logo
June 21 Marks Year's Longest Day: All About the Summer Solstice

June 21 Marks Year's Longest Day: All About the Summer Solstice

Hans India21-06-2025

As the Northern Hemisphere steps into summer, June 21, 2025, stands out as a remarkable astronomical event—welcoming the longest day and the shortest night of the year, known as the summer solstice.
At precisely 8:12 am IST, the solstice occurs when Earth's axis leans at its maximum toward the Sun. This alignment places the Sun directly overhead at the Tropic of Cancer, allowing regions like India, the United States, and Europe to bask in extended daylight. The North Pole, in fact, will witness a full 24 hours of sunlight.
This phenomenon is driven by Earth's 23.5-degree axial tilt, which not only governs the seasons but also determines the length of daylight each region receives throughout the year. The tilt causes the Sun's rays to strike the Northern Hemisphere more directly and for a longer span during the summer solstice.
Interestingly, the solstice date can vary slightly every year due to Earth's orbital period of approximately 365.25 days. This small difference is corrected through leap years, which help sync our calendar with Earth's celestial movements.
While June 21 marks peak sunlight for the Northern Hemisphere, it is quite the opposite for the Southern Hemisphere. Regions as far south as the Antarctic Circle enter polar night—a stretch where the Sun doesn't rise above the horizon at all.
Beyond its scientific relevance, the summer solstice carries deep cultural and historical significance. Civilizations from ancient Egypt to pre-modern Europe have honored this celestial moment. One of the most iconic tributes continues at Stonehenge, where thousands gather to witness the Sun rising through the ancient stone structure—a tradition rooted in millennia.
In India, the solstice also sets the stage for International Yoga Day, observed on the same day. This global celebration emphasizes harmony between mind, body, and the natural world, symbolizing the connection between humanity and the cosmos.
Though June 21 heralds the official start of astronomical summer, it also marks the gradual shortening of days. From June 22 onward, daylight hours begin to wane—reminding us of the Earth's continuous and graceful orbit around the Sun.

Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

Breakthrough: IIA Bengaluru uses dish TV antenna to study Sun
Breakthrough: IIA Bengaluru uses dish TV antenna to study Sun

New Indian Express

timea day ago

  • New Indian Express

Breakthrough: IIA Bengaluru uses dish TV antenna to study Sun

BENGALURU: It is possible to measure the Sun's magnetic field using commercial dish TV antennas. In a major breakthrough to study the Sun, the radio astronomy group at the Indian Institute of Astrophysics (IIA), Bengaluru has proved that low-cost dish antennas that are used for TV networks can be used to observe the Sun and its magnetic field. 'The scientific and technical personnel at IIA, associated with the Gauribidanur radio astronomy field station near Bengaluru, are successfully operating a unique and large world-class radio antenna array for regular observations of the solar corona and magnetic field. The observations are carried out every day unlike the optical observations, where the solar corona can be observed from the ground only during a total solar eclipse. The radio observations are not affected by the clouds,' said Prof R Ramesh, senior professor at IIA. He is in charge of the institute's radio astronomy field station at Gauribidanur and is the principal investigator for the VELC instrument on board Aditya-L1, India's maiden space mission for dedicated observations of the Sun. 'The solar corona overlying the Sun's photosphere as well as present beyond its limb can be observed with a radio telescope. These are unique advantages of radio observations. The antennas used in the array are designed and fabricated in the Gauribidanur observatory workshop. The analog and digital receiver systems are also developed in-house using off-the-shelf components,' he added. While the measurement of the Sun's magnetic field at its visible surface (the photosphere) is routinely carried out with both ground and space-based observational facilities, regular measurements of the extension of the same magnetic field to the outer layers in the Sun's atmosphere like the chromosphere and corona are not there.

Moon-Mars conjunction to dazzle skywatchers
Moon-Mars conjunction to dazzle skywatchers

New Indian Express

time2 days ago

  • New Indian Express

Moon-Mars conjunction to dazzle skywatchers

BENGALURU: Skywatchers are in for a celestial event in the early hours of June 30, when the Moon and Mars will appear unusually close to each other in what astronomers call a conjunction. While such alignments between the Moon and planets occur regularly, this particular one stands out for its timing as Mars edges closer to its opposition later this year, gradually becoming brighter in the night sky. In this phenomena, in the pre-dawn hours, observers with clear skies may witness a slender crescent Moon paired with the reddish glow of Mars, both positioned in the same region of the sky — separated by just about 3 degrees. Although the two bodies are actually million of kilometres apart, they will appear side by side from Earth due to a quirk of orbital alignment. Despite the event's potential, seasoned skywatchers and experts caution that those in Bengaluru and much of India may miss out due to monsoon conditions. 'Cloud cover and moisture-laden air during the early mornings can obscure the eastern horizon where the Moon and Mars will rise,' said an official from the Indian Institute of Astrophysics (IIA), adding that even a thin veil of clouds can completely wash out the view of the crescent Moon.' A conjunction happens when two celestial bodies appear to align in the sky from Earth's perspective. In this case, the Moon, which moves faster along its orbit, catches up and passes near Mars in the background sky. Such close approaches often go unnoticed, but when they involve bright planets and occur during dark-sky hours - like this one - they can create dramatic views. 'This conjunction is unique because of the geometry involved — the thin waning crescent Moon rising shortly before dawn, with Mars just above it, makes for a particularly delicate arrangement,' an official from the IIA said, adding that such well-positioned conjunctions are infrequent. While Moon-planet conjunctions are common, most are either obscured by daylight, occur too close to the horizon, or involve planets that are faint or too close to the Sun. What makes the June 30 event rare is a combination of factors - Mars is steadily brightening, the Moon is in a delicate crescent phase, and the timing - just before sunrise - provides a dark enough sky for good contrast, a senior official from the Jawaharlal Nehru Planetarium explained.

