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A Trio of Tropical Cyclones in the Pacific

In a full-disk satellite view of Earth, three tropical cyclones—named Lowell, Karina, and Marie—swirl above the blue waters of the Pacific Ocean and to the west of Central America.

When hurricane forecasters released their seasonal outlooks in spring 2026, the El Niño brewing in the Pacific contributed to predictions of below-normal activity in the Atlantic basin but above-normal activity in the northeastern and central Pacific basins. In early September, near the climatological peak of hurricane season, those spring outlooks were on target, with the eastern Pacific buzzing with activity and the Atlantic notably quiet.

As of September 3, the Northeast Pacific had produced 15 named storms and six hurricanes, well above the norm for that point in the season. The Atlantic basin, meanwhile, laboring under unfavorable wind shear conditions, had produced just five named storms and no hurricanes. El Niño typically enhances hurricane activity in the eastern and central Pacific basins because of the unusually warm water temperatures it brings to those parts of the ocean. It tends to suppress hurricane activity in the Atlantic basin by shifting large-scale circulation patterns in a way that makes it harder to sustain storms there.

At 1:14 p.m. Pacific Daylight Time (20:14 Universal Time) on September 1, NASA’s EPIC (Earth Polychromatic Imaging Camera) on the DSCOVR (Deep Space Climate Observatory) satellite captured an image of three tropical cyclones churning simultaneously in the Pacific, along with one in the Atlantic. A band of clouds and thunderstorms associated with the Intertropical Convergence Zone (ITCZ) is visible to the south of the storms. The spacecraft was nearly 1 million miles from Earth and just shy of 93 million miles from the Sun when the image was acquired.

The trio of storms in the Pacific were Lowell, Karina, and Marie. Of the three, Lowell became the strongest, with winds reaching category 5 strength for several hours on September 2. Around the same time, Karina, spinning a few thousand kilometers to the east, achieved category 4 strength, a rare case of category 4 and 5 hurricanes occurring simultaneously in the area. Marie, spinning southwest of Baja California, was still a tropical storm when the image was acquired but was strengthening as it moved northwest.

In the Atlantic, Tropical Storm Edouard was visible to EPIC over Louisiana and Texas, shortly after the short-lived storm made landfall. It brought torrential rains and strong winds that downed trees and power lines. Some areas received 15 to 24 inches (38 to 61 centimeters) of rain, according to National Weather Service meteorologists.

As of September 3, the Atlantic basin’s total accumulated cyclone energy (ACE) index was 4.4, about 9 percent of normal for that date, according to statistics compiled by Colorado State University meteorologists. Meanwhile, the Northeast Pacific basin’s ACE was 130, about 50 percent above normal. The ACE index incorporates both the intensity and longevity of storms, making it easier to compare individual storms and seasons.

Several NASA Earth-observing platforms provide data that can aid in emergency preparedness before landfall and damage assessment and response afterward. Use the “Events” tab on NASA’s Worldview browser to track current hurricanes and explore related NASA data products.

NASA Earth Observatory image by Lauren Dauphin, using data from DSCOVR EPIC. Story by Adam Voiland.

References & Resources

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Stay up-to-date with the latest content from NASA as we explore the universe and discover more about our home planet.

Lala Batters Hawaii

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Tropical Storm Arthur

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The first named storm of the 2026 Atlantic hurricane season brought intense rainfall and the threat of flash flooding to…

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El Niño Is Underway

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Satellite observations of sea surface height indicated that the 2026 event continued to strengthen in early June.

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Source: science.nasa.gov

APOD: 2026 September 4 – Na Uhane Mahoe Huki Pu i ke Ola

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.

Two spiral galaxies colliding.

