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What’s Up: October 2025 Skywatching Tips from NASA

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Skywatching

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Tips & GuidesSkywatching FAQNight Sky NetworkA supermoon, and meteor showers from the Draconids and OrionidsA supermoon takes over the sky, the Draconid meteor shower peeks through, and the Orionid meteor shower shines bright.
Skywatching HighlightsOct. 6: The October supermoonOct. 6-10: The Draconid meteor showerOct. 21: The Orionid meteor shower peaks (full duration Sept. 26 – Nov. 22)TranscriptWhat’s Up for October? A Supermoon takes over, the Draconid meteor shower peeks through, and the Orionid meteors sparkle across the night sky.
The evening of October 6, look up and be amazed as the full moon is bigger and brighter because – it’s a supermoon!
Illustrated infographic showing the difference (as seen from Earth) between perigee, when a supermoon appears, and apogee, when a micromoon appears.
NASA/JPL-Caltech
This evening, the moon could appear to be about 30% brighter and up to 14% larger than a typical full moon. But why?
Supermoons happen when a new moon or a full moon coincides with “perigee,” which is when the moon is at its closest to Earth all month.
So this is an exceptionally close full moon! Which explains its spectacular appearance.
And what timing – while the supermoon appears on October 6th, just a couple of days before on October 4th is “International Observe the Moon Night”!
It’s an annual, worldwide event when Moon enthusiasts come together to enjoy our natural satellite.You can attend or host a moon-viewing party, or simply observe the Moon from wherever you are.
So look up, and celebrate the moon along with people all around the world!
The supermoon will light up the sky on October 6th, but if you luck into some dark sky between October 6th and 10th, you might witness the first of two October meteor showers – the Draconids!
The Draconid meteor shower comes from debris trailing the comet 21P Giacobini-Zinner burning up in Earth’s atmosphere
These meteors originate from nearby the head of the constellation Draco the dragon in the northern sky and the shower can produce up to 10 meteors per hour!
The Draconids peak around October 8th, but if you don’t see any, you can always blame the bright supermoon and wait a few weeks until the next meteor shower – the Orionids!
Sky chart showing the Draconid meteor shower, including the radiant point of the shower and the Draco constellation where the meteors in the shower are often seen and stem from.
NASA/JPL-Caltech
The Orionid meteor shower, peaking October 21, is set to put on a spectacular show, shooting about 20 meteors per hour across the night sky.
This meteor shower happens when Earth travels through the debris trailing behind Halley’s Comet and it burns up in our atmosphere.
The full duration of the meteor shower stretches from September 26 to November 22, but your best bet to see meteors is on October 21 befo..

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NASA, International Partners Deepen Commitment to Artemis Accords

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Representatives of the Artemis Accords signatories, including acting NASA Administrator Sean Duffy and NASA Associate Administrator Amit Kshatriya, met Sept. 29, 2025, for a principals meeting during the 76th International Astronautical Congress in Sydney.
Credit: NASA/Max van OtterdykNASA, along with leaders from global space agencies and government representatives worldwide, convened on Monday to further the implementation of the Artemis Accords — practical principles designed to guide the responsible exploration of the Moon, Mars, and beyond.
The meeting was held during the 76th International Astronautical Congress (IAC) taking place in Sydney. In opening remarks, acting NASA Administrator Sean Duffy highlighted the five-year anniversary of the Artemis Accords next month.
“When President Trump launched the Artemis Accords in his first term, he made sure American values would lead the way – bringing together a coalition of nations to set the rules of the road in space and ensure exploration remains peaceful. After five years, the coalition is stronger than ever. This is critical as we seek to beat China to the Moon, not just to leave footprints, but this time to stay,” said Duffy.
The United States, led by NASA and the U.S. Department of State, signed the accords on Oct. 13, 2020, with seven other founding nations. The accords were created in response to the growing global interest in lunar activities by governments and private companies. They now comprise 56 country signatories — nearly 30% of the world’s countries.
The event was co-chaired by NASA, the Australian Space Agency, and the UAE Space Agency. Dozens of nations were represented, creating the foundation for future space exploration for the Golden Age of exploration and innovation.
“Australia is a proud founding signatory of the Artemis Accords and is focused on supporting new signatories in the Indo-Pacific region,” said Head of Australian Space Agency Enrico Palermo. “The purpose of the accords is as important — if not more important — as it was when first established. This annual gathering of principals at IAC 2025 is a key opportunity to reaffirm our collective commitment to exploring the Moon, Mars and beyond in a peaceful, safe, and sustainable way.”
During the meeting, leaders discussed recommendations for non-interference in each other’s space activities including transparency on expected launch dates, general nature of activities, and landing locations. They also discussed orbital debris mitigation and disposal management, interoperability of systems for safer and more efficient operations, and the release of scientific data.
In May 2025, the United Arab Emirates hosted an Artemis Accords workshop focused on topics, such as non-interference and space object registration and reporting beyond Earth orbit.
“Through our active participation in the Artemis Accords and by organizing specialised work..