Earth trapping heat has doubled in 20 years
Earth trapping heat has doubled in 20 years

Hans India

time2 days ago

  • Hans India

Earth trapping heat has doubled in 20 years

How do you measure climate change? One way is by recording temperatures in different places over a long period of time. While this works well, natural variation can make it harder to see longer-term trends. But another approach can give us a very clear sense of what's going on: track how much heat enters Earth's atmosphere and how much heat leaves. This is Earth's energy budget, and it's now well and truly out of balance. Our recent research found this imbalance has more than doubled over the last 20 years. Other researchers have come up with similar conclusions. This imbalance is now substantially more than climate models have suggested. In the mid-2000s, the energy imbalance was about 0.6 watts per square metre (W/m2) on average. In recent years, the average was about 1.3 W/m2. This means the rate at which energy is accumulating near the planet's surface has doubled. These findings suggest climate change might well accelerate in the coming years. Worse still, this worrying imbalance is emerging even as funding uncertainty in the United States threatens our ability to track the flows of heat. Energy in, energy out: Earth's energy budget functions a bit like your bank account, where money comes in and money goes out. If you reduce your spending, you'll build up cash in your account. Here, energy is the currency. Life on Earth depends on a balance between heat coming in from the Sun and heat leaving. This balance is tipping to one side. Solar energy hits Earth and warms it. The atmosphere's heat-trapping greenhouse gases keep some of this energy. But the burning of coal, oil and gas has now added more than two trillion tonnes of carbon dioxide and other greenhouse gases to the atmosphere. These trap more and more heat, preventing it from leaving. Some of this extra heat is warming the land or melting sea ice, glaciers and ice sheets. But this is a tiny fraction as 90 per cent has gone into the oceans due to their huge heat capacity. Earth naturally sheds heat in several ways. One way is by reflecting incoming heat of clouds, snow and ice and back out to space. Infrared radiation is also emitted back to space. From the beginning of human civilisation up until just a century ago, the average surface temperature was about 14°C. The accumulating energy imbalance has now pushed average temperatures 1.3-1.5°C higher. Tracking faster than the models: Scientists keep track of the energy budget in two ways. First, we can directly measure the heat coming from the Sun and going back out to space, using the sensitive radiometers on monitoring satellites. This dataset and its predecessors date back to the late 1980s. Second, we can accurately track the build-up of heat in the oceans and atmosphere by taking temperature readings. Thousands of robotic floats have monitored temperatures in the world's oceans since the 1990s. Both methods show the energy imbalance has grown rapidly. Doubling of the energy imbalance has come as a shock, because the sophisticated climate models we use largely didn't predict such a large and rapid change. Typically, the models forecast less than half of the change we're seeing in the real world. Why has it changed so fast? We don't yet have a full explanation. But new research suggests changes in clouds is a big factor. Clouds have a cooling effect overall. But the area covered by highly reflective white clouds has shrunk, while the area of jumbled, less reflective clouds has grown. It isn't clear why the clouds are changing. One possible factor could be the consequences of successful efforts to reduce sulphur in shipping fuel from 2020, as burning the dirtier fuel may have had a brightening effect on clouds. However, the accelerating energy budget imbalance began before this change. Natural fluctuations in the climate system such as the Pacific Decadal Oscillation might also be playing a role. Finally – and most worryingly – the cloud changes might be part of a trend caused by global warming itself, that is, positive feedback on climate change. What does this mean? These findings suggest recent extremely hot years are not one-offs but may reflect a strengthening of warming over the coming decade or longer. This will mean a higher chance of more intense climate impacts from searing heatwaves, droughts and extreme rains on land, and more intense marine heatwaves. This imbalance may lead to worse longer-term consequences. New research shows the only climate models coming close to simulating real world measurements are those with a higher 'climate sensitivity'. We don't know yet whether other factors are at play, however. It's still too early to definitively say we are on a high-sensitivity trajectory. We've known the solution for a long time: stop the routine burning of fossil fuels and phase out human activities causing emissions such as deforestation. Keeping accurate records over long periods of time is essential if we are to spot unexpected changes. Satellites are our advance warning system, telling us about heat storage changes roughly a decade before other methods. But funding cuts and drastic priority shifts may threaten essential satellite climate monitoring. (Steven Sherwood is from UNSW Sydney, Benoit Meyssignac is with the Université de Toulouse and Thorsten Mauritsen is from Stockholm University)

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into a world of global content with local flavor? Download Daily8 app today from your preferred app store and start exploring.
app-storeplay-store