Wednesday, June 12, 2024

A Tribute to Scientist & Explorer Edward C. Stone (1936-2024) | NASA/JPL

A Tribute to Scientist & Explorer Edward C. Stone (1936-2024) | NASA/JPL

Edward C. Stone, former director of NASA’s Jet Propulsion Laboratory (JPL) and longtime project scientist of the Voyager mission, passed away on June 9, 2024. He was 88 years old. In this 2018 video, Stone talks about the Voyager 2 spacecraft reaching interstellar space, six years after Voyager 1 reached the same milestone. The twin Voyager spacecraft were launched in 1977 on a five-year mission that is still operating today. Stone served as the mission’s project scientist for 50 years, from 1972 to 2022.

In addition to his work on Voyager, Stone was the director of JPL from 1991 to 2001. Under his leadership, JPL was responsible for 21 missions and instruments and developed six new missions. Highlights during Stone’s tenure included landing NASA’s Pathfinder mission with the first Mars rover, Sojourner, in 1996 and launching the NASA-European Space Agency (ESA) Cassini/Huygens mission in 1997. The first Saturn orbiter, Cassini was a direct outgrowth of the scientific questions that arose from Voyager’s two flybys, and it carried the only probe that has ever landed in the outer solar system (at Titan).

The twin Voyager 1 and 2 spacecraft are traveling where no spacecraft—or anything touched by humanity—has gone before. As we prepare to celebrate the 47th anniversary of the Voyager 1 launch later this year, we reflect on the vision and work of people like Ed Stone that supported its achievements and enduring legacy.


Video Credit: NASA's Jet Propulsion Laboratory (JPL)

Duration: 2 minutes

Release Date: June 11, 2024


#NASA #Astronomy #Space #Science #VoyagerSpacecraft #Voyager1 #Voyager2 #Planets #Mars #Jupiter #Saturn #SolarSystem #InterstellarSpace #MilkyWayGalaxy #SpaceExploration #EdStone #EdwardStone #Scientist #Explorer #JPL #Caltech #History #UnitedStates #STEM #Education #HD #Video

Expedition 71 & Crew Flight Test Team Portrait | International Space Station

Expedition 71 & Crew Flight Test Team Portrait | International Space Station

The seven Expedition 71 crew members gather with the two Crew Flight Test members for a team portrait aboard the International Space Station. In the front from left are, Suni Williams, Oleg Kononenko (Russia), and Butch Wilmore. Second row from left are, Alexander Grebenkin (Russia), Tracy C. Dyson, and Mike Barratt. In the back are, Nikolai Chub (Russia), Jeanette Epps, and Matthew Dominick.

Boeing's Starliner spacecraft carrying Crew Flight Test (CFT) members and NASA astronauts Butch Wilmore and Suni Williams docked with the station on June 6, 2024.

Follow Expedition 71 Updates: 


Expedition 71 Crew
Station Commander: Oleg Kononenko (Russia)
Roscosmos (Russia): Nikolai Chub, Alexander Grebenkin (Russia)
NASA: Tracy Dyson, Matthew Dominick, Mike Barrett, Jeanette Epps

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. The ISS has been the most politically complex space exploration program ever undertaken.

Image Credit: NASA's Johnson Space Center (JSC)

Image Date: June 6, 2024


#NASA #Space #Earth #ISS #Science #Astronauts #BoeingStarliner #CFTCrew #HumanSpaceflight #SpaceTechnology #SpaceLaboratory #Engineering #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #Expedition71 #STEM #Education

Tuesday, June 11, 2024

NASA Analysis Confirms a Year of Monthly Temperature Records | NASA Goddard

NASA Analysis Confirms a Year of Monthly Temperature Records | NASA Goddard


May 2024 was the warmest May on the books, marking a full year of record-high monthly temperatures, NASA scientists found. Average global temperatures for the past 12 months hit record highs for each respective month—an unprecedented streak—according to scientists from NASA’s Goddard Institute for Space Studies (GISS) in New York.

The run of record temperatures fits within a long-term warming trend driven by human activity—primarily greenhouse gas emissions. The trend has become evident over the past four decades, with the last 10 consecutive years being the warmest 10 since record-keeping began in the late 19th century. Before this streak of 12 straight months of record temperatures, the second longest streak lasted for seven months between 2015 and 2016.

“It’s clear we are facing a climate crisis. Communities across America—like Arizona, California, Nevada—and communities across the globe are feeling first-hand extreme heat in unprecedented numbers.

—NASA Administrator Bill Nelson

“We’re experiencing more hot days, more hot months, more hot years,” said Kate Calvin, NASA’s chief scientist and senior climate advisor. “We know that these increases in temperature are driven by our greenhouse gas emissions and are impacting people and ecosystems around the world.”

