Sunday, December 01, 2024

Jupiter makes closest approach to Earth: December 2-8, 2024 | BBC Star Diary

Jupiter makes closest approach to Earth: December 2-8, 2024 | BBC Star Diary

Jupiter and Venus are due to shine brightly in the sky this week. Find out how to see them along with many more stargazing highlights in this week’s Star Diary podcast, from the makers of BBC Sky at Night Magazine. 

What’s next for Comet C/2023 A3 (Tsuchinshan-ATLAS)? https://www.skyatnightmagazine.com/advice/comet-c-2023-a3-tsuchinshan-atlas


Video Credit: BBC Sky at Night Magazine
Caption Credit: NASA Goddard/BBC
Duration: 17 minutes
Release Date: Dec. 1, 2024

#NASA #Space #Astronomy #Science #Earth #Meteors #Aurora #Planets #Venus #Jupiter #SolarSystem #Stars #StarClusters #Constellations #Nebulae #MilkyWayGalaxy #Galaxies #Universe #Skywatching #BBC #UK #Britain #Europe #UnitedStates #Canada #NorthernHemisphere #STEM #Education #Podcast #HD #Video

Shenzhou-19 Crew Conduct Scientific Experiments | China Space Station

Shenzhou-19 Crew Conduct Scientific Experiments | China Space Station

China's Shenzhou-19 crew aboard the orbiting Tiangong Space Station has carried out a series of space experiments and performed equipment maintenance in the first month of their space mission. This video was released on Wednesday, Novemmber 27, 2024, a day marking the 25th anniversary of successful launch of China's first uncrewed spacecraft, Shenzhou-1, on November 20, 1999 from northwest China's Jiuquan Satellite Launch Center.

Up to date, China has launched 19 Shenzhou spacecraft, 14 of these have sent 24 astronauts into space, with the number of total trips reaching 38.

The crew members, Cai Xuzhe, Song Lingdong and Wang Haoze, were sent into the space station on October 30, 2024, for a six-month mission.

"On the same day 25 years ago, China's first unmanned spacecraft was successfully launched from the Jiuquan Satellite Launch Center. The first show of the Long March 2F carrier rocket or CZ 2F shocked the world and the first flight of Shenzhou-1 spacecraft has made all the Chinese proud. China's manned space program has taken the first step from blueprinting and dreaming to striving to realize the dream, laying a solid foundation for realizing the Chinese nation's millennium skyward dream," said Cai.

"Over the past 25 years, generations of astronauts have been confident, self-reliant and hardworking. With a coordinated national response and all people being of one mind, we have set new heights in exploring space again and again, including completing the strategic mission of three-step manned space program, building the Chinese people's own space station, highlighting the Chinese Dream through realizing the Space Dream and writing a brilliant chapter in exploring the vast space," said Song.

Shenzhou-19 Crew:
Commander Cai Xuzhe (蔡旭哲)
Mission Specialist Wang Haoze (王浩泽)
Mission Specialist Song Lingdong (宋令东)

Video Credit: CCTV
Duration: 1 minute, 35 seconds
Release Date: Nov. 30, 2024

#NASA #Space #Science #Earth #China #中国 #MicrogravityExperiments #Shenzhou19 #神舟十九号 #Taikonauts #Astronauts #CSS #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #CMSA #国家航天局 #LongDurationMissions #HumanSpaceflight #STEM #Education #HD #Video

Sonification of The Dreaded Clown-faced 'Emoji' Nebula: NGC 2392 | Hubble

Sonification of The Dreaded Clown-faced 'Emoji' Nebula: NGC 2392 | Hubble


This post is dedicated to all users of the notorious "clown-faced emoji" out there (and you know who you are). ;) In this sonification, the image is scanned clockwise like a radar. The radius is mapped to pitch, so light farther from the center is higher pitched. The outline of the nebula’s shell can be heard in the rising and falling of pitch, punctuated by its spokes. Brightness controls the volume. The Clown-faced Nebula (NGC 2392) or Caldwell 39, is a bipolar double-shell planetary nebula (PN). It was discovered by astronomer William Herschel in 1787. It is surrounded by gas that composed the outer layers of a Sun-like star. The visible inner filaments are ejected by a strong wind of particles from the central star. The outer disk contains unusual, light-year-long filaments.

