APOD: 2026 October 1 – Harvest Moon with Erupting Mount Etna

APOD: 2026 October 1 – Harvest Moon with Erupting Mount Etna

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

Rise of the Harvest Moon over the slopes of Mount Etna and the simultaneous play of colors in the anti-twilight.

Harvest Moon with Erupting Mount Etna

Explanation: Have you ever seen the full moon rise? This colorful image was photographed last weekend in Sicily, just outside the town of Nicosia, in Italy. It is a composite photograph that shows the Moon rising as the sky turns darker. Lower clouds are reflecting the colors of antitwilight, while ash and gas from Mount Etna are seen higher in the background. The pink band lower in the sky is called the Belt of Venus. During a full moon, the Moon and the Sun are in opposition in the sky: the moon rises as the sun sets. The lunar phase cycle lasts approximately 29.5 days (but the Moon takes approximately 27 days to orbit the Earth). In some cultures of the Northern Hemisphere, the September full moon is called the Harvest Moon. Does your culture have a special name for it? (A full moon by any other name would shine as bright.)

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Tomorrow’s picture: sharpless

Date October 1, 2026
Credit & Copyright Dario Giannobile
Authors & editors: Cecilia Chirenti, Robert Nemiroff, Jerry Bonnell, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

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An Agricultural “Island” in the Saskatchewan River Delta

An Agricultural “Island” in the Saskatchewan River Delta




Summer
autumn

A satellite image captured in summer shows farm fields in a patchwork of green and brown, surrounded by green wetlands dotted with dark patches of open water.
NASA Earth Observatory/Michala Garrison

The same area in autumn shows many of the farm fields are now brown, and the surrounding wetlands hold less water.
NASA Earth Observatory/Michala Garrison

A satellite image captured in summer shows farm fields in a patchwork of green and brown, surrounded by green wetlands dotted with dark patches of open water.
NASA Earth Observatory/Michala Garrison
The same area in autumn shows many of the farm fields are now brown, and the surrounding wetlands hold less water.
NASA Earth Observatory/Michala Garrison

Summer

autumn


Farmland across the Carrot River Valley, Manitoba’s northernmost agricultural area, moves from summer growth into harvest season in images captured on July 2, 2026 (left), and September 21, 2026 (right), with the OLI (Operational Land Imager) on the NASA-USGS Landsat 9 and Landsat 8 satellites, respectively. NASA Earth Observatory images by Michala Garrison.

Much of the Saskatchewan River Delta, a large inland delta that straddles the Canadian provinces of Saskatchewan and Manitoba, is too wet for extensive farming. But amid the delta’s winding channels, lakes, and marshes, an “island” of straight-edged fields breaks up the curvy contours. These fields, west of the town of The Pas, make up Manitoba’s northernmost agricultural area.

Known as the Carrot River Valley (Pasquia Area Settlement), the area lies within the Rural Municipality of Kelsey. Its actively farmed land spans more than 40,000 hectares (100,000 acres) between the Carrot and Pasquia rivers—tributaries of the Saskatchewan River—and is surrounded by wetlands, including the marshes of the Saskeram Wildlife Management Area to the north.

These images show the valley at two points during the 2026 growing season: on July 2 (left) and September 21 (right). They were acquired with the OLI (Operational Land Imager) on the NASA-USGS Landsat 9 and Landsat 8 satellites, respectively.

Landsat data feed into the Agriculture and Agri-Food Canada annual crop inventory. The 2026 inventory was not released as of late September, but the 2025 map shows that farmers in the Carrot River Valley grew mostly canola and spring wheat that year, along with small patches of Canary seed.

The July 2026 image shows green crops across many of the valley’s fields. Planting in the area, part of Manitoba Agriculture’s Northwest crop reporting region, began later than in parts of the region to the south because of wet conditions. Still, fertile soils and long summer days at this northern latitude can help crops grow quickly.

By the time of the September image, the pattern had flipped. The Pas recorded little rainfall in the preceding week (1.6 millimeters, or 0.06 inches), while wetter weather elsewhere in the Northwest region (up to 43.9 millimeters, or 1.7 inches) held up the harvest. By then, farmers across the region had harvested about 10 percent of the canola and 50 percent of the spring wheat.

Managing water has long been a challenge in the valley. In the 1950s, a major flood control and drainage project got underway, and farming in the area today still depends on diking and pumping for agricultural flood protection.

NASA Earth Observatory images by Michala Garrison, using Landsat data from the U.S. Geological Survey. Story by Kathryn Hansen.