In NASA’s analysis, a temperature baseline is defined by several decades or more—typically 30 years. The average global temperature over the past 12 months was 2.34 degrees Fahrenheit (1.30 degrees Celsius) above the 20th century baseline (1951 to 1980). This is slightly over the 2.69 degree Fahrenheit (1.5 degree Celsius) level with respect to the late 19th century average.

To calculate Earth’s global temperature, NASA scientists gather data from tens of thousands of meteorological stations on land, plus thousands of instruments on ships and buoys on the ocean surface. This raw data is analyzed using methods that account for the varied spacing of temperature stations around the globe and for urban heating effects that could skew the calculations.

El Niño Subsiding, La Niña Arriving?

Phenomena such as El Niño and La Niña, which alternately warm and cool the tropical Pacific Ocean, can contribute a small amount of variability in global temperatures from year to year. The strong El Niño that began in spring 2023 helped stoke last year’s extreme summer and fall heat.

As of May 2024, scientists at the National Oceanic and Atmospheric Administration (NOAA) Climate Prediction Center projected a 49% chance of La Niña developing between June and August, and a 69% chance of it developing between July and September. By cooling a large swath of the tropical Pacific, a La Niña event could partially suppress average global temperatures this year.

"It’s hard to know whether 2024 will set another global heat record. Factors like volcanic eruptions and sun-blocking aerosol emissions can affect our climate in any given year. NASA missions are actively studying these influences," said Gavin Schmidt, director of GISS.

“There are open questions that can impact our predictions over the next few years and decades, and we’re in evidence-gathering mode,” Schmidt said. “This year may well end up setting another global temperature record. Right now, it’s in line to be close to 2023.”

Ocean Temperatures and Hurricanes

Scientists are watching to see how ocean temperatures may influence this year’s hurricane season. Temperatures remained high as the 2024 hurricane and typhoon seasons got underway. Across the Northern Hemisphere, ocean temperatures for the January-April period were 2.12 degrees Fahrenheit (1.18 degrees Celsius) above average, according to NOAA. Despite the waning El Niño, temperatures at the sea surface and at deeper depths are still above average in many places, said Josh Willis, an oceanographer at NASA’s Jet Propulsion Laboratory in Southern California.

Willis cited rising carbon dioxide emissions as the main driver of ocean warming. As much as 90% of the excess atmospheric heat in recent decades has been absorbed by the ocean, with much of that heat stored near the water surface.  

“The ocean is the flywheel of our climate,” Willis said. “Since the ocean covers more than two-thirds of Earth, whatever sea surface temperatures are, the rest of the planet follows.”  

La Niña years also can contribute to more active Atlantic hurricane seasons. That’s because La Niña conditions weaken westerly winds high in the atmosphere near the Americas, over the Caribbean Sea and tropical Atlantic Ocean. Wind shear—abrupt changes in wind speed and direction—can cut hurricanes down before they grow. La Niña effectively lifts this brake, allowing tropical storms to form and intensify unimpeded.

NASA’s full dataset of global surface temperatures, as well as details of how NASA scientists conducted the analysis, are publicly available from GISS, a NASA laboratory managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland. 

Learn more: NASA Analysis Confirms a Year of Monthly Temperature Records


Credit: NASA's Goddard Space Flight Center (GSFC)/NASA’s Scientific Visualization Studio

Release Date: June 11, 2024


#NASA #Space #Satellites #Science #Planet #Earth #GlobalTemperatureRecords #Weather #Meteorology #Model #ClimateChange #GlobalHeating #Climate #Environment #InSituMeasurements #GlobalTemperatureMap #GreenhouseGases #GHG #EarthObservation #RemoteSensing #NASAGISS #GISS #GSFC #UnitedStates #STEM #Education

NASA Analysis Confirms a Year of Monthly Temperature Records | NASA Goddard

NASA Analysis Confirms a Year of Monthly Temperature Records | NASA Goddard

This visualization shows monthly global surface temperatures from 1880 to May 2024. The last 12 months (June 2023 through May 2024) hit record highs for each respective month. 

May 2024 was the warmest May on the books, marking a full year of record-high monthly temperatures, NASA scientists found. Average global temperatures for the past 12 months hit record highs for each respective month—an unprecedented streak—according to scientists from NASA’s Goddard Institute for Space Studies (GISS) in New York.

The run of record temperatures fits within a long-term warming trend driven by human activity—primarily greenhouse gas emissions. The trend has become evident over the past four decades, with the last 10 consecutive years being the warmest 10 since record-keeping began in the late 19th century. Before this streak of 12 straight months of record temperatures, the second longest streak lasted for seven months between 2015 and 2016.

“It’s clear we are facing a climate crisis. Communities across America—like Arizona, California, Nevada—and communities across the globe are feeling first-hand extreme heat in unprecedented numbers.

—NASA Administrator Bill Nelson

“We’re experiencing more hot days, more hot months, more hot years,” said Kate Calvin, NASA’s chief scientist and senior climate advisor. “We know that these increases in temperature are driven by our greenhouse gas emissions and are impacting people and ecosystems around the world.”