NGC 2392 lies about 6,500 light-years away, and is visible with a small telescope in the constellation of Gemini.

At the center of NGC 2392, there is an O-type star with a spectral type of O(H)6f.

An emoji (絵文字 in Japanese) is a pictogram, logogram, ideogram, or smiley embedded in text and used in electronic messages and web pages. The primary function of modern emoji is to fill in emotional cues otherwise missing from typed conversation as well as to replace words as part of a logographic system. The first emoji sets were created by Japanese portable electronic device companies in the late 1980s and the 1990s. Emoji became increasingly popular worldwide in the 2010s after Unicode began encoding emoji into the Unicode Standard. They are now considered to be a large part of popular culture in the West and around the world.


Credit: NASA, European Space Agency (ESA), Andrew Fruchter (STScI), and the ERO team (STScI + ST-ECF)
Sonification credits: SYSTEM Sounds (M. Russo, A. Santaguida)
Duration: 36 seconds
Release Date: Nov. 5, 2021

#NASA #ESA #Astronomy #Space #Science #Hubble #Nebulae #Nebula #NGC2392 #ClownFacedNebula #Sonification #PlanetaryNebula #Star #Gemini #Constellation #MilkyWayGalaxy #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education #Emoji #Humor #History #HD #Video

China's First Commercial Rocket Launch Site Starts Operations in Hainan

China's First Commercial Rocket Launch Site Starts Operations in Hainan

The Hainan International Commercial Aerospace Launch Site is the first in China dedicated to commercial space missions. It began formal operations on November 30, 2024, with the successful maiden flight of the Long March 12 carrier rocket that delivered two satellites into designated orbits. CGTN reporter Zheng Yibing visited the site and spoke with the president of the facility. The mission also marked the inauguration of the Hainan Commercial Space Launch Site, China's first dedicated commercial space launch facility. Construction began in July 2022 and was completed in 878 days.

The successful launch from the spaceport has filled the gap in China's lack of a commercial space launch site. It marks the completion of the full industrial chain of the commercial aerospace sector. This includes satellite and rocket manufacturing, a commercial launch site, and satellite data application services. 

Hainan is an island province and the southernmost province of China. It consists of Hainan Island and many smaller islands in the South China Sea


Video Credit: CGTN
Duration: 3 minutes
Release Date: Dec. 1, 2024

#NASA #Space #Science #Earth #China #中国 #CNSA #中国国家航天局 #LongMarch12 #长征十二号运载火箭 #Rocket #CarrierRocket #MediumLift #CASC #SpaceTechnology #Engineering #CommercialSpace #CommercialSpaceflight #WSLS #HICAL #Spaceport #Wenchang #Hainan #STEM #Education #HD #Video

Cosmic Fireflies: Starlink Satellites over Earth | International Space Station

Cosmic Fireflies: Starlink Satellites over Earth | International Space Station

NASA Astronaut & Expedition 72 Flight Engineeer Don Pettit: "Cosmic fireflies. Actually, these are Starlink satellites momentarily flashing sunlight towards the International Space Station."

Starlink is a satellite Internet constellation of thousands of satellites that orbit the planet close to Earth, at about 550km. It is operated by Starlink Services, LLC, an international telecommunications provider that is a subsidiary of the American aerospace firm SpaceX. It provides network coverage to over 100 countries and territories. Starlink also plans to support global mobile broadband services.

Learn about Starlink technology here:


Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.

Learn more about the important research being operated on Station:
https://www.nasa.gov/iss-science 
For more information about STEM on Station:
https://www.nasa.gov/stemonstation
Science, Technology, Engineering, Math (STEM)


Video Credit: NASA's Johnson Space Center (JSC)/D. Pettit
Duration: 12 seconds
Release Date: Nov. 27, 2024


#NASA #Space #Science #ISS #Earth #LEO #SpaceX #Starlink #Satellites #SatelliteConstellations #TelecommunicationServices #Astronauts #Astronaut #DonPettit #AstronautPhotography #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #SpaceLaboratory #HumanSpaceflight #UnitedStates #Expedition72 #STEM #Education #HD #Video

Long March-12 Success Marks Milestone for China's Commercial Launch Services

Long March-12 Success Marks Milestone for China's Commercial Launch Services


The launch of the Long March-12 carrier rocket on Saturday, November 30, 2024, marks the beginning of operations at China's first-ever commercial launch site and signifies a major milestone for the nation, according to experts.

