What If? Lab
What if the Sun stayed low in the sky?
In winter the Sun stays low in the sky. Low sunshine is weaker. Let's find out why in Olly's lab!
A low Sun spreads its light thinly over more ground, and in winter it is up for fewer hours too. In our sunlight model, London's noon Sun drops from about 62 degrees in June to about 15 degrees in December, and its daily sunlight falls to about one seventh.
A beam arriving at altitude a spreads over 1/sin a times the area it would cover overhead. In London that factor grows from 1.13 at the June noon (61.9°) to 3.84 at the December noon (15.1°). Combined with daylight falling from 16.4 to 7.6 h, daily top-of-atmosphere insolation drops from 497 to 73 W/m²: a factor of 6.8.
The big question
In summer the Sun climbs high in the sky. In winter it stays low.
Does it matter how high the Sun is? What if it stayed low all day?
On a winter afternoon the Sun hangs low, shadows stretch long across the ground, and even on a clear day the sunshine feels weak. In summer the noon Sun is high and the light feels strong.
It is the same Sun. So why does a low Sun warm us so much less? In this lab you can keep a town in place, slide the date from June to December, and watch how the Sun's height and the sunlight it delivers change.
Earth's distance from the Sun changes only a little through the year, and NASA Space Place notes that this change does not make much difference to our weather. Yet a mid-latitude town receives far less solar energy per day in winter than in summer.
This lab separates the two causes: the angle at which sunlight strikes the ground and the number of daylight hours. Using London at 51.5°N, how much does each contribute to the drop in daily insolation between the solstices?
Try the experiment
Make a prediction
In December, London's Sun stays low. How much daily sunshine does London get compared with June?
On December 21 London's noon Sun is about 15 degrees high instead of about 62. How much daily sunlight does the model give, compared with June 21?
Between day 172 and day 355 at 51.5°N, by roughly what factor does the model's daily insolation fall?
- About the same
- About half
- About one seventh
| Control | In our world | What ifโฆ | Range |
|---|---|---|---|
| Day of the year ยท Which day of the year it is. Day 172 is about June 21, when London's noon Sun is highest; day 355 is about December 21, when it is lowest. | 172 | 355 | 1โ365 |
| Where you live (latitude) ยท How far north (+) or south (−) of the equator you are. London is 51.5°N. | 51.5 ° | — | -90โ90 ° |
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What the model shows
In the model, London's December Sun is much lower than in June.
In this model, London's noon Sun is about 62 degrees high on June 21 but about 15 degrees on December 21.
At 51.5°N the model's noon altitude is 61.9° on day 172 and 15.1° on day 355 (minimum 15.06° on day 354).
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What the model shows
In the model, London gets much less sunshine in December.
In this model, London's daily sunlight drops from 497 to 73 watts per square meter, about one seventh, as the days shorten from 16.4 to 7.6 hours.
Daily top-of-atmosphere insolation falls from 497 to 73 W/m² (×1/6.8); the noon beam-spreading factor alone rises 3.4 times.
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Established fact
Low sunshine spreads out over more ground, so it warms less.
In winter, sunlight is spread over a larger area, so the ground receives less heat (Bureau of Meteorology).
Winter sunlight is spread over a larger area, delivering less heat to the ground (Bureau of Meteorology); summer combines more direct light with longer days (NASA).
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Established fact
Winter is not because Earth is far from the Sun.
Earth is closest to the Sun in January, so a low winter Sun, not distance, makes northern winter cold (NASA).
Perihelion falls in January (NASA Space Place); seasonal change comes from the tilt-driven Sun angle and day length.
In our world
In London in June, the Sun climbs high at lunchtime.
It shines for more than 16 hours. The sunshine is strong and warm.
Start in London, at 51.5° north, on June 21. In the model the noon Sun climbs to about 62 degrees and stays up for 16.4 hours. Every square meter at the top of the atmosphere gets an average of 497 watts of sunlight over the whole day.
The Met Office says summer in the UK, June to August, brings the hottest temperatures and sunniest days.
At 51.5°N on day 172 the model gives a noon altitude of 61.9°, 16.4 h of daylight and a daily-mean insolation of 497 W/m², 115 percent of the equator's equinox value.
NASA's energy budget explains that in the summer hemisphere the combination of more direct sunlight and longer days increases the incoming solar energy; the Met Office puts the UK's summer in June to August.
Keep the Sun low
Now Olly moves the date to December. The Sun stays low all day.
It is up for less than 8 hours. The sunshine is much weaker. Brr!
Now move the date to December 21 and keep the town where it is. The noon Sun only reaches about 15 degrees, and it is up for just 7.6 hours.
The daily sunlight falls from 497 to 73 watts per square meter, about one seventh. Watch the chart of the noon Sun through the year: it rises to its highest around June 21 and sinks to its lowest around December 21.
