAylóꞌchaxnim (informally named Vatira before its discovery) population of Atira-class asteroids. ꞌAylóꞌchaxnim has the smallest known aphelion and third-smallest known semi-major axis among all asteroids. With an absolute magnitude approximately 16.2, the asteroid is expected to be larger than 1 km in diameter.

References

  1. Learner's Dictionary
  2. Online Etymology Dictionary
  3. Origin of the phrase "Good Morning Archived 2012-02-03 at the Wayback Machine
  4. Etymology of the word "morning"
  5. "Definition of good morning | Dictionary.com". www.dictionary.com. Retrieved 2019-12-31.
  6. "Why some of us are early risers". BBC News. London. 2003-06-17. Retrieved 2008-01-30.
  7. Schaefer, Bradley E. (1987). "Heliacal Rise Phenomena". Journal for the History of Astronomy, Archaeoastronomy Supplement. 18 (11): S19. Bibcode:1987JHAS...18...19S. doi:10.1177/002182868701801103.
  8. Grego, Peter (2008). "Recording Mercury and Venus". Venus and Mercury, and How to Observe Them. Astronomers’ Observing Guides. New York, NY.: Springer. pp. 177–206. doi:10.1007/978-0-387-74286-1_5. ISBN   978-0-387-74285-4.
  9. Marsden, B. G. (1994). Milani, Andrea; Di Martino, Michel; Cellino, A. (eds.). Search Programs for Comets. Asteroids, Comets, Meteors 1993: Proceedings of the 160th Symposium of the International Astronomical Union, held in Belgirate, Italy, June 14-18, 1993. International Astronomical Union. Symposium no. 160. Dordrecht: Kluwer Academic Publishers. p. 1. Bibcode:1994IAUS..160....1M.
  10. Ye, Quanzhi; et al. (February 2020). "A Twilight Search for Atiras, Vatiras, and Co-orbital Asteroids: Preliminary Results". The Astronomical Journal. 159 (2): 70. arXiv: 1912.06109 . Bibcode:2020AJ....159...70Y. doi: 10.3847/1538-3881/ab629c . 70.
  11. Cladera, Antoni. "Zodiacal Light: The Definitive Photography Guide". photopills.com. Retrieved 2023-03-14.
  12. Gene determines sleep patterns