The Long March-12 carrier rocket blasted off at 22:25 (Beijing Time) from the site's No. 2 launch pad, successfully sending two experimental satellites into their planned orbits.

The launch mission achieved complete success at 22:48, according to Hainan provincial authorities.

Developed by the Shanghai Academy of Spaceflight Technology under the China Aerospace Science and Technology Corporation (CASC), it is currently the country's largest single-core carrier rocket in payload capacity. It features a two-stage configuration propelled by six liquid oxygen/kerosene engines, with a length of about 62 meters and a diameter of 3.8 meters.

The rocket is designed with a carrying capacity of no less than 12 tonnes in low Earth orbit and no less than six tonnes in 700-km sun-synchronous orbit.

Construction work on the Hainan commercial space launch site commenced in July 2022, and it is now the country's first launch site dedicated to commercial missions.The site currently features two launch pads for liquid-propellant rockets. The No. 1 pad is designed for the Long March-8, China's new-generation medium-lift carrier rocket, while the No. 2 pad can accommodate multiple rocket types with varying diameters from commercial rocket companies. Each pad has an annual launch capacity of 16 launches.

Saturday's launch was the 548th flight mission of the Long March rocket series.


Video Credit: CCTV
Duration: 48 seconds
Release Date: Dec. 1, 2024

#NASA #Space #Science #Earth #China #中国 #CNSA #中国国家航天局 #LongMarch12 #长征十二号运载火箭 #Rocket #CarrierRocket #MediumLift #CASC #SpaceTechnology #Engineering #CommercialSpace #Spaceflight #WSLS #Wenchang #Hainan #STEM #Education #HD #Video

A Cosmic Wreath: Barnard 3 in Perseus | NASA WISE Mission

A Cosmic Wreath: Barnard 3 in Perseus | NASA WISE Mission

NASA's Wide-field Infrared Survey Explorer (WISE) Mission presents the "Wreath Nebula." Although this is not the nebula's official name (it is actually called Barnard 3, or IRAS Ring G159.6-18.5), one might picture a wreath in these bright green and red dust clouds—a ring of evergreens donned with a festive red bow, a jaunty sprig of holly, and silver bells throughout. Interstellar clouds like these are stellar nurseries, places where baby stars are being born.

Wreaths are part of many ancient traditions dating back to the earliest civilizations. The circle is a symbol of immortality; throughout history, wreaths have been associated with life, rejuvenation, and renewal. Originally, wreaths were worn around the head, neck, or waist.

The Greeks awarded laurel wreaths to their triumphant athletes; in the Persian Empire, they were worn on the head as a symbol of importance; and ancient Romans wore them like crowns. In Sweden, candles were incorporated into the wreaths to celebrate the return of light after the winter solstice. Nowadays, we use them in a window or on a door as a sign of welcome during the holidays.

In this NASA WISE infrared image, the green ring (evergreen) is made of tiny particles of warm dust whose composition is very similar to smog found here on Earth. The red cloud (bow) in the middle is probably made of dust that is more metallic and cooler than the surrounding regions. The bright star in the middle of the red cloud, called HD 278942, is so luminous that it is likely what is causing most of the surrounding ring to glow. In fact, its powerful stellar winds are what cleared out the surrounding warm dust and created the ring-shaped feature in the first place. The bright greenish-yellow region left of center (holly) is similar to the ring, though more dense. The bluish-white stars (silver bells) scattered throughout are stars located both in front of, and behind, the nebula.

Regions similar to this nebula are found near the band of the Milky Way galaxy in the night sky. The “wreath” is slightly off this band, near the boundary between the constellations of Perseus and Taurus, but at a relatively close distance of only about 1,000 light-years, the cloud is a still part of our Milky Way.

The colors used in this image represent specific wavelengths of infrared light. Blue and cyan (blue-green) represent light emitted at wavelengths of 3.4 and 4.6 microns, which is predominantly from stars. Green and red represent light from 12 and 22 microns, respectively, which is mostly emitted by dust.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., managed and operated the Wide-field Infrared Survey Explorer for NASA's Science Mission Directorate, Washington. The principal investigator was Edward Wright at UCLA. 