In NASA’s analysis, a temperature baseline is defined by several decades or more—typically 30 years. The average global temperature over the past 12 months was 2.34 degrees Fahrenheit (1.30 degrees Celsius) above the 20th century baseline (1951 to 1980). This is slightly over the 2.69 degree Fahrenheit (1.5 degree Celsius) level with respect to the late 19th century average.

To calculate Earth’s global temperature, NASA scientists gather data from tens of thousands of meteorological stations on land, plus thousands of instruments on ships and buoys on the ocean surface. This raw data is analyzed using methods that account for the varied spacing of temperature stations around the globe and for urban heating effects that could skew the calculations.

El Niño Subsiding, La Niña Arriving?

Phenomena such as El Niño and La Niña, which alternately warm and cool the tropical Pacific Ocean, can contribute a small amount of variability in global temperatures from year to year. The strong El Niño that began in spring 2023 helped stoke last year’s extreme summer and fall heat.

As of May 2024, scientists at the National Oceanic and Atmospheric Administration (NOAA) Climate Prediction Center projected a 49% chance of La Niña developing between June and August, and a 69% chance of it developing between July and September. By cooling a large swath of the tropical Pacific, a La Niña event could partially suppress average global temperatures this year.

"It’s hard to know whether 2024 will set another global heat record. Factors like volcanic eruptions and sun-blocking aerosol emissions can affect our climate in any given year. NASA missions are actively studying these influences," said Gavin Schmidt, director of GISS.

“There are open questions that can impact our predictions over the next few years and decades, and we’re in evidence-gathering mode,” Schmidt said. “This year may well end up setting another global temperature record. Right now, it’s in line to be close to 2023.”

Ocean Temperatures and Hurricanes

Scientists are watching to see how ocean temperatures may influence this year’s hurricane season. Temperatures remained high as the 2024 hurricane and typhoon seasons got underway. Across the Northern Hemisphere, ocean temperatures for the January-April period were 2.12 degrees Fahrenheit (1.18 degrees Celsius) above average, according to NOAA. Despite the waning El Niño, temperatures at the sea surface and at deeper depths are still above average in many places, said Josh Willis, an oceanographer at NASA’s Jet Propulsion Laboratory in Southern California.

Willis cited rising carbon dioxide emissions as the main driver of ocean warming. As much as 90% of the excess atmospheric heat in recent decades has been absorbed by the ocean, with much of that heat stored near the water surface.  

“The ocean is the flywheel of our climate,” Willis said. “Since the ocean covers more than two-thirds of Earth, whatever sea surface temperatures are, the rest of the planet follows.”  

La Niña years also can contribute to more active Atlantic hurricane seasons. That’s because La Niña conditions weaken westerly winds high in the atmosphere near the Americas, over the Caribbean Sea and tropical Atlantic Ocean. Wind shear—abrupt changes in wind speed and direction—can cut hurricanes down before they grow. La Niña effectively lifts this brake, allowing tropical storms to form and intensify unimpeded.

NASA’s full dataset of global surface temperatures, as well as details of how NASA scientists conducted the analysis, are publicly available from GISS, a NASA laboratory managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland. 

Image Description:

Line graph of monthly temperature anomalies for each month of every year from 1880 to May 2024. The X-axis runs from June to May and the Y-axis is anomalies in degrees Celsius from -.5 to 1.5. Each month’s anomaly forms a point on a line for that entire year. As the points appear, the current year’s line is red and fades to yellow then white as newer years are added. Overall, the earlier years in the timespan are much cooler, sometimes dipping even below the -.5 degree Y-axis line. Over time, temperature anomalies increase, as human activities warm the climate, with small variations between individual years. The final 12-month span that runs from June 2023 to May 2024 is a red line running above each of its respective months, representing a full year of record high monthly temperatures. Finally, the graph turns 90 degrees toward the viewer, creating a familiar, annual temperature anomaly line graph. The X-axis changes to years, running from 1880 to 2024, showing overall warming. 

Learn more: NASA Analysis Confirms a Year of Monthly Temperature Records


Credit: NASA's Goddard Space Flight Center (GSFC)/NASA’s Scientific Visualization Studio

Duration: 30 seconds

Release Date: June 11, 2024


#NASA #Space #Satellites #Science #Planet #Earth #GlobalTemperatureRecords #Weather #Meteorology #Model #ClimateChange #GlobalHeating #Climate #Environment #InSituMeasurements #GlobalTemperatureMap #GreenhouseGases #GHG #EarthObservation #RemoteSensing #NASAGISS #GISS #GSFC #UnitedStates #STEM #Education #HD #Video

Planet Earth: A Year of Monthly Temperature Records | NASA Goddard

Planet Earth: A Year of Monthly Temperature Records | NASA Goddard

May 2024 was the warmest May on the books, marking a year of record-breaking monthly temperatures. Globally, average temperatures for the last 12 months hit record highs for each respective month—an unprecedented streak.