Nā ʻUhane Māhoe Huki Pū i ke Ola

Explanation: Nā ʻUhane Māhoe Huki Pū i ke Ola, is the Hawaiian name given to this image of a pair of spiral galaxies locked in a mutual gravitational embrace. Some 200 million light-years distant toward the high flying constellation Pegasus their spectacular, galactic scale merger is captured in sharp detail in the image from the 8.1 meter Gemini North telescope on Maunakea, Hawai‘i. The galaxy pair, known as NGC 7253 and Arp 278, was chosen as a target, researched, and given a Hawaiian name by high school students in the joint Gemini Observatory and University of Hawaiʻi Project Hōkūlani internship program. The name translates to “The Twin Spirits Pulling Together Creating Life”. That’s both culturally and astronomically appropriate for galaxy collisions that trigger a cosmic maelstrom of star formation from galactic reservoirs of elemental building blocks of life. These merging galaxies are found within a region of Pegasus identified as the Hawaiian navigational constellation Ka Lupe o Kawelo.

APOD’s main NASA site is moving: From apod.nasa.gov to science.nasa.gov/apod
Tomorrow’s picture: chasing shadows

Date September 4, 2026
Credit: Image Credit: International Gemini Observatory / NOIRLab/NSF/AURA
Image Processing: J. Miller & M. Rodriguez (International Gemini Observatory/NSF NOIRLab),
T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)
Authors & editors: Jerry Bonnell, Cecilia Chirenti, Robert Nemiroff, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

Source: science.nasa.gov

Lunar Occultation of Venus

Venus is seen as it disappears behind the Moon at the start of the occultation on June 17, 2026, from the Mary W. Jackson NASA Headquarters building in Washington
NASA/Joel Kowsky

On Wednesday, June 17, skywatchers across the United States—and parts of Canada—enjoyed a rare event: a daytime lunar occultation of Venus. A lunar occultation occurs when the Moon moves directly in front of another celestial object from our viewpoint on Earth, briefly hiding it from sight.

This time, the Moon slipped in front of Venus for the first of three occultations happening this year, creating a striking daylight moment for those who caught it. If you missed it, there will be two more opportunities to see Venus disappear behind the Moon in 2026: Sept. 14, visible from parts of Asia, Africa, Europe, and western Russia; and Nov. 7, visible from southern South America.

Source: www.nasa.gov

NASA Hosts Virtual Artemis Webinar for Blind, Low-Vision Community

Two technicians at NASA’s Michoud Assembly Facility in New Orleans stand around one of the four RS-25 engines for the agency’s SLS (Space Launch System) rocket on Sept. 8, 2023. The RS-25 engine looks like a bell-shaped nozzle attached to a network of pipes. The engine is being lifted by the horizontal engine installer so it appears to be lying on its side. The RS-25 engine is about the size of a large pickup truck. The technicians are wearing hard hats and safety harnesses.
Two technicians at NASA’s Michoud Assembly Facility in New Orleans stand around one of the four RS-25 engines for the agency’s SLS (Space Launch System) rocket on Sept. 8, 2023. The RS-25 engine looks like a bell-shaped nozzle attached to a network of pipes. The engine is being lifted by the horizontal engine installer so it appears to be lying on its side. The RS-25 engine is about the size of a large pickup truck. The technicians are wearing hard hats and safety harnesses.
Credit: NASA/Michael Democker

NASA will host a virtual webinar at 2 p.m. EDT on Friday, Oct. 2, titled “The RS-25 Engine and the Future of Artemis Missions: An Accessible Webinar for the Blind and Low-Vision Community.” This webinar is open to the public, however it is tailored specifically for a blind and low-vision audience.

The webinar will last about two hours and include an audio-described video of an RS-25 engine test, a Q&A session with an Artemis engineer, and a panel about accessibility in space and science. The event will be hosted on the Zoom platform. 

Participants in the session include:

  • Dr. Kimberly Arcand, visualization scientist, NASA’s Chandra X-ray Observatory
  • Josh Greiner, test director, NASA’s Stennis Space Center in Bay St. Louis, Mississippi
  • Dr. Craig Moore, materials engineer, NASA’s Marshall Space Flight Center in Huntsville, Alabama
  • Dr. Robert Shelton, lead simulation engineer, NASA’s Johnson Space Center in Houston
  • Christine Malec, freelance writer and consultant

Those interested in attending the webinar must RSVP using this form by Friday, Sept. 25. Any questions can be directed to [email protected]. The details of the webinar will be emailed to registrants in the days leading up to the event.

