Sunrise and sunset times in New Kensington (2024)

Calculation of data (6/20/2024UTC−04:00)

The beginning of the astronomical night is the moment when the sun drops below the horizon below 18 degrees.

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The end of the astronomical night is the moment when the sun is less than 18 degrees below the horizon.

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Distance from Earth to Sun — the distance from the center of Earth to the center of Sun.

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Astronomical twilight — the period of time during which the sun is below the horizon, and the natural illumination on Earth is provided by the reflection of sunlight from the upper atmosphere. The interval of the angle of the sun under the horizon from 12 ° to 18 °. Usually, astronomers can already observe celestial bodies at this time.

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Astronomical night does not occur on this date - the sun does not fall below 18 ° from the horizon (or does not rise, in the case of a polar night).

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Sunrise Time — the moment when the upper edge of the solar disk becomes visible on the horizon. This parameter depends on many factors, such as the location and height of the observer above sea level, the presence of obstacles on the horizon (mountains, houses), atmospheric refraction, and others.

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The sun does not rise on this date (the sun does not rise above the horizon)

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The sun does not set on this date (the sun does not drop below the horizon)

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Sunset Time — is the point in time when the solar disk is completely hidden behind the horizon line. This parameter, like sunrise, depends on the latitude and longitude of the observer, so it is important to indicate your exact location.

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Astronomical night does not occur on this date - the sun does not fall below 18 ° from the horizon (or does not rise, in the case of a polar night).

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Astronomical twilight — the period of time during which the sun is below the horizon, and the natural illumination on Earth is provided by the reflection of sunlight from the upper atmosphere. The interval of the angle of the sun under the horizon from 12 ° to 18 °. Usually, astronomers can already observe celestial bodies at this time.

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Nadir (Antizenith) — is a point in the celestial sphere located under the horizon, opposite the zenith. In relation to the sun, this is the lowest point reached by the sun in its orbit, relative to the observer.

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Julian date — is an astronomical method of measuring time, which counts the number of days that have passed since Monday noon, January 1, 4713 BC Julian calendar (or from November 24, 4713 Gregorian calendar, which is the same).

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Local time is determined for a specific place on Earth, depending on geographic longitude. Usually, it is the same for all settlements located on the same meridian.

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Universal Time (or Coordinated Universal Time, UTC) is an atomic time scale that approximates the UT1 standard (calculated in proportion to the angle of rotation of the Earth relative to the international celestial coordinate system ICRS), on which time zone time is based. UTC witness synchronously with international atomic time.

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Daylight hours — the time interval between sunrise and sunset. During this period, at least part of the solar disk should be above the horizon.

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Sunrise Direction — the angle counted counterclockwise between the direction to the south and the sunrise point is always negative.

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Sunset Direction — the angle counted in a clockwise direction between the direction south and the point of sunset. Is always positive.

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The vernal equinox — is an astronomical phenomenon when the sun, in its visible motion along the ecliptic, crosses the celestial equator. In other words, on the day of the vernal equinox, day is almost equal to night, while the length of daylight continues to grow.

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The Summer Solstice — is the moment when the Sun, in its movement along the ecliptic, enters its northernmost point in the northern hemisphere, or the southernmost point in the southern hemisphere. The summer solstice is the longest daylight hours of the year (and the shortest night).

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Autumnal equinox — is an astronomical phenomenon, when the Sun in its visible motion along the ecliptic crosses the celestial equator. In other words, on the day of the autumnal equinox, the day is almost equal to night, while the duration of daylight hours decreases with each subsequent day.

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Winter Solstice — is the day of the year when the Sun passes through the southernmost point of the ecliptic in the northern hemisphere (or through the northernmost point in the southern hemisphere). The winter solstice is the shortest daylight and the longest night.

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Blue hour — a period of time shortly before sunrise (or after sunset), when the sky turns intense blue, due to which saturated blue shades begin to prevail in natural light.

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Golden hour — the period of time when the sun is close to the horizon (immediately after sunrise or shortly before sunset), while natural light gives a soft and rich golden color.

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Blue hour — a period of time shortly before sunrise (or after sunset), when the sky turns intense blue, due to which saturated blue shades begin to prevail in natural light.

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Golden hour — the period of time when the sun is close to the horizon (immediately after sunrise or shortly before sunset), while natural light gives a soft and rich golden color.

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The elevation of the sun — is the angle between the horizon and the position of the Sun in the sky at a certain point in time, measured in degrees. If the sun is below the horizon, the height becomes negative. Measured perpendicularly horizon plane.

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Hour angle — the angle between the south point and the position of the sun in the sky, measured along the horizon in a clockwise direction.