Image Credit: NASA/JPL-Caltech/UCLA
Caption Credit: JPL-Caltech/Robin Sweetser
Release Date: Dec. 22, 2011

#NASA #Space #Astronomy #Science #WISE #WISEMission #SpaceTelescope #InfraredAstronomy #Nebulae #Nebula #Barnard3 #IRASRingG1596185 #WreathNebula #Star #HD278942 #Perseus #Constellation #Cosmos #Universe #JPL #Caltech #UCLA #California #GSFC #UnitedStates #History #STEM #Education

Saturday, November 30, 2024

The North America Nebula in Cygnus | Palomar Observatory

The North America Nebula in Cygnus | Palomar Observatory

NGC 7000, also known as the North America Nebula, is a giant emission nebula in the constellation of Cygnus at a distance of about 1,800 light years. This image is a composite from black and white images taken with the Palomar Observatory's 48-inch (1.2 meter) Samuel Oschin Telescope in California as a part of the second National Geographic Palomar Observatory Sky Survey (POSS II). The images were recorded on two glass photographic platesone sensitive to red light and the other to blue and later they were digitized. 


In order to produce the color image seen here a total of 62 different frames were processed with the European Space Agency/European Southern Observatory/NASA Photoshop FITS Liberator by Italian amateur astronomer Davide De Martin31 frames for each color band, coming from 4 different plates taken between 1990 and 1993. The original file is 14,264 x 15,429 pixels with a resolution of about 1 arc-second per pixel. The image covers an area of sky larger than 4› x 4.3› (for comparison, the Full Moon is about 0.5› in diameter).

Learn more about the Palomar Observatory and the Samuel Oschin Telescope:

https://sites.astro.caltech.edu/palomar/about/telescopes/oschin.html


Credit: Davide De Martin (ESA/Hubble), the ESA/ESO/NASA Photoshop FITS Liberator & Digitized Sky Survey 2
Release Date: Aug. 8, 2005


#NASA #Astronomy #Space #Science #Stars #Nebulae #Nebula #NGC7000 #Caldwell20 #NorthAmericaNebula #EmissionNebula #Cygnus #Constellation #Star #Deneb #MilkyWayGalaxy #Cosmos #Universe #DSS2 #STScI #SamuelOschinTelescope #PalomarObservatory #California #UnitedStates #STEM #Education

The North America Nebula & The Pelican Nebula | Kitt Peak National Observatory

The North America Nebula & The Pelican Nebula | Kitt Peak National Observatory


The North America Nebula (NGC 7000), named for its resemblance to the North American continent here on Earth, is located in the constellation of Cygnus, along with the Pelican Nebula (IC 5070) at a distance of about 1,800 light years. Most of the nebulosity shown here is in the foreground (superimposed) of the band of the Milky Way. The stars are very dense towards this spiral arm and where the dust and gas thins, their numbers are plain to see.This four frame mosaic subtends more than 4 degrees of the sky. You could easily fit over 30 Moons in this picture! 

The very bright star on the right of the frame is Deneb, and surprisingly it is not associated with the nebula as it is well over 1,500 light years away. Indeed, if Deneb were 50 times closer (30 light years, I am insinuating absolute magnitude) it would be brighter than Venus in the sky and rival the moon! (-7.2 in magnitude). However, the wonderfully glowing clouds shown here are closer, and until recently the star (or stars) responsible for making them glow was a mystery.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.


Credit: KPNO/NOIRLab/NSF/AURA/Adam Block
Release Date: June 11, 2014


#NASA #Astronomy #Space #Science #Stars #Nebulae #Nebula #NGC7000 #Caldwell20 #NorthAmericaNebula #EmissionNebula #PelicanNebula #IC5070 #Cygnus #Constellation #Star #Deneb #MilkyWayGalaxy #Cosmos #Universe #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

North America Nebula Flythrough: Fulldome View | NASA/JPL

North America Nebula Flythrough: Fulldome View | NASA/JPL

NGC 7000, also known as the North America Nebula, is a giant emission nebula within the Milky Way Galaxy in the constellation of Cygnus at a distance of about 1,800 light years.

Note: The full dome video display format is designed for projection systems in planetariums.