NASA’s Artemis program will send astronauts on increasingly difficult missions to explore the Moon and establish a Moon Base on the lunar surface. For additional information on the Artemis missions, visit:

https://www.nasa.gov/artemis

Details

Last Updated

Sep 04, 2026

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Source: www.nasa.gov

NASA Ames Fire Department Aircraft Firefighting Training

The fire department at NASA’s Ames Research Center in California’s Silicon Valley will perform training on the Moffett Federal Airfield beginning Tuesday, Sept. 8 through Friday, Sept. 11. The training will involve the use of a propane-fueled aircraft fire simulator and be conducted from 8 a.m. to 8 p.m. PDT.

Because the aircraft simulator is fueled by propane, very little smoke should be produced during the controlled training fires. However, flames may be visible to drivers on U.S. Highway 101. The training is intended to prepare Ames’ first responders to respond to a variety of realistic aircraft firefighting scenarios.

For more information about NASA’s Ames Research Center, visit:

http://www.nasa.gov/ames

-end-

Jeanne Neal
Ames Research Center, Silicon Valley
650-604-4789
[email protected]

To receive local NASA Ames news, email [email protected] with “subscribe” in the subject line. To unsubscribe, email the same address with “unsubscribe” in the subject line.

Source: www.nasa.gov

APOD: 2026 September 5 – Chasing the Moon’s Shadow

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.

A solar eclipse as viewed by a pilot from an aircraft cockpit.

Chasing the Moon’s Shadow

Explanation: Chasing the shadow of a New Moon, NASA’s WB-57F high altitude research aircraft took to the skies off the coast of Iceland on August 12 to observe a total solar eclipse. At 50,000 feet the aircraft was piloted along the precisely determined path of totality to maximize its time in the Moon’s shadow. A suite of high-resolution cameras on board was able to record eclipse data from above the clouds, dust, and atmospheric water vapor that interfere with observations made closer to the ground. This view from the cockpit, taken from an inflight video, captures the solar corona emerging at the beginning of totality. The sky appears dark in the shadow of the Moon. Venus is shining left of center in the video frame, while Jupiter and Mercury are just visible to the right of the eclipsed Sun. But the sky is bright along the distant horizon below, beyond the reach of the Moon’s shadow.

APOD’s main NASA site is moving: From apod.nasa.gov to science.nasa.gov/apod
Tomorrow’s picture: enhancing Pluto

Date September 5, 2026
Credit: NASA
Authors & editors: Jerry Bonnell, Cecilia Chirenti, Robert Nemiroff, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

Source: science.nasa.gov

A Bright Spot at Mount Michael

A small ice- and snow-covered island with an active volcanic crater at its center is surrounded by drifting pieces of sea ice. A thermal signal and small plume appear in the crater, and ash darkens the snow on the volcano’s northern slopes.
Mount Michael on Saunders Island, seen in this image acquired with the OLI (Operational Land Imager) on Landsat 8 on August 24, 2026, hosts a frequently active lava lake in its summit crater.
NASA Earth Observatory/Michala Garrison

Winter near the Antarctic Circle brings months of frozen darkness, when sea ice chokes ocean waters and many of its denizens hunker down to ride out the harsh conditions. But as winter began to release its icy grip, an uncommonly clear satellite image revealed that part of this remote realm was still very much awake, at least volcanically speaking.

Mount Michael, the stratovolcano at the center of Saunders Island, rises above the ice-filled South Atlantic Ocean in this image, acquired with the OLI (Operational Land Imager) on the NASA-USGS Landsat 8 satellite on August 24, 2026. The natural-color image is overlaid with an infrared signal (OLI bands 7-6-5), shown in red, revealing heat from the persistent lava lake in its summit crater. A puff of a volcanic plume hovering over the peak, along with darkened snow on its northern slopes, also suggests ongoing activity.

