A space tool went to the Moon.
It took new pictures. It saw the side we cannot see. These pictures showed big hills. It helps us learn about space. Do you like the Moon?
A space tool went to the Moon in 1959.
It was the first to see the far side. This side is hidden from our eyes on Earth.
The tool took 29 new pictures. These pictures showed many big hills. The far side looks different than the side we see.
It found two dark spots on the Moon. These spots looked like seas.
The tool sent the pictures back to Earth. People all over the world saw them. It was a very big discovery.
In 1959, a Soviet spacecraft named Luna 3 went to the Moon.
It was a very special mission. It was the first to photograph the far side of the Moon. This is the side that we cannot see from Earth.
Luna 3 used a special tool called the Yenisey-2 imaging system. This system had two lenses for its camera. The camera took 29 pictures over 40 minutes. These photos showed that the far side looks different. It has many mountains. It also has only two dark areas.
These dark areas are called maria, which means seas. One was named Mare Moscoviense. The other was Mare Desiderii.
To get home, the craft used a gravity assist. This is a way to change a path using gravity. The Moon's gravity pulled on the craft. This helped it fly back toward Earth.
The craft sent 17 pictures back to Earth. People all over the world were excited to see them. These new views helped make the first map of the far side.
In 1959, a Soviet spacecraft named Luna 3 went on a historic journey.
It was the first mission to photograph the far side of the Moon. This is the side of the Moon that stays hidden from Earth. People had never seen these views before. The mission was part of a larger group of missions called the Luna programme. Luna 3 was the third Soviet probe sent toward the Moon. It changed how we understand our closest neighbor in space.
The spacecraft worked using a clever imaging system called Yenisey-2.
It had two different lenses to take pictures. One lens could see the whole Moon at once. The other lens could zoom in on specific spots. After the camera took a photo, the film moved to an onboard processor. This system developed, fixed, and dried the film right there in space. Then, a scanner turned the pictures into electric signals. These signals were sent back to Earth as radio waves.
Scientists planned the mission using math and research.
Experts like Mstislav Keldysh helped guide the research for the flight. The spacecraft used a gravity assist to help it return home. This means the Moon's gravity pulled on the craft to change its path. This maneuver helped the probe fly back toward Earth. The return path was carefully calculated to pass over the Northern hemisphere. This allowed ground stations in the Soviet Union to find the signal.
Luna 3 traveled very close to the Moon on 6 October 1959.
It passed within 6,200 km of the Moon's south pole. On 7 October, the camera took 29 pictures over 40 minutes. These photos covered 70% of the far side. The pictures showed a landscape full of mountains. Scientists found only two dark, low-lying regions called maria. One was named Mare Moscoviense, or the Sea of Moscow. The other was Mare Desiderii, or the Sea of Desire.
These new images helped experts make the first map of the far side.
In 1960, the USSR Academy of Sciences published an atlas of the area. This atlas listed 500 different features of the Moon's landscape. They even named craters after famous people like Marie Curie and Thomas Edison. Today, we can compare these old, grainy photos to new pictures from modern probes. Luna 3 showed us a world that had been a mystery for a long time.
Luna 3 was a historic Soviet spacecraft launched in 1959. It was part of the Luna programme. This mission was the first to photograph the far side of the Moon. For all of human history, this side of the Moon remained a mystery. It is the hemisphere that always faces away from Earth. Luna 3 changed our understanding of the lunar landscape forever.
The spacecraft was a long, cylindrical canister with hemispheric ends. It was hermetically sealed and pressurized to maintain its internal environment. Solar cells were mounted on the outside of the cylinder. These cells provided electric power to the storage batteries inside. To manage heat, the probe had thermal control shutters. These shutters opened to expose a radiating surface if internal temperatures exceeded 30 °C. The probe also carried scientific tools like cosmic ray detectors. It used gas jets for its attitude control system.
The imaging system was called Yenisey-2. It used a dual-lens camera known as the AFA-E1. One lens had a 200 mm focal length to image the full Moon. The second lens had a 500 mm focal length to zoom in on specific regions. The camera used 35mm isochrome film. This film was specially treated to resist radiation and temperature changes. After the photos were taken, an onboard processor developed, fixed, and dried the film. A flying-spot scanner then converted the images into electric signals. These signals were transmitted to Earth using frequency-modulated analog video.
The mission required complex navigation and physics. Luna 3 was launched over the North Pole using a Luna 8K72 rocket. The spacecraft used a gravity assist maneuver to return to Earth. This maneuver used the Moon's gravity to change the spacecraft's orbit. It also changed the orbital plane of the probe. This calculation was based on research led by Mstislav Keldysh. The return path was designed to pass over the Northern hemisphere. This ensured Soviet ground stations could receive the signals.
On 6 October 1959, Luna 3 reached its closest approach to the Moon. It passed within 6,200 km of the lunar south pole. The photography sequence began on 7 October when a photocell detected sunlight. The cameras took 29 pictures over a period of 40 minutes. These images covered 70% of the far side of the Moon. The spacecraft was at distances between 63,500 km and 66,700 km during this time. Eventually, 17 photographs were successfully transmitted back to Earth.
The images revealed a landscape very different from the near side. The far side was mostly mountainous terrain. It lacked the large, dark areas seen on the side facing Earth. Scientists identified only two dark, low-lying regions called maria. One was named Mare Moscoviense, or the Sea of Moscow. The other was Mare Desiderii, or the Sea of Desire. Later, Mare Desiderii was found to contain a smaller mare called Mare Ingenii. Scientists believe the lack of dark lava on the far side is due to how lavas flowed during the Moon's formation.
The data from Luna 3 led to significant scientific achievements. In 1960, the USSR Academy of Sciences published an atlas of the far side. This atlas contained a catalog of 500 different landscape features. In 1961, the first Moon globes were created using these images. Scientists named several craters after famous figures like Marie Curie and Thomas Edison. Even today, researchers compare these early images to modern data.
This comparison shows how accurately the original Yenisey-2 system mapped the lunar surface. The mission remains a foundational moment in space exploration.
Where will your curiosity go next?
🖼️ Images & Media (5)
More to explore
✨ What else?
Related topics you might enjoy
🔬 Go deeper
More advanced topics to explore
🪜 Step back
Simpler topics to build understanding
What is Nepedia?
A free, ad-free encyclopedia for children. Every article is written at five reading levels, so the same page works for a five-year-old and a fifteen-year-old — use the level switcher above to see this one change. No account needed to read.