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NASA, Blue Origin Invite Media to Attend Mars Mission Launch

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A stylized illustration shows the twin ESCAPADE spacecraft entering Mars’ orbit.Credits: James Rattray/Rocket Lab USANASA and Blue Origin are reopening media accreditation for the launch of the agency’s ESCAPADE (Escape and Plasma Acceleration and Dynamics Explorers) mission. The twin ESCAPADE spacecraft will study the solar wind’s interaction with Mars, providing insight into the planet’s real-time response to space weather and how solar activity drives atmospheric escape. This will be the second launch of Blue Origin’s New Glenn rocket.
Media interested in covering ESCAPADE launch activities must apply for media credentials. Media who previously applied for media credentials for the ESCAPADE launch do not need to reapply.
U.S. media and U.S. citizens representing international media must apply by 11:59 p.m. EDT on Monday, Oct. 13. Media accreditation requests should be submitted online to: https://media.ksc.nasa.gov.
A copy of NASA’s media accreditation policy is available online. For questions about accreditation, please email: ksc-media-accreditat@mail.nasa.gov. For other mission questions, please contact NASA Kennedy’s newsroom: 321-867-2468.
Blue Origin is targeting later this fall for the launch of New Glenn’s second mission (NG-2) from Space Launch Complex 36 at Cape Canaveral Space Force Station in Florida. Accredited media will have the opportunity to participate in prelaunch media activities and cover the launch. Once a specific launch date is targeted, NASA and Blue Origin will communicate additional details regarding the media event schedule.
NASA will post updates on launch preparations for the twin Martian orbiters on the ESCAPADE blog.
The ESCAPADE mission is part of the NASA Small Innovative Missions for Planetary Exploration program and is funded by the agency’s Heliophysics Division. The mission is led by the University of California, Berkeley Space Sciences Laboratory, and Rocket Lab designed the spacecraft. The agency’s Launch Services Program, based at NASA’s Kennedy Space Center in Florida, secured launch services under the VADR (Venture-class Acquisition of Dedicated and Rideshare) contract.
To learn more about ESCAPADE, visit:
https://science.nasa.gov/mission/escapade
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Abbey Interrante
Headquarters, Washington
301-201-0124
abbey.a.interrante@nasa.gov
Leejay Lockhart
Kennedy Space Center, Florida
321-747-8310
leejay.lockhart@nasa.gov

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October’s Night Sky Notes: Let’s Go, LIGO!

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October’s Night Sky Notes: Let’s Go, LIGO!

An artist’s impression of gravitational waves generated by binary neutron stars.

Credits:
R. Hurt/Caltech-JPL

by Kat Troche of the Astronomical Society of the Pacific
September 2025 marks ten years since the first direct detection of gravitational waves as predicted by Albert Einstein’s 1916 theory of General Relativity. These invisible ripples in space were first directly detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO). Traveling at the speed of light (~186,000 miles per second), these waves stretch and squeeze the fabric of space itself, changing the distance between objects as they pass.
Waves In SpaceGravitational waves are created when massive objects accelerate in space, especially in violent events. LIGO detected the first gravitational waves when two black holes, orbiting one another, finally merged, creating ripples in space-time. But these waves are not exclusive to black holes. If a star were to go supernova, it could produce the same effect. Neutron stars can also create these waves for various reasons. While these waves are invisible to the human eye, this animation from NASA’s Science Visualization Studio shows the merger of two black holes and the waves they create in the process.
Two black holes orbit each other, generating space-time ripples called gravitational waves in this animation. As the black holes get closer, the waves increase in until they merge completely.
NASA’s Goddard Space Flight Center Conceptual Image Lab
How It WorksA gravitational wave observatory, like LIGO, is built with two tunnels, each approximately 2.5 miles long, arranged in an “L” shape. At the end of each tunnel, a highly polished 40 kg mirror (about 16 inches across) is mounted; this will reflect the laser beam that is sent from the observatory. A laser beam is sent from the observatory room and split into two, with equal parts traveling down each tunnel, bouncing off the mirrors at the end. When the beams return, they are recombined. If the arm lengths are perfectly equal, the light waves cancel out in just the right way, producing darkness at the detector. But if a gravitational wave passes, it slightly stretches one arm while squeezing the other, so the returning beams no longer cancel perfectly, creating a flicker of light that reveals the wave’s presence.
When a gravitational wave passes by Earth, it squeezes and stretches space. LIGO can detect this squeezing and stretching. Each LIGO observatory has two “arms” that are each more than 2 miles (4 kilometers) long. A passing gravitational wave causes the length of the arms to change slightly. The observatory uses lasers, mirrors, and extremely sensitive instruments to detect these tiny changes.
NASA
The actual detection happens at the point of recombination, when even a minuscule stretching of one arm and squeezing of the other changes how long..

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