Dr. Kate Calvin, NASA's Chief Scientist and Senior Climate Advisor, answers examples of the top questions pertaining to these temperature records and our changing climate.

Learn more: NASA Analysis Confirms a Year of Monthly Temperature Records


Credit: NASA's Goddard Space Flight Center (GSFC)

Katie Jepson (KBR Wyle Services, LLC): Producer, Editor

Katherine Calvin (NASA HQ): Lead Scientist, Interviewee

Mark SubbaRao (NASA/GSFC): Visualizer

Kathleen Gaeta (Advocates in Manpower Management, Inc): Producer

Grace Weikert (KBR Wyle Services, LLC): Producer

Katy Mersmann (NASA GSFC): Producer, Social 

Sofie Bates (KBR Wyle Services, LLC): Producer, Social

Rob Andreoli (Advocates in Manpower Management, Inc.): Videographer

John D. Philyaw (Advocates in Manpower Management, Inc.): Videographer

Duration: 3 minutes

Release Date: June 11, 2024


#NASA #Space #Satellites #Science #Planet #Earth #GlobalTemperatureRecords #Weather #Meteorology #Model #ClimateChange #GlobalHeating #Climate #Environment #InSituMeasurements #GlobalTemperatureMap #GreenhouseGases #GHG #EarthObservation #RemoteSensing #NASAGISS #GISS #GSFC #UnitedStates #STEM #Education #HD #Video

Advancing Plant Science with Space Gardens | International Space Station

Advancing Plant Science with Space Gardens | International Space Station

Gardens growing on the International Space Station are leading to groundbreaking research and offering astronauts a taste of home. 

Learn more about eXposed Root On-Orbit Test System (XROOTS) Tech Demo

https://science.nasa.gov/biological-physical/investigations/xroots

The Vegetable Production System, or “Veggie":

https://www.nasa.gov/missions/station/ways-the-international-space-station-helps-us-study-plant-growth-in-space/

Follow Expedition 71 Updates: 


Expedition 71 Crew
Station Commander: Oleg Kononenko (Russia)
Roscosmos (Russia): Nikolai Chub, Alexander Grebenkin (Russia)
NASA: Tracy Dyson, Matthew Dominick, Mike Barrett, Jeanette Epps

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. The ISS has been the most politically complex space exploration program ever undertaken.

Video Credit: National Aeronautics and Space Administration (NASA)

Duration: 2 minutes, 37 seconds

Release Date: June 11, 2024


#NASA #Space #Earth #ISS #Science #Botany #Gardening #XROOTS #Veggie #PlantHabitat #FreshFood #Vegetables #Astronauts #HumanSpaceflight #SpaceTechnology #SpaceLaboratory #Engineering #UnitedStates #Cosmonauts #Russia #Россия #Roscosmos #Роскосмос #InternationalCooperation #Expedition71 #STEM #Education #HD #Video

Mars Images: June 2024 | NASA Mars Curiosity & Perseverance Rovers

Mars Images: June 2024 | NASA Mars Curiosity & Perseverance Rovers

MSL - sol 4206
MSL - sol 4207
MSL - sol 4207
MSL - sol 4207
MSL - sol 4505
Mars 2020 - sol 1171
MSL - sol 4210 (Note: slight image misalignment)
MSL - sol 4209

Celebrating 11+ Years on Mars (2012-2024)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 3+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Dates: June 6-11, 2024

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Boeing's Starliner Crew Spacecraft Approaches the International Space Station

Boeing's Starliner Crew Spacecraft Approaches the International Space Station


This view from a window on the cupola overlooks Japan's Kibo laboratory module as Boeing's Starliner spacecraft carrying NASA astronauts Butch Wilmore and Suni Williams approaches the International Space Station prior to autonomous docking on June 6, 2024. Starliner launched on June 5, with NASA astronauts Butch Wilmore and Suni Williams aboard, as part of NASA's Boeing Crew Flight Test (CFT). This first crewed flight of Starliner aims to certify the spacecraft for rotational missions to the space station.

NASA’s Commercial Crew Program works with the American aerospace industry to provide safe, reliable, and cost-effective transportation to and from the orbital outpost on American-made rockets and spacecraft launching from American soil.

Learn more about NASA’s Commercial Crew Program at: 

https://www.nasa.gov/commercialcrew


Image Credit: NASA's Johnson Space Center (JSC)

Image Date: June 6, 2024


#NASA #Space #Earth #ISS #KiboLaboratory #Japan #日本 #JAXA #Boeing #Starliner #CST100 #CommercialCrewProgram #CFT #Astronauts #SuniWilliams #BarryWilmore #HumanSpaceflight #SpaceTechnology #Engineering #LaunchAmerica #CommercialSpace #UnitedStates #STEM #Education

NASA Astronaut Suni Williams Answers Student Questions | International Space Station

NASA Astronaut Suni Williams Answers Student Questions | International Space Station

NASA astronaut Suni Williams discussed living and working in space as part of the Crewed Flight Test (CFT) of the Boeing Starliner spacecraft during an in-flight interview with the Sunita L. Williams Elementary School in Needham, Massachusetts on June 10, 2024. 