On day 355 at 51.5°N the noon altitude is 15.1° (the year's minimum, 15.06° on day 354), daylight 7.6 h and insolation 73 W/m², 17 percent of the equator's equinox value.
The ratio 497/73 = 6.8 splits into two parts. At noon, the beam-spreading factor 1/sin a rises from 1.13 to 3.84, about 3.4 times; the shorter, lower day accounts for the rest.
Why it happens
Shine a flashlight straight down. You get a small, bright spot.
Tip the flashlight low. The spot gets big and dim. A low Sun is like that!
Imagine shining a flashlight straight down at the floor: you get a small, bright circle. Tip it low and the same light stretches into a big, dim oval. The Bureau of Meteorology explains that in winter, sunlight is spread over a larger area, so the ground receives less heat.
In London in December, each beam of noon sunlight covers almost four times as much ground as it would from straight overhead. And with only 7.6 hours of daylight, there is less time to soak it up.
Irradiance on a horizontal surface is S·sin a, where a is the Sun's altitude. At 61.9° that is 88 percent of the beam; at 15.1° only 26 percent. Integrating over the day gives the model's daily mean Q = (S₀/π)(h₀ sin φ sin δ + cos φ cos δ sin h₀).
The low winter Sun comes from Earth's tilt: in December the Northern Hemisphere leans away from the Sun. NASA Space Place notes that Earth is actually closest to the Sun in January, so distance is not the cause. The model gives sunlight at the top of the atmosphere; air and clouds are not included.
Living with a low Sun
When the Sun is low, your shadow is very long!
In winter, the far north gets even less sunshine than London.
You can see the low Sun in your shadow. Trigonometry gives the noon shadow of a 1-meter stick from the model's Sun heights: about half a meter in London in June, but almost four meters in December.
The Met Office says the UK's winter months, December to February, are the coldest of the year, with the shortest days. Go farther north and it gets more extreme: at 60° north, the model's December noon Sun is under 7 degrees high and the day lasts 5.5 hours.
A vertical stick of height h casts a noon shadow h/tan a: 0.53 h at 61.9° and 3.71 h at 15.1°, a practical way to measure the Sun's altitude.
The Met Office relates the seasons to how directly the Sun's heat reaches the hemisphere tilted toward it, and the Bureau of Meteorology to sunlight spread over a larger area in winter. At 60°N on day 355 the model gives a 6.6° noon Sun, 5.5 h of daylight and 24 W/m².
Amazing facts
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In December, London's noon shadow can be almost four times as long as you are tall.
From the model's December Sun height, a 1-meter stick in London casts a noon shadow almost 4 meters long; in June it is about half a meter.
Noon shadow length is h/tan a: 3.71 h at London's December 15.1°, 0.53 h at its June 61.9°.
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Earth is closest to the Sun in January, in the middle of northern winter.
NASA says Earth is about 91.4 million miles from the Sun in January and about 94.5 million miles in July.
Perihelion (about 91.4 million miles) is in January and aphelion (about 94.5 million) in July (NASA Space Place).
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The farther north you go, the lower the winter Sun.
In the model, at 60° north the December noon Sun is less than 7 degrees high and the day lasts only about 5.5 hours.
At 60°N on day 355 the model gives a 6.6° noon Sun, 5.5 h of daylight and 24 W/m², a third of London's 73.
Words to know
- solar altitude
- how high the Sun is above the horizon, in degrees
- insolation
- how much sunlight reaches a surface, here averaged over a whole day
- solstice
- the day of the year with the longest or shortest daylight
- watt per square meter
- a measure of how much light energy lands on each square meter every second
- tilt
- a lean; Earth's axis leans by about 23.5 degrees
Discovery challenge
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Why is low sunshine weaker?
Why does a low Sun warm the ground less than a high Sun?
Horizontal irradiance from a low Sun is smaller mainly because…
- Its light is spread over more ground
- The Sun is farther away
- The Sun gives out less light
Show the answer
Its light is spread over more ground
The light spreads out over a bigger space, like a tipped flashlight.
The same beam is spread over a larger area, so each patch of ground gets less.
…it scales with sin a; the beam is spread over 1/sin a times the area.
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When is London's noon Sun lowest?
In the model, around which day is London's noon Sun lowest?
At 51.5°N the model's minimum noon altitude occurs…
- Around December 21
- Around June 21
- Around March 21
Show the answer
Around December 21
Around December 21, in winter.
Around December 21: about 15 degrees.
…at the December solstice: 15.06° on day 354, 15.1° on day 355.
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In the model, how much sunshine does London get in December, compared with June?
In the model, London's daily sunlight on December 21 is about what fraction of June 21's?
The ratio of the model's daily insolation at 51.5°N, day 355 to day 172, is about…
- About one seventh
- About half
- About the same
Show the answer
About one seventh
Much less: about one seventh.
About one seventh: 73 against 497 watts per square meter.
…1/6.8 (73/497 W/m²).