Credits:
Image Credit: NASA/ JPL-Caltech/ L. Rebull (SCC/Caltech)/ D. De Martin
Animation Credit: Robert Sawallisch (Zeiss-Planetarium Jena)
Duration: 27 seconds
Release Date: June 14, 2018

#NASA #Astronomy #Space #Science #Stars #Nebulae #Nebula #NGC7000 #Caldwell20 #NorthAmericaNebula #EmissionNebula #Cygnus #Constellation #MilkyWayGalaxy #Cosmos #Universe #JPL #Caltech #UnitedStates #STEM #Education #Planetariums #Fulldome #HD #Video

The North America Nebula: NGC 7000 East | WIYN Telescope

The North America Nebula: NGC 7000 East | WIYN Telescope

NGC 7000, also known as the North America Nebula, is a giant emission nebula in the constellation of Cygnus at a distance of about 1,800 light years. This image shows the eastern part of the nebula, where beautiful dust lanes are visible. The dust is slowly being eroded and blown away by the light from stars embedded in the nebula. The reddish color is characteristic of hydrogen and it dominates. In 1890, the pioneering German astrophotographer, Max Wolf, noticed this nebula's characteristic shape on a long-exposure photograph, and dubbed it the North America Nebula.

This image was obtained with the wide-field view of the Mosaic camera on the WIYN 0.9m-meter telescope at Kitt Peak National Observatory. 
The image was generated with observations in Hydrogen alpha (red), Oxygen [OIII] (green) and Sulfur [SII] (blue) filters. In this image, North is left, East is down.

The Wisconsin-Indiana-Yale-NOIRLab (WIYN) Observatory is situated atop Kitt Peak National Observatory, a partnership consisting of University of California Irvine, Purdue University, the National Science Foundation’s NOIRLab, and NASA.

Learn more about the WIYN Observatory:
https://www.wiyn.org/0.9m/index.html


Credit: T.A. Rector (University of Alaska Anchorage) and NOIRLab/NSF/AURA
Release Date: June 30, 2020


#NASA #Astronomy #Space #Science #Stars #Nebulae #Nebula #NGC7000 #Caldwell20 #NorthAmericaNebula #EmissionNebula #Cygnus #Constellation #MilkyWayGalaxy #Cosmos #Universe #WIYNTelescope #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

The North America Nebula: NGC 7000 South | WIYN Telescope

The North America Nebula: NGC 7000 South | WIYN Telescope


NGC 7000, also known as the North America Nebula, is a giant emission nebula in the constellation of Cygnus at a distance of about 1,800 light years. This image shows only the southern tip of the nebula (the Mexico part of the nebula). The nebula is being energized by the light from stars embedded within. In 1890, the pioneering German astrophotographer, Max Wolf, noticed this nebula's characteristic shape on a long-exposure photograph, and dubbed it the North America Nebula.

This image was obtained with the wide-field view of the Mosaic camera on the WIYN 0.9m-meter telescope at Kitt Peak National Observatory. 

The image was generated with observations in Hydrogen alpha (red), Oxygen [OIII] (green) and Sulfur [SII] (blue) filters. In this image, North is up, East is to the left.

The Wisconsin-Indiana-Yale-NOIRLab (WIYN) Observatory is situated atop Kitt Peak National Observatory, a partnership consisting of University of California Irvine, Purdue University, the National Science Foundation’s NOIRLab, and NASA.

Learn more about the WIYN Observatory:
https://www.wiyn.org/0.9m/index.html


Credit: T.A. Rector (University of Alaska Anchorage) and NOIRLab/NSF/AURA
Release Date: April 15, 2015


#NASA #Astronomy #Space #Science #Stars #Nebulae #Nebula #NGC7000 #Caldwell20 #NorthAmericaNebula #EmissionNebula #Cygnus #Constellation #MilkyWayGalaxy #Cosmos #Universe #WIYNTelescope #KPNO #KittPeakNationalObservatory #Arizona #NOIRLab #NSF #AURA #UnitedStates #STEM #Education

Supercomputer 3D Simulation of Our Sun's Turbulent Upper Layers | NASA Ames

Supercomputer 3D Simulation of Our Sun's Turbulent Upper Layers | NASA Ames

A 3D simulation showing the evolution of turbulent flows in the upper layers of the Sun. The more saturated and bright reds represent the most vigorous upward or downward twisting motions. Clear areas represent areas where there are only relatively slow up-flows, with very little twisting.