Williams is an alumnus of the school and is the midst of completing a test flight to check out Starliner’s systems ahead of spacecraft certification. Williams will remain at the space station for about a week to complete a series of test objectives before departing the complex for a landing in the southwestern United States alongside NASA astronaut Butch Wilmore. 

For more info on CFT and Starliner, visit: boeing.com/starliner

Follow Expedition 71 Updates: 


Expedition 71 Crew
Station Commander: Oleg Kononenko (Russia)
Roscosmos (Russia): Nikolai Chub, Alexander Grebenkin (Russia)
NASA: Tracy Dyson, Matthew Dominick, Mike Barrett, Jeanette Epps

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. The ISS has been the most politically complex space exploration program ever undertaken.

NASA’s Commercial Crew Program works with the American aerospace industry to provide safe, reliable, and cost-effective transportation to and from the orbital outpost on American-made rockets and spacecraft launching from American soil.

Learn more about NASA’s Commercial Crew Program at: 

https://www.nasa.gov/commercialcrew


Video Credit: NASA's Johnson Space Center (JSC)

Duration: 25 minutes

Release Date: June 10, 2024


#NASA #Space #Earth #ISS #Boeing #Starliner #CST100 #CommercialCrewProgram #CFT #Astronauts #SuniWilliams #BarryWilmore #Cosmonauts #Russia #Россия #Roscosmos #HumanSpaceflight #SpaceTechnology #Engineering #Students #Massachusetts #UnitedStates #InternationalCooperation #STEM #Education #HD #Video

Astronauts Selected for China's Crewed Moon Missions: Chief Designer

Astronauts Selected for China's Crewed Moon Missions: Chief Designer

China has selected a new batch of astronauts to prepare for its crewed lunar exploration programs, said Huang Weifen, chief designer of the manned space program's astronaut system.

The China Manned Space Agency (CMSA) announced Tuesday, June 11, 2024, that 10 candidates, including eight space pilots and two payload specialists, have been selected as the country's fourth batch of astronauts.

Of the two payload specialists, one is from the Hong Kong Special Administrative Region and the other is from the Macao Special Administrative Region, said the CMSA.

It added that this is first time it has selected payload specialists from the Hong Kong and Macao regions, a move that has garnered strong support and enthusiastic responses from these communities.

"The payload specialists from Hong Kong and Macao have undergone a rigorous selection process, from initial screenings to the secondary selection, with comprehensive medical examinations, physiological function tests, endurance tests for space environment adaptability, various psychological assessments, and evaluations of professional qualities. And we also conducted inspection visits and interviews for the final decision. They have met our criteria for selection," said Huang.

The CMSA announced in late May 2024 that China plans to realize manned lunar landing by 2030. Huang said the building of a astronaut team, from the selection of astronauts to the training programs, has been designed to support both the space station missions and future lunar missions.

"For the training of our existing second and third batches of astronauts, as well as the upcoming fourth batch, we have opened fundamental courses related to geology. We have also arranged for the astronauts relevant training, including field studies and geological surveys. When the development of training simulators for crewed lunar missions is completed, we will be able to unfold more substantive training tasks. Currently, we are making preliminary preparations and involving both our existing astronauts and the newly selected astronauts in engineering development work to allow them to study in the frontline of scientific research and to make the technical reserve for future missions," said Huang.


Video Credit: China Central Television (CCTV) Video News Agency

Duration: 2 minutes

Release Date: June 11, 2024


#NASA #CNSA #CMSA #Space #Astronomy #Science #China #中国 #Moon #Astronauts #Taikonauts #Training #Geology #HongKong #Macao #HumanSpaceflight #CLEP #SpaceTechnology #SpaceExploration #SolarSystem #STEM #Education #History #HD #Video

Comet Pons-Brooks Develops Opposing Tails

Comet Pons-Brooks Develops Opposing Tails

Why does Comet Pons-Brooks now have tails pointing in opposite directions? The most spectacular tail is the blue-glowing ion tail that is visible flowing down the image. The ion tail is pushed directly out from the Sun by the solar wind. On the upper right is the glowing central coma of Comet 12P/Pons–Brooks. Fanning out from the coma, mostly to the left, is the comet's dust tail. Pushed out and slowed down by the pressure of sunlight, the dust tail tends to trail the comet along its orbit. It can appear opposite to the ion tail at certain angles. 