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Station Prepares to Welcome Crew-13 while Continuing Space Research

Station Prepares to Welcome Crew-13 while Continuing Space Research

The seven-member Expedition 75 crew poses for a portrait inside the International Space Station. Clockwise from left are, NASA astronauts Jessica Meir and Jack Hathaway, Roscosmos cosmonauts Anna Kikina and Andrey Fedyaev, astronauts Anil Menon of NASA and Sophie Adenot of ESA (European Space Agency), and Roscosmos cosmonaut Pyotr Dubrov.
The seven-member Expedition 75 crew poses for a portrait inside the International Space Station. Clockwise from left are, NASA astronauts Jessica Meir and Jack Hathaway, Roscosmos cosmonauts Anna Kikina and Andrey Fedyaev, astronauts Anil Menon of NASA and Sophie Adenot of ESA (European Space Agency), and Roscosmos cosmonaut Pyotr Dubrov.
NASA

Expedition 75 is getting the International Space Station ready for the arrival of NASA’s SpaceX Crew-13 mission scheduled to launch and dock to the orbital outpost on Thursday, Oct. 1. In the meantime, space research and lab maintenance rounded out the schedule keeping the astronauts and cosmonauts busy on Wednesday.

Crew-13 commander Jessica Watkins and pilot Luke Delaney, both NASA astronauts, along with mission specialists Johsua Kutryk of CSA (Canadian Space Agency) and Sergey Teteryatnikov of Roscosmos will launch aboard a SpaceX Dragon spacecraft atop the Falcon 9 rocket at 11:10 a.m. EDT on Thursday. NASA+ begins its live launch coverage at 9:20 a.m. from Cape Canaveral Space Force Station’s Launch Pad 40 in Florida.

Dragon will dock to the Harmony module’s forward port on the orbital outpost about 7 p.m. the same day. The four Crew-13 members will open the hatch about an hour-and-a-half later, enter Harmony, and join the Expedition 75 crew for welcoming remarks and a safety orientation. Docking coverage begins at 5:20 p.m. on NASA+.

Three NASA astronauts living aboard the station worked together on Wednesday getting ready for the arrival of Crew-13. Station commander Jessica Meir reorganized cargo inside the Harmony’s pressurized mating adapter-2, where Dragon will dock, making room for Crew-13’s entry into the orbital outpost. Flight engineers Anil Menon and Jack Hathaway staged supplies in Harmony necessary to support the four crewmates immediately after their entry into the station and beginning their mission.

Flight engineer Sophie Adenot of ESA (European Space Agency) focused primarily on science throughout her shift on Wednesday. Adenot started her day in the Columbus laboratory module working out on the European Enhanced Exploration Exercise Device (E4D). She pedaled on the E4D’s exercise cycle continuing to test the device’s ability to keep crews fit inside spacecraft during long-term missions to the Moon, Mars, and beyond. Next, she practiced simulated lunar landing techniques on a computer helping researchers understand how microgravity affects a crew member’s cognition when manually piloting a spacecraft.

Roscosmos flight engineer Andrey Fedyaev continued testing the lower body negative pressure suit that reverses space-caused fluid shifts from the head toward the feet. The specialized suit may help crews adjust quicker to Earth’s gravity after a long-term mission in weightlessness.

Roscosmos flight engineers Anna Kikina and Pyotr Dubrov took turns wearing arm, wrist, and finger cuffs measuring their blood pressure to understand how microgravity affects a crew member’s microcirculatory system. Afterward, Kikina unloaded cargo delivered recently aboard the Progress 96 cargo spacecraft while Dubrov worked on life support and computer maintenance.

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark A. Garcia

Curiosity Blog, Sols 5016–5021: Fantastic Minerals and How To Detect Them

Curiosity Blog, Sols 5016–5021: Fantastic Minerals and How To Detect Them

3 min read

Curiosity Blog, Sols 5016–5021: Fantastic Minerals and How To Detect Them

A close-up view of a dusty, reddish-brown Martian rock surface taken by the Curiosity rover. The surface is highly textured, covered with a complex network of small, raised, intersecting ridges that resemble tiny blades or crystals buried under a fine layer of sand. Right in the center of the frame is a small, distinct, dark circular hole.
NASA’s Mars rover Curiosity generated this close-up image of a brushed spot on bedrock (informally named “Salar de Vacas”), showing a jumble of roughly disc-shaped features as well as a divot generated by the brushing from the rover’s Dust Removal Tool (DRT). The features are about 3-4 millimeters across (about 0.12-0.16 inches) and about 1 millimeter thick (about 0.04 inches). Curiosity created the image using its Mars Hand Lens Imager (MAHLI), a close-up camera located on the turret at the end of the rover’s robotic arm, and an onboard focusing process that merges multiple images of the same target at different focus positions, creating a composite that brings as many features into focus as possible. Curiosity performed the focus merge on Sept. 16, 2026 — Sol 5016, or Martian day 5,016 of the Mars Science Laboratory Mission — at 02:14:02 UTC.
NASA/JPL-Caltech/MSSS