Saunders Island is one of the South Sandwich Islands, a string of small volcanic peaks about 350 kilometers (220 miles) long that formed from the South American plate subducting beneath the tiny South Sandwich plate. Regular eruptions, including at Mount Michael, have occurred on these islands in recent centuries.

Because of the volcanoes’ remoteness, scientists rely on satellite data to understand their activity. An analysis of thermal anomalies in Landsat, Sentinel, and ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer) observations spanning 30 years led researchers to conclude that Mount Michael hosts a persistent lava lake in its summit crater. Only a handful of other volcanoes on Earth, including Kīlauea, Nyamulagira, and Erta Ale, are known to have similar, frequently active features.

Thermal observations from the MODIS (Moderate Resolution Imaging Spectroradiometer) and VIIRS (Visible Infrared Imaging Radiometer Suite) instruments have also enabled long-term monitoring of Mount Michael. Data provided through MIROVA, a near-real-time volcanic hot spot detection system, indicate that low-intensity activity has been ongoing at the volcano for the past several years. Other observations from NASA’s Aura satellite show that emissions of sulfur dioxide and other gases are common at Mount Michael.

A series of V-shaped wave clouds appears over an ocean filled with pieces of sea ice.
Wave clouds form downwind of Saunders Island in this image acquired with the OLI (Operational Land Imager) on Landsat 9 on September 1, 2026.
NASA Earth Observatory/Michala Garrison

The cloud-free window over Mount Michael would close in short order. One week later, when Landsat 9 passed over the island, a more active atmosphere had returned. But the weather patterns interacted with the island to put on a spectacle of their own. The 843-meter-high (2,766-foot-high) peak jutting from the ocean disturbed passing winds to produce a series of wave clouds resembling the wake of a ship, a familiar phenomenon in this region. False-color imagery captured by NASA’s Aqua satellite indicates that a volcanic track caused by degassing sulfur dioxide was likely present as well.

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

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Source: science.nasa.gov

APOD: 2026 September 7 – The Pelican Nebula in Gas, Dust, and Stars

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.

A busy starfield is dominated by red and blue glowing gas and dark filamentary dust. The nebula appears to some to have the shape of a pelican.

The Pelican Nebula in Gas, Dust, and Stars

Explanation: The Pelican Nebula is slowly being transformed. IC 5070 (an official designation) is divided from the larger North America Nebula by a molecular cloud filled with dark dust. The deep featured picture from UtahUSA incorporates 25 hours of exposure and brings out great details of this filamentary dust. The Pelican Nebula receives much study because it is a particularly active mix of star formation and evolving gas clouds. The light from young energetic stars is slowly transforming the cold gas to hot gas, with the advancing boundary between the two, known as an ionization front, visible in bright orange on the upper right. Particularly dense tentacles of cold gas remain. Millions of years from now, the Pelican Nebula, bounded by dark nebula LDN 935, might no longer be known as the Pelican, as the balance and placement of stars and gas will surely leave something that appears completely different.

APOD’s main site is moving: From apod.nasa.gov to science.nasa.gov/apod
Tomorrow’s picture: geometric Saturn

Date: September 7, 2026
Credit & Copyright: Mark Killion
Authors & editors: Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

Source: science.nasa.gov

Casino en ligne en France : fonctionnement, risques et précautions

Les casinos en ligne reproduisent sur Internet des jeux traditionnellement proposés dans les établissements physiques. Ils peuvent offrir des machines à sous, des jeux de cartes, de la roulette ou des parties animées en direct. Leur accessibilité ne signifie cependant pas qu’ils sont légalement autorisés dans tous les pays.

Quels jeux sont autorisés en France ?