NASA supercomputers are shedding light on what causes the Sun’s most complex behaviors. Using data from the suite of active Sun-watching spacecraft currently observing the star at the heart of our solar system, researchers can explore solar dynamics like never before. This animation shows the strength of the turbulent motions of the Sun’s inner layers as materials twist into its atmosphere, resembling a roiling pot of boiling water or a flurry of schooling fish sending material bubbling up to the surface or diving it further down below. 

“Our simulations use what we call a realistic approach, which means we include as much as we know to-date about solar plasma to reproduce different phenomena observed with NASA space missions,” said Irina Kitiashvili, a scientist at NASA’s Ames Research Center in California’s Silicon Valley who helped lead the study. 

Using modern computational capabilities, the team was able for the first time to reproduce the fine structures of the subsurface layer observed with NASA’s Solar Dynamics Observatory.

“Right now, we don’t have the computational capabilities to create realistic global models of the entire Sun due to the complexity,” said Kitiashvili. “Therefore, we create models of smaller areas or layers, which can show us structures of the solar surface and atmosphere—like shockwaves or tornado-like features measuring only a few miles in size; that’s much finer detail than any one spacecraft can resolve.”

Scientists seek to better understand the Sun and what phenomena drive the patterns of its activity. The connection and interactions between the Sun and Earth drive the seasons, ocean currents, weather, climate, radiation belts, auroras and many other phenomena. Space weather predictions are critical for exploration of space, supporting the spacecraft and astronauts of NASA’s Artemis campaign. Surveying this space environment is a vital part of understanding and mitigating astronaut exposure to space radiation and keeping our spacecraft and instruments safe.

This has been a big year for our special star, studded with events like the annular eclipse, a total eclipse, and the Sun reaching its solar maximum period. In December 2024, NASA’s Parker Solar Probe mission—that is helping researchers to understand space weather right at the source—will make its closest-ever approach to the Sun and beat its own record of being the closest human-made object to reach the Sun. 

“The Sun keeps surprising us,” said Kitiashvili. “We are looking forward to seeing what kind of exciting events will be organized by the Sun.”

These simulations were run on the Pleaides supercomputer at the NASA Advanced Supercomputing facility at NASA Ames over several weeks of runtime, generating terabytes of data.

Learn more about NASA's Advanced Supercomputing (NAS) Division at the Ames Research Center: https://www.nas.nasa.gov/index.html

https://www.nas.nasa.gov/pubs/stories/2014/feature_Sun_Kitiashvili.html


3D Visualization Credit: NASA/Irina Kitiashvili and Timothy A. Sandstrom
Duration: 26 seconds
Release Date: Nov. 21, 2024

#NASA #Space #Astronomy #Science #Sun #SolarPlasma #SpaceWeather #NASASDO #ParkerSolarProbe #SolarSystem #Heliophysics #Astrophysics #NASASupercomputers #Supercomputers #SupercomputerSimulations #NASAAmes #UnitedStates #STEM #Education #Visualizations #3DSimulations #Animation #HD #Video

Planet Earth's Exceptional & Unexpected Heat of 2023 & 2024 | NASA GISS

Planet Earth's Exceptional & Unexpected Heat of 2023 & 2024 | NASA GISS

Temperatures 1880 - October 2024

This chart shows Schmidt’s expectation for how much monthly temperatures from January 2023 to August 2024 would differ from NASA’s 1951-1980 baseline (also known as an anomaly). The expectation (represented as the dashed line in the chart) was based on an equation that calculates global average temperature based on the most recent 20-year rate of warming (about 0.25°C per decade) and NOAA’s sea surface temperature measurements from the tropical Pacific, accounting for a three-month delay for these temperatures to affect the global average. The shaded area shows the range of variability (plus or minus two standard deviations).

The chart above shows how global temperatures calculated from January 2023 to August 2024 differed from NASA’s baseline (1951–1980). The previous record temperature anomalies for each month—set in 2016 and 2020—are indicated by the red dashed line. Starting in June 2023, temperatures exceeded previous records by 0.3 to 0.5°C every month. Although temperature anomalies in 2024 were closer to past anomalies, they continued to break records through August 2024. The global average temperature in September 2024 was 1.26°C above NASA’s baseline—lower than September 2023 but still 0.3°C above any September in the record prior to 2023.