Written by Lucy Lim, Planetary Scientist at NASA Goddard Space Flight Center

Earth planning date: Friday, Sept. 18, 2026

Curiosity surprised us at the beginning of the week with a change in rock texture — instead of the finely layered bedrock blocks we’ve been seeing in our recent sulfate unit workspaces, suddenly we were looking at blocks covered (and likely filled) with a jumble of small disc-shaped lumps. We’ve seen somewhat similar features before much earlier in the mission — for example, close to the Pahrump Hills back in the Murray mudstones, and they’re sometimes seen in Earth rocks as well, especially in settings in which minerals were precipitating from an evaporating fluid. The disc-like shapes could be created by the growth habits of a specific crystalline mineral that is known to grow into similar shapes, or they could be bits of a harder rock layer that broke up and collected here. We planned Mastcam and MAHLI imaging for more morphological detail on the jumbled disc blocks (“Yungay,” “Chiu Chiu”) as well as LIBS (“Puya Raimondii,” “Liolaemus Tacnae,” “Pisqu Warkatana”) and APXS (“Salar de Vacas”) to investigate their composition. 

Ongoing long-distance imaging projects were furthered by ChemCam long-distance remote imager (RMI) and Mastcam mosaics of the buttes on either side of Valle Grande. These “cutaway”-view images of the strata above the rover will help us map sedimentary structures in these upcoming units and understand how these rocks formed and eroded. Views of more recent erosional deposits will also help us to understand the formation of Valle Grande itself.

In order to identify minerals, Curiosity needs data from the CheMin X-ray diffraction instrument, which means a drill campaign. We’ve driven over a kilometer since our last drill site at Campo Marte, and this will be our first drill above the erosional supersurface. The Wednesday plan’s drive brought us up next to a promising drill workspace a little beyond where we saw the disc-shaped features discussed above (imaged as “Torres del Paine” by Mastcam) and Friday’s planning included site characterization with the instruments on Curiosity’s arm (“Alberta Wild Rose,” “Moonraker Mountain”), ChemCam LIBS (“Osoyoos”), and Mastcam (“Trincomali Channel,” “Yellow Lady’s Slipper”). The team also selected a specific drill target and planned a very short drive to bring it in range of the arm — first for contact science and then, if all goes well, for the preload test and drill.

I’ll be back on planning on Monday as Geology and Mineralogy Science Theme Lead for Drill Sol 1 (Triage Contact Science) and we’ll see how things go from there!

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Curiosity rover at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

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Last Updated
Sep 30, 2026

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Help Overlap Zoo Reveal Cosmic Dust

Help Overlap Zoo Reveal Cosmic Dust

Galaxies, vast collections of billions of stars, gas, and dust held together by gravity, are scattered across the immensity of space. But every so often, a coincidence occurs: Two galaxies line up from our point of view on Earth (or from a space telescope) and appear to overlap in the sky. These rare overlapping galaxies give astronomers a chance to study something normally difficult to see: the dust inside one of these distant cosmic objects. That’s the focus of NASA’s new Overlap Zoo project.

Picture the background galaxy acting like a cosmic flashlight, shining through the nearer galaxy. The backlit dust creates dark silhouettes, like shadows on a screen. By studying these silhouettes, astronomers can map how dust is distributed throughout galaxies and learn how it blocks, scatters, and dims starlight traveling through space. Measurements of how dust impacts light can even help astronomers refine estimates of the distances to faraway objects.

However, before we can study galaxy pairs and their dust, we first need to find them! Overlap Zoo is asking for your help with the search. 

“As new and better observations of galaxies continue to multiply, it is becoming incredibly difficult for astronomers to classify every candidate galaxy pair,” said Trevor Butrum, Overlap Zoo project lead and graduate student. “Your help is invaluable to creating the biggest and cleanest catalog of overlapping galaxy pairs for further analysis.”

As a volunteer in Overlap Zoo, you’ll view images that volunteers in the Galaxy Zoo project have identified as containing possible overlapping galaxies. The Overlap Zoo project will teach you how to verify the presence of galaxy pairs in these images, classify key features of each galaxy, and mark their outlines. You’ll learn as you go, classifying as many of these images as you like. Your contributions will help build the first large-scale catalog of galaxy pairs suitable for dust studies and enable a huge step forward in accuracy of astronomical estimates.

Head over to Overlap Zoo and start classifying galaxies today. No prior experience needed – just curiosity and a few minutes of your time. Your observations will help unlock the secrets hidden in these rare cosmic alignments!

Two overlapping galaxies against a dark field of distant stars and galaxies. A bright, smooth galaxy at left partially overlaps a face-on spiral galaxy at right, whose winding arms are dotted with blue and pink regions.
A prime example of an overlapping galaxy pair known as VV191a/b.
Image credit: NASA, ESA, CSA, JWST PEARLS Team, Rogier Windhorst (ASU), William Keel (University of Alabama), Stuart Wyithe (University of Melbourne); Image Processing: Alyssa Pagan (STScI)

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