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Sunrise and sunset times in New Kensington (2024)

FAQs

Sunrise and sunset times in New Kensington? ›

Sunrise/Sunset Calculations

Then the UTC time of sunrise (or sunset) in minutes is: sunrise = 720 – 4*(longitude + ha) – eqtime where longitude and hour angle are in degrees and the equation of time is in minutes.

How to solve sunrise and sunset? ›

Sunrise/Sunset Calculations

Then the UTC time of sunrise (or sunset) in minutes is: sunrise = 720 – 4*(longitude + ha) – eqtime where longitude and hour angle are in degrees and the equation of time is in minutes.

What causes these sunrise and sunset times to be regular and predictable responses? ›

The changing position of the Sun in the sky over the course of a day is mainly an effect of the Earth's rotation on its axis, which is quite uniform to a small fraction of a second. However, where the Sun appears in the sky at any given time is also affected by the position of the Earth in its orbit around the Sun.

How accurate are sunrise and sunset predictions? ›

Regardless of model, she concluded, sunrise and sunset times can't be reliably predicted to better than 2 minutes. Two minutes might sound inconsequential, but Wilson noted that, if GPS fails, sailors will use celestial navigation.

Why do we see sunrise before 2 minutes of the actual sunrise and sunset after 2 minutes? ›

It is because of atmospheric refraction. When the Sun is slightly below the horizon, the light coming from it travels from less dense to more dense air and is refracted downwards. Thus, the Sun appears to be raised and can be seen 2 min before actual sunrise and 2 min after actual sunset.

How are sunrise and sunset determined? ›

The timekeeper for the United States, the Naval Observatory, defines sunrise and sunset as the moments when the center of the Sun is physically 50 minutes of arc below the horizon, which is less than the width of your finger held at arm's length.

How to calculate the equation of time? ›

So mean time is indicated by the mean Sun, and apparent solar time is indicated by the actual Sun and is, for example, measured by sundials. The precise definition of the Equation of Time is E = GHA (apparent Sun) - GHA (mean Sun) (1) where GHA is the Greenwich hour angle.

What factors affect sunrise and sunset times? ›

Variables That Affect Sunrise and Sunset Times Where You Live. That's because sunrise and sunset times depend on a number of variables, including longitude, latitude, altitude, and location in relationship to your specific Time Zone.

Which country sees the sun first? ›

Specifically, Kiribati's easternmost uninhabited island, Millennium Island, also known as Caroline Island, is often the first place on Earth to welcome the sun.

What influences sunset and sunrise? ›

But it appears to rise and set because of the Earth's rotation on its axis. It makes one complete turn every 24 hours. It turns toward the east. As the Earth rotates toward the east, it looks like the sun is moving west.

Can people tell the difference between sunrise and sunset? ›

Most people can usually tell quite quickly whether the colors of the sky signify morning or evening based on where the sun is or whether it's appearing or disappearing.

What time does the sunset look best? ›

Sunset: The best time to get that color is roughly 15-20 minutes AFTER the sun has gone below the horizon!

What conditions make the best sunsets? ›

The following factors are helpful in helping you predict if a sunset will be beautiful or not. The air should be clean with relatively low humidity, and the best sunsets typically happen when you have mid and high-level clouds covering around 25% to 60% of the evening sky.

What is the 30 minutes prior to sunrise and 30 minutes after sunset called? ›

In its most general sense, twilight is the period of time before sunrise and after sunset, in which the atmosphere is partially illuminated by the sun, being neither totally dark or completely lit.

Why does the Sun look red at sunrise and sunset? ›

Red light scatters the least by the molecules present in the air. So at sunrise and sunset, the sunlight travels a longer path through the atmosphere to reach our eyes. The blue light scatters the most and has been mostly removed, leaving the red light remaining which reaches our eyes, hence it appears red. Q.

What is the reason behind 2 minutes early sunrise and delayed sunset? ›

Advanced sunrise and delayed sunset are phenomena caused due to atmospheric refraction. In this the Sun appears to rise early by 2 minutes and set late by 2 minutes.

How to calculate sunrise and sunset using latitude? ›

To calculate the sunrise hour angle:
  1. Find the latitude and day of the year, n .
  2. Estimate the declination angle of the Sun using the equation: ...
  3. Multiply the tangents of latitude and declination angle.
  4. Find the cosecant inverse for the negative of the product.
Jan 18, 2024

How does Google calculate sunrise and sunset? ›

Unlike the weather, sunrises and sunsets are quite predictable, and as a result, we don't use a data source. Instead, we calculate sunrise and sunset times based on latitude, longitude and the current time.

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