The distant, bright star Alpha Leporis is seen at the bottom of this featured image captured last week from Namibia. On June 2, 2024, the comet passed its closest to the Earth and is now best visible from southern skies as it dims and glides back to the outer Solar System.


Image Credit & Copyright: Rolando Ligustri & Lukas Demetz

Rolando's Instagram Page:

https://www.instagram.com/rolandoligustri/

Release Date: June 6, 2024


#NASA #Space #Astronomy #Science #Sun #Earth #Comets #Comet #Comet12PPonsBrooks #SolarSystem #Star #AlphaLeporis #Astrophotography #RolandoLigustri #LukasDemetz #Astrophotographers #CitizenScience #Namibia #Africa #STEM #Education #APoD

Monday, June 10, 2024

Virgin Galactic #07 Spaceflight Recap: Final VSS Unity Mission

Virgin Galactic #07 Spaceflight Recap: Final VSS Unity Mission

Virgin Galactic’s VSS Unity spaceplane conducted its final commercial mission June 8, 2024, taking a Turkish researcher and three private astronauts on a suborbital spaceflight. VSS Unity, attached to its VMS Eve mothership aircraft, took off from Spaceport America in southern New Mexico at 10:31 a.m. Eastern. Unity released from Eve at 11:26 a.m. Eastern, flying its typical suborbital trajectory to an altitude of 87.5 kilometers before gliding to a landing back at the spaceport at 11:41 a.m. Eastern.

Galactic 07 featured a Turkish research astronaut, Tuva Atasever. His flight was arranged through Axiom Space, which flew another Turkish astronaut, Alper Gezeravcı, on the Ax-3 private astronaut mission to the International Space Station in January. Atasever was the backup for that mission.

Atasever planned to conduct seven experiments during the suborbital flight. “The experimental side of the flight was a huge success,” he said at a press conference after the flight. Those experiments included sensors to monitor brain activity, radiation dosimeters and insulin pens designed to operate in microgravity. The brain activity experiment, he noted, included tests to try and capture any changes in brain activity linked to the perspective-altering “Overview Effect” caused by seeing the Earth from space.

He said that testing of the insulin pens, an experiment developed by Axiom Space, during tests in the week leading up to the flight revealed they were not working as expected. “We iterated, we changed a couple of things, and this time around worked perfectly in microgravity.”

The vehicle also carried a rack with automated payloads from Purdue University to study propellant slosh in microgravity and from the University of California Berkeley to test 3D printing. Those payloads were flown through NASA’s Flight Opportunities program.

The other three customers were private astronauts, whose identities were disclosed by Virgin Galactic only after the vehicle landed. They were:

Andy Sadhwani, a principal propulsion engineer at SpaceX who previously did research at NASA and Stanford University;

Irving Pergament, a New York real estate developer and private pilot; and

Giorgio Manenti, an Italian investment manager living in London.

Unity was commanded by Nicola Pecile, making his fourth flight, with Jameel Janjua, on his first spaceflight, as pilot.

This was the seventh commercial flight for VSS Unity and the 12th flight overall. It will also be the last for VSS Unity, the second SpaceShipTwo vehicle built for Virgin Galactic, as the company shifts its focus to completing work on the new Delta series of vehicles.

Learn more at: https://www.virgingalactic.com


Video Credit: Virgin Galactic

Caption Credit: SpaceNews/Jeff Foust

Duration: 2 minutes, 21 seconds

Release Date: Jan. 28, 2024


#NASA #Space #Earth #CommercialSpaceflight #VirginGalactic #SpaceShipTwoVehicle #Galactic07 #VSSUnity #SuborbitalFlight #Astronauts #TuvaAtasever #Türkiye #AndySadhwani #IrvingPergament #GiorgioManenti #HumanSpaceflight #SpaceportAmerica #SpaceTourism #NewMexico #UnitedStates #STEM #Education #HD #Video

NASA’s Boeing Starliner Crew Flight Test: ULA Atlas V Launch Rocket Camera

NASA’s Boeing Starliner Crew Flight Test: ULA Atlas V Launch Rocket Camera


NASA astronauts Butch Wilmore and Suni Williams launched atop a United Launch Alliance Atlas 5 rocket on the Boeing Starliner spacecraft to the International Space Station June 5, 2024, from Cape Canaveral in Florida. Starliner successfully docked with the space station at 1:34 p.m. ET on June 6, 2024.

NASA’s Commercial Crew Program works with the American aerospace industry to provide safe, reliable, and cost-effective transportation to and from the orbital outpost on American-made rockets and spacecraft launching from American soil.

