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Home»Science»International Observe the Moon Night 2025: 4 things to see on the lunar surface on Oct. 4
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International Observe the Moon Night 2025: 4 things to see on the lunar surface on Oct. 4

October 5, 2025No Comments
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International Observe the Moon Night 2025 is upon us! Here’s what to look for when the lunar disk rises above the eastern horizon on Oct. 4.

Each year NASA teams up with a host of international partners to hold events to engage the public in observing the moon and learn about humanity’s efforts to explore Earth’s natural satellite. Be sure to check out the Observe the Moon Night website to explore over 950 virtual and in-person events that are being held to mark the occasion!

To celebrate, we’ve put together a list of stunning targets to observe through a telescope, binoculars, or with the naked eye that showcase the diverse nature of the lunar surface.


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5 lunar targets to celebrate Observe the Moon Night 2025

1 – The terminator

The line separating night from day on the lunar surface is known as the terminator. On Oct. 4, this shadowy divide will fall over the extreme left side of the 95%-lit moon, just two days before it reaches its full moon phase on Oct. 6 and gives rise to a spectacular full “Harvest Supermoon”.

Look to the top of the terminator to see the shadow-drenched form of the 75 mile-wide (120 kilometer) Pythagoras Crater scarring the lunar surface, while to the south the western rim of the sprawling Schickard Crater is thrown into relief below the striking oval form of the impact crater Byrgius.

A near full lunar disk is shown against a black sky with a tiny crescent on its left side hidden in shadow. The line separating night from day is labelled as the terminator. The Pythagoras Crater is labelled on the terminator to the north, while the Byrigius and Schickard craters are labelled to the south. The lunar sea Oceanus Procellarum dominates the lunar equator close to the terminator.

The terminator rests on the left side of the lunar disk mere days ahead of the full moon phase. (Image credit: NASA’s Scientific Visualization Studio, annotated in Canva by Anthony Wood)

2 – Mare Nubium

Look south of the moon’s equator on Oct. 4 to find Mare Nubium (Latin for “the Sea of Clouds”) darkening a vast swathe of the lunar surface, with the prominent Lubiniezky, Bullialdus and Wolf craters pockmarking this basalt plain.

The lunar seas were formed billions of years ago when lakes of lava flooded networks of impact basins excavated by brutal asteroid strikes. The lava subsequently cooled and solidified to repave the lunar surface, leaving vast regions that appear relatively unscathed by the bombardment that ravaged the more ancient parts of the lunar surface.

Breaking space news, the latest updates on rocket launches, skywatching events and more!

The southern lunar disk is shown with the dark expanse of the lunar sea Mare Nubium labelled with the prominent Lubiniezky, Bullialdus and Wolf craters scarring its surface

Spot Mare Nubium darkening the southern lunar surface on Oct. 4. (Image credit: NASA’s Scientific Visualization Studio, annotated in Canva by Anthony Wood)

3 – Mountains surrounding the “Bay of Rainbows”

Montes Jura is a vast mountainous range of terrain bordering the northern edge of the Sinus Iridum (Latin for “Bay of Rainbows”) impact site. The upper peaks are perfectly positioned to catch the sun’s light around 11 days after the monthly new moon phase, making it appear as if a vast “Golden Handle” resides upon the lunar surface.

The northwest region of the lunar surface is shown with the curved profile of the Montes Jura mountain range labelled and highlighted with a white circle.

The Montes Jura mountain range surrounds the northwestern edge of the Sinus Iridum impact site. (Image credit: NASA’s Scientific Visualization Studio, annotated in Canva by Anthony Wood)

4 – Ejecta rays

The nights surrounding a full moon phase are the perfect time to spot ejecta rays brightening the lunar surface. These bright streaks emanating from craters are formed when asteroid strikes cast out reflective material from the moon’s interior and can extend for hundreds of kilometers. Tonight, look for them streaking away from large impact sites such as Kepler, Copernicus and the 53-mile-wide (85 km) Tycho Crater that dominates the south lunar surface.

All impact craters once boasted ejecta rays of their own, which become dulled with prolonged exposure to the space environment. The ones we see today are relatively young, with Tycho for example being just 108 million years old.

The moon is shown close to its full moon phase, with the bright young Copernicus Aristarchus, Kepler and Tycho craters labelled.

Bright streaks known as ejecta rays surrounding young craters are particularly visible around the full moon phase. (Image credit: NASA’s Scientific Visualization Studio, annotated in Canva by Anthony Wood)

Editor’s Note: If you capture an image of the lunar surface and want to share it with Space.com’s readers, then please send your photo(s), comments, and your name and location to spacephotos@space.com.

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