October 2024 was the second-hottest October ever, according to NASA Goddard Institute for Space Studies' record, GISTEMP.
This October was 1.32°C (or about 2.38°F) above the long-term 1951-1980 average. It was slightly cooler than Oct. 2023, although the margins of error overlap, so the two are effectively tied.

In 2024, global temperatures for June through August 2024 were the hottest on record, narrowly topping the same period in 2023. The exceptional heat extended throughout other seasons, too, with global temperatures breaking records for 15 straight months from June 2023 until August 2024, according to scientists from NASA’s Goddard Institute for Space Studies (GISS).

Although this spell of record heat fits within a long-term warming trend driven by human activity—primarily greenhouse gas emissions—the intensity of the heat, reaching a crescendo in the last half of 2023, surprised leading climate scientists. In a commentary in Nature, Gavin Schmidt, the director of GISS, used words like “humbling” and “confounding” to explain just how far temperatures overshot expectations during that period.

“Warming in 2023 was head-and-shoulders above any other year, and 2024 will be as well,” Schmidt said. “I wish I knew why, but I don’t. We’re still in the process of assessing what happened and if we are seeing a shift in how the climate system operates.”

Setting Expectations

Earth’s air and ocean temperatures during a given year typically reflect a combination of long-term trends, such as those associated with climate change, and shorter-term influences, such as volcanic activity, solar activity, and the state of the ocean.

In late 2022, as he has done each year since 2016, Schmidt used a statistical model to project global temperatures for the coming year. La Niña—which cools sea surface temperatures in the tropical Pacific—was present for the first part of 2023 and should have taken the edge off global temperatures. Schmidt calculated that average 2023 global temperatures would reach about 1.22 degrees Celsius above the baseline, putting it in the top three or four warmest years, but that it would not be a record-breaking year. Scientists at the UK Met Office, Berkeley Earth, and Carbon Brief made similar assessments using a variety of methods.

“More complex global climate models are helpful to predict long-term warming, but statistical models like these help us project year-to-year variability, which is often dominated by El Niño and La Niña events,” said Zeke Hausfather, a climate scientist at the University of California, Berkeley. Hausfather helps produce the Berkeley Earth global temperature record and also generates annual predictions of global temperature changes based on those data.

Schmidt’s statistical model—that successfully predicted the global average temperature every year since 2016—underestimated the exceptional heat in 2023, as did the methods used by Hausfather and other climatologists. Schmidt expected global temperature anomalies to peak in February or March 2024 as a lagged response to the additional warming from El Niño. Instead, the anomalous heat emerged well before El Niño had peaked. And the heat came with unexpected intensity—first in the North Atlantic Ocean and then virtually everywhere.

“In September, the record was broken by an absolutely astonishing 0.5 degrees Celsius,” Schmidt said. “That has not happened before in the GISS record.”

To calculate Earth’s global average temperature changes, NASA scientists analyze data from tens of thousands of meteorological stations on land, plus thousands of instruments on ships and buoys on the ocean surface. The GISS team analyzes this information using methods that account for the varied spacing of temperature stations around the globe and for urban heating effects that could skew the calculations.

Investigating Possible Contributors

Since May 2024, Schmidt has been compiling research about possible contributors to the unexpected warmth, including changes in greenhouse gas emissions, incoming radiation from the Sun, airborne particles called aerosols, and cloud cover, as well as the impact of the 2022 Hunga Tonga-Hunga Ha’apai volcanic eruption. However, none of these factors provide what Schmidt and other scientists consider a convincing explanation for the unusual heat in 2023.

Atmospheric greenhouse gas levels have continued to rise, but Schmidt estimates that the extra load since 2022 only accounted for additional warming of about 0.02°C. The Sun was nearing peak activity in 2023, but its roughly 11-year cycle is well measured and not enough to explain the temperature surge either.

Major volcanic eruptions, such as El Chichón in 1982 and Pinatubo in 1991, have caused brief periods of global cooling in the past by lofting aerosols into the stratosphere. And research published in 2024 indicates the eruption in Tonga had a net cooling effect in 2022 and 2023. “If that’s the case, there’s even more warming in the system that needs to be explained,” Schmidt said.