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What keeps the winter Sun low?
What keeps the Sun low in a northern winter?
The low December Sun at 51.5°N is a consequence of…
- Earth's tilt
- Earth being far from the Sun
- Clouds
Show the answer
Earth's tilt
Earth leans, and in December our half leans away.
Earth's tilt: in December the north leans away from the Sun. Earth is actually closest in January.
…the axial tilt (δ = −23.4°); perihelion is in January.
Experiments to try
- Watch Try it What If? Lab What if Earth’s tilt changed? Earth's axis leans 23.4 degrees, and that lean is what gives us seasons. Straighten Earth up in our sunlight model and the Sun climbs to the same height every noon, every day lasts 12 hours, and summer and winter disappear.
- Watch Try it What If? Lab What if Earth spun on its side like Uranus? Earth's spin axis leans 23.44 degrees, which gives us gentle seasons. Tip it all the way over to 90 degrees, like Uranus, and each pole points at the Sun in turn. In our model, a place 60 degrees north would get about four months of non-stop daylight, then about four months with no sunrise at all.
- Watch Try it What If? Lab What if June were winter? Earth's two halves take turns leaning toward the Sun, so they have opposite seasons. In our sunlight model, on June 21 London gets 16.4 hours of daylight and a high Sun, while Sydney, south of the equator, gets just 9.7 hours and a low Sun: its shortest day of the year.
Explore next
- Watch Try it What If? Lab What if Earth’s tilt changed? Earth's axis leans 23.4 degrees, and that lean is what gives us seasons. Straighten Earth up in our sunlight model and the Sun climbs to the same height every noon, every day lasts 12 hours, and summer and winter disappear.
- Watch Try it What If? Lab What if Earth spun on its side like Uranus? Earth's spin axis leans 23.44 degrees, which gives us gentle seasons. Tip it all the way over to 90 degrees, like Uranus, and each pole points at the Sun in turn. In our model, a place 60 degrees north would get about four months of non-stop daylight, then about four months with no sunrise at all.
- Watch Try it What If? Lab What if June were winter? Earth's two halves take turns leaning toward the Sun, so they have opposite seasons. In our sunlight model, on June 21 London gets 16.4 hours of daylight and a high Sun, while Sydney, south of the equator, gets just 9.7 hours and a low Sun: its shortest day of the year.
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Watch
City
London
London, the capital of the United Kingdom, began as a Roman town almost 2,000 years ago. About 8.8 million people lived in Greater London in 2021. It has the Tower of London, Big Ben, Tower Bridge and the Tube, an underground railway that opened in 1863.
- Watch Try it What If? Lab What if Earth had no atmosphere? Earth's air works like a jacket: it keeps heat in and carries it around. Take the air away in our model of a sandy patch of ground on the equator, and the coldest part of the night drops from about 13 °C to about 2 °C.
- Watch Try it What If? Lab What if there were no greenhouse gases? Greenhouse gases such as carbon dioxide and water vapor hold some of Earth's heat in, like a blanket. Take them all away in our energy-balance model and Earth's average temperature falls from about 15 °C to about −19 °C, well below freezing.
- Watch Try it What If? Lab What if there were more greenhouse gases? Adding greenhouse gases makes it harder for Earth's heat to escape, so the planet warms until it balances again. In our model a small change in how freely heat escapes warms Earth by about 2.6 °C, and the oceans make the warming take years.
- Watch Try it What If? Lab What if Earth were covered in ice? White ice bounces sunlight back to space, so an icy planet soaks up less of the Sun's warmth. In our energy-balance model, making Earth reflect 60 percent of its sunlight instead of 30 percent drops its average temperature from about 15 °C to about −23 °C.
For parents & teachers
What children will learn
- The Sun's height in the sky changes through the year because of Earth's tilt.
- A low Sun spreads its light over more ground, so each patch gets less energy.
- Winter is darker and colder because of a low Sun and short days together.
- Shadow length is a simple way to measure how high the Sun is.
Recommended ages: 11 to 17 ยท About 20 minutes
Talk about it
- How could you use a shadow to tell what season it is?
- Why might solar panels in winter be tilted more steeply toward the Sun?
- If Earth's distance from the Sun doesn't cause winter, why do many people think it does?
Try at home or in class
- Shine a flashlight onto squared paper straight down, then tipped low. Count how many squares each spot covers.
- Stand a stick upright outdoors and measure its shadow at noon once a month. Graph the lengths through the year.
Key vocabulary: solar altitude, insolation, solstice, watt per square meter, tilt
Where these facts come from
- Solstices, equinoxes and the seasons , Australian Government Bureau of Meteorology
- Climate and Earth's Energy Budget , NASA Earth Observatory
- Our seasons , Met Office
- What Causes the Seasons? , NASA Space Place
Checked, not yet human-reviewed. Last updated October 27, 2026. Spotted a mistake? Tell us.