La réglementation française distingue les casinos physiques autorisés des jeux accessibles sur Internet. En ligne, les opérateurs agréés peuvent proposer des paris sportifs, des paris hippiques et du poker.

En revanche, les machines à sous et les jeux de table de casino ne sont pas autorisés en ligne. Un site accessible depuis la France peut donc rester illégal, même lorsqu’il affiche une licence internationale.

Les risques associés aux sites non autorisés

L’utilisation d’un casino en ligne non autorisé peut exposer le joueur à plusieurs problèmes. Il peut s’agir d’un refus de paiement, d’une fermeture soudaine du compte, d’un vol de données ou d’une absence de recours efficace en cas de litige.

Les autorités françaises peuvent également demander le blocage de plateformes proposant illégalement des jeux d’argent sur le territoire.

Reconnaître les principaux signaux d’alerte

Un site doit être considéré avec prudence lorsqu’il :

  • promet des gains garantis ;
  • exerce une forte pression pour effectuer un dépôt ;
  • dissimule ses conditions de retrait ;
  • réclame des frais imprévus pour libérer des gains ;
  • ne fournit aucune information vérifiable sur son exploitant ;
  • utilise abusivement le logo d’une autorité française.

La présence d’une licence étrangère ne remplace pas l’agrément exigé en France.

Protéger son budget

Aucune méthode ne garantit un bénéfice régulier aux jeux de hasard. Le résultat dépend principalement du hasard et l’opérateur conserve généralement un avantage mathématique.

Pour réduire les risques, il faut déterminer une limite de dépenses, ne jamais emprunter pour jouer et faire des pauses régulières. Les mineurs ne doivent jamais accéder aux jeux d’argent.

Lorsqu’une personne ressent une perte de contrôle, elle peut utiliser les dispositifs d’auto-exclusion ou demander une interdiction volontaire de jeux. Demander de l’aide rapidement permet de mieux protéger sa santé et sa situation financière.

Top casino en ligne : quels critères permettent d’évaluer une plateforme ?

Les classements de casinos en ligne sont nombreux, mais ils ne reposent pas toujours sur des méthodes objectives. Certains comparateurs privilégient les plateformes qui leur versent les commissions les plus élevées. Un lecteur doit donc comprendre les critères utilisés avant d’accorder sa confiance à une recommandation.

La situation réglementaire en France

Les jeux de casino en ligne comme les machines à sous, la roulette ou le baccarat ne sont pas autorisés en France. Les sites disposant uniquement d’une licence étrangère ne sont pas agréés par les autorités françaises.

Pour les activités permises, comme le poker et certains paris, la première vérification consiste à consulter la liste officielle des opérateurs agréés par l’Autorité nationale des jeux.

La sécurité et la protection des données

La sécurité constitue un critère essentiel pour identifier ce qu’un comparateur présente comme le meilleur casino en ligne. Le site doit protéger les connexions, expliquer le traitement des données personnelles et proposer des méthodes fiables de vérification d’identité.

Les joueurs doivent utiliser un mot de passe unique et éviter de communiquer leurs documents par courrier électronique ou messagerie instantanée.

La clarté des paiements

Une plateforme transparente indique les moyens de paiement disponibles, les éventuels frais, les montants minimaux et les délais de traitement. Les conditions de retrait doivent être consultables avant tout dépôt.

Les retards répétés, les demandes de paiement supplémentaires ou les modifications inexpliquées des règles sont des signaux d’alerte.

La qualité du service client

Un service client compétent doit apporter des réponses précises concernant les comptes, les paiements et les conditions promotionnelles. La disponibilité d’une assistance en français peut faciliter les échanges, mais elle ne prouve pas que la plateforme est autorisée en France.

Les outils de jeu responsable

Les meilleurs dispositifs permettent de définir des limites de dépôt, de prendre une pause ou de fermer temporairement un compte. Ces outils complètent une règle fondamentale : ne jamais jouer avec de l’argent nécessaire au logement, à l’alimentation ou au remboursement de dettes.