Another possible contributor is reduced air pollution. A research team led by Tianle Yuan, an atmospheric research scientist at NASA’s Goddard Space Flight Center, has found a significant drop in aerosol pollution from shipping since 2020. The drop coincides with new international regulations on sulfur content in shipping fuels and with sporadic drops in shipping due to the coronavirus pandemic.

Sulfur aerosol emissions promote the formation of bright clouds that reflect incoming sunlight back to space and have a net cooling effect. Reducing this pollution has the opposite effect: clouds are less likely to form. This could warm the climate. Although scientists, including Yuan, generally agree that the drop in sulfur emissions likely caused a net warming in 2023, the scientific community continues to debate the precise size of the effect.

“All of these factors explain, perhaps, a tenth of a degree in warming,” Schmidt said. “Even after taking all plausible explanations into account, the divergence between expected and observed annual mean temperatures in 2023 remains near 0.2°C—roughly the gap between the previous and current annual record.”

Grappling With Uncertainty

Both Hausfather and Schmidt expressed concern that these unexpected temperature changes could signal a shift in how the climate system functions. It could also be some combination of climate variability and a change in the system, Schmidt said. “It doesn’t have to be an either-or.”

One of the biggest uncertainties in the climate system is how aerosols affect cloud formation, which in turn affects the amount of radiation reflected back to space. However, one challenge for scientists trying to piece together what happened in 2023 is the lack of updated global aerosol emissions data. “Reliable assessments of aerosol emissions depend on networks of mostly volunteer-driven efforts, and it could be a year or more before the full data from 2023 are available,” Schmidt said.

NASA’s PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) satellite, which launched in February 2024, could help shed light on these uncertainties. The satellite will help scientists make a global assessment of the composition of various aerosol particles in the atmosphere. PACE data may also help scientists understand cloud properties and how aerosols influence cloud formation. This is essential to creating accurate climate models.

Schmidt and Hausfather invite scientists to discuss research related to the contributors of the 2023 heat at a session they are convening at the fall meeting of the American Geophysical Union in Washington, D.C., on December 9–13, 2024.

Updates and more at NASA's Goddard Institute for Space Studies (GISS):


Credits: NASA Earth Observatory map and charts/Michala Garrison/NASA Goddard Institute for Space Studies/Climate spiral visualization by Mark SubbaRao, NASA/GSFC/Center/Scientific Visualization Studio
Article Credit: Emily Cassidy
Release Date: Nov. 20, 2024


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Dark Nebula LDN 1519 in Auriga

Dark Nebula LDN 1519 in Auriga


Dark nebula LDN 1519 lies in the constellation Auriga. The Auriga constellation lies in the northern hemisphere. Its name means “the charioteer” in Latin. Lynds' astronomical Catalogue of Dark Nebulae (abbreviation: LDN) was originally published in 1962. It was based on a study of the red and blue prints of the National Geographic - Palomar Observatory Sky Atlas. Objects listed in the catalog are numbered with the prefix LDN. Beverly Turner Lynds (August 19, 1929 – October 5, 2024) was best known for compiling the Lynds' Catalogue of Dark Nebulae. We honor her many lasting contributions to astronomical science.

Image Credit: Frankastro
Release Date: Nov. 30, 2024

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Friday, November 29, 2024

How Earth radar satellites are used to help humanity | European Space Agency

How Earth radar satellites are used to help humanity | European Space Agency

Radar allows us to see through what would otherwise be invisible. By sending out radio waves that bounce off objects and return as echoes, radar creates a detailed picture of our surrounding world.

This technology is everywhere—from guiding air traffic and enabling self-driving cars to tracking the movements of athletes. However, its reach does not stop there—radar is also transforming how we observe Earth from space.

Satellites like Europe's Copernicus Sentinel-1 Mission use radar to see through clouds, darkness and any weather conditions. This capability is valuable for detecting subtle changes on Earth’s surface—changes that are often hidden from the human eye. Discover how radar technology is helping us unlock these hidden insights about our planet.

Learn more about the European Space Agency's Copernicus Earth Observation Programme:

https://sentinel.esa.int/web/sentinel/copernicus/


Video Credit: European Space Agency (ESA)
Duration: 7 minutes, 40 seconds
Release Date: Nov. 28, 2024


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