Learn more about NASA’s Commercial Crew Program at: 

https://www.nasa.gov/commercialcrew


ULA Atlas V Rocket info:

https://www.ulalaunch.com/rockets/atlas-v


Video Credit: United Launch Alliance (ULA)

Duration: 6 minutes

Release Date: June 10, 2024


#NASA #Space #Earth #ISS #Boeing #Starliner #CST100 #AtlasVRocket #RocketCam #CommercialCrewProgram #CFT #Astronauts #SuniWilliams #BarryWilmore #HumanSpaceflight #SpaceTechnology #Engineering #LaunchAmerica #NASAKennedy #ULA #SLC41 #CapeCanaveral #Florida #UnitedStates #STEM #Education #HD #Video

James Webb Space Telescope Finds 10 times More Supernovae in Early Universe

James Webb Space Telescope Finds 10 times More Supernovae in Early Universe


NASA’s James Webb Space Telescope is proving to be a fine supernova hunter! With its extreme infrared sensitivity, Webb is finding far-off supernovae almost everywhere it looks. Webb is ideal for identifying extremely distant supernovae because of a phenomenon called cosmological redshift, where light traveling across the universe is stretched into longer wavelengths. Visible light from ancient supernovae is stretched so much that it ends up in the infrared. Webb’s instruments are tuned to see infrared light, making it ideal for finding these distant supernovae. Using data from a deep Webb survey of the early universe, a team has identified 10 times more far-off supernovae than were previously known. This study is the first significant step toward more extensive surveys of ancient supernovae with Webb.

Image Description: JADES Transient Survey (NIRCam Image) | This James Webb Space telescope image showing hundreds of objects of different colors, shapes, and sizes scattered across the black background of space with about 80 objects (many are supernovae) circled in green.

Prior to this survey, only a handful of supernovae had been found above a redshift of 2, corresponding to when the universe was only 3.3 billion years old—just 25% of its current age. This JADES (JWST Advanced Deep Extragalactic Survey) program sample contains many supernovae that exploded even further in the past, when the universe was less than 2 billion years old. It includes the farthest one ever spectroscopically confirmed, at a redshift of 3.6. Its progenitor star exploded when the universe was only 1.8 billion years old.

"Webb is a supernova discovery machine," said Christa DeCoursey, a third-year graduate student at the Steward Observatory and the University of Arizona in Tucson. “The sheer number of detections plus the great distances to these supernovae are the two most exciting outcomes from our survey.”

Previously, researchers used NASA’s Hubble Space Telescope to view supernovae from when the universe was in the "young adult" stage. With JADES, scientists are seeing supernovae when the universe was in its “teens” or “pre-teens.” In the future, they hope to look back to the “toddler” or “infant” phase of the universe.

To discover the supernovae, the team compared multiple images taken up to one year apart and looked for sources that disappeared or appeared in those images. These objects that vary in observed brightness over time are called transients, and supernovae are a type of transient. In all, the JADES Transient Survey Sample team uncovered about 80 supernovae in a patch of sky only about the thickness of a grain of rice held at arm’s length. 

“This is really our first sample of what the high-redshift universe looks like for transient science,” said teammate Justin Pierel, a NASA Einstein Fellow at the Space Telescope Science Institute (STScI) in Baltimore, Maryland. “We are trying to identify whether distant supernovae are fundamentally different from or very much like what we see in the nearby universe.”

Pierel and other STScI researchers provided expert analysis to determine what transients were actually supernovae and which were not, because often they looked very similar.

The team identified a number of high-redshift supernovae, including the farthest one ever spectroscopically confirmed, at a redshift of 3.6. Its progenitor star exploded when the universe was only 1.8 billion years old. It is a so-called core-collapse supernova, an explosion of a massive star.  

Uncovering Distant Type Ia Supernovae

Of particular interest to astrophysicists are Type Ia supernovae. These exploding stars are so predictably bright that they are used to measure far-off cosmic distances and help scientists to calculate the universe's expansion rate. The team identified at least one Type Ia supernova at a redshift of 2.9. The light from this explosion began traveling to us 11.5 billion years ago when the universe was just 2.3 billion years old. The previous distance record for a spectroscopically confirmed Type Ia supernova was a redshift of 1.95, when the universe was 3.4 billion years old.

Scientists are eager to analyze Type Ia supernovae at high redshifts to see if they all have the same intrinsic brightness, regardless of distance. This is critically important, because if their brightness varies with redshift, they would not be reliable markers for measuring the expansion rate of the universe.

Pierel analyzed this Type Ia supernova found at redshift 2.9 to determine if its intrinsic brightness was different than expected. While this is just the first such object, the results indicate no evidence that Type Ia brightness changes with redshift. More data is needed, but for now, Type Ia supernova-based theories about the universe’s expansion rate and its ultimate fate remain intact. Pierel also presented his findings at the 244th meeting of the American Astronomical Society.  

Looking Toward the Future

The early universe was a very different place with extreme environments. Scientists expect to see ancient supernovae that come from stars that contain far fewer heavy chemical elements than stars like our Sun. Comparing these supernovae with those in the local universe will help astrophysicists understand star formation and supernova explosion mechanisms at these early times.

“We’re essentially opening a new window on the transient universe,” said STScI Fellow Matthew Siebert, who is leading the spectroscopic analysis of the JADES supernovae. “Historically, whenever we've done that, we've found extremely exciting things—things that we didn't expect.”

“Because Webb is so sensitive, it's finding supernovae and other transients almost everywhere it’s pointed,” said JADES team member Eiichi Egami, a research professor at the University of Arizona in Tucson. “This is the first significant step toward more extensive surveys of supernovae with Webb.”

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, European Space Agency (ESA) and Canadian Space Agency (CSA).   


Image Credit: NASA, European Space Agency (ESA), Canadian Space Agency (CSA), Space Telescope Science Institute (STScI), JADES Collaboration

Release Date: June 10, 2024


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Planet Mars Auroras during Epic May 2024 Solar Storm | NASA MAVEN Mission

Planet Mars Auroras during Epic May 2024 Solar Storm | NASA MAVEN Mission

The purple color in this video shows auroras on Mars’ nightside as detected by the ultraviolet instrument aboard NASA’s MAVEN orbiter between May 14 and 20, 2024. The brighter the purple, the more auroras that were present. 

Auroras Over Mars: High above NASA's Mars Curiosity rover, NASA’s MAVEN (Mars Atmosphere and Volatile EvolutioN) orbiter captured another effect of the recent solar activity—glowing auroras over the planet. The way these auroras occur is different than those seen on Earth.

Our home planet is shielded from charged particles by a robust magnetic field. It normally limits auroras to regions near the poles. (Solar maximum is the reason behind the recent auroras seen as far south as Alabama.) Mars lost its internally generated magnetic field in the ancient past, so there is no protection from the barrage of energetic particles. When charged particles hit the Martian atmosphere, it results in auroras that engulf the entire planet.

During solar events, the Sun releases a wide range of energetic particles. Only the most energetic can reach the surface to be measured by RAD. Slightly less energetic particles, those that cause auroras, are sensed by MAVEN’s Solar Energetic Particle instrument.

Scientists can use that instrument’s data to rebuild a timeline of each minute as the solar particles screamed past, meticulously teasing apart how the event evolved.

“This was the largest solar energetic particle event that MAVEN has ever seen,” said MAVEN Space Weather Lead, Christina Lee of the University of California, Berkeley’s Space Sciences Laboratory. “There have been several solar events in past weeks, so we were seeing wave after wave of particles hitting Mars.”

The data coming in from NASA’s spacecraft won’t only help future planetary missions to the Red Planet. It is contributing to a wealth of information being gathered by the agency’s other heliophysics missions, including Voyager, Parker Solar Probe, and the forthcoming ESCAPADE (Escape and Plasma Acceleration and Dynamics Explorers) mission.

Targeting a late-2024 launch, ESCAPADE’s twin small satellites will orbit Mars and observe space weather from a unique dual perspective that is more detailed than what MAVEN can currently measure alone.

More About the Missions
MAVEN’s principal investigator is based at the Laboratory for Atmospheric and Space Physics (LASP) at the University of Colorado Boulder. LASP is also responsible for managing science operations and public outreach and communications. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN mission. Lockheed Martin Space built the spacecraft and is responsible for mission operations. NASA’s Jet Propulsion Laboratory in Southern California provides navigation and Deep Space Network support. The MAVEN team is preparing to celebrate the spacecraft’s 10th year at Mars in September 2024.

Similarly, the star camera NASA’s 2001 Mars Odyssey orbiter uses for orientation was inundated with energy from solar particles, momentarily going out. (Odyssey has other ways to orient itself, and recovered the camera within an hour.) Even with the brief lapse in its star camera, the orbiter collected vital data on X-rays, gamma rays, and charged particles using its High-Energy Neutron Detector.

This was not Odyssey’s first brush with a solar flare. In 2003, solar particles from a solar flare that was ultimately estimated to be an X45 fried Odyssey’s radiation detector. Ironically, it was designed to measure such events.

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN mission.

For more information on MAVEN, go to: https://science.nasa.gov/mission/maven/

Video Credit: NASA/University of Colorado/LASP
Duration: 17 seconds
Release Date: June 10, 2024

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NASA's Mars Curiosity Rover Records Major May 2024 Solar Storm | NASA/JPL

NASA's Mars Curiosity Rover Records Major May 2024 Solar Storm | NASA/JPL



In addition to producing auroras, a recent extreme storm provided more detail on how much radiation future astronauts could encounter on the Red Planet.

Mars scientists have been anticipating epic solar storms ever since the Sun entered a period of peak activity earlier this year called solar maximum. Over the past month, NASA’s Mars rovers and orbiters have provided researchers with front-row seats to a series of solar flares and coronal mass ejections that have reached Mars—even causing Martian auroras at times.

This science bonanza has offered an unprecedented opportunity to study how such events unfold in deep space, as well as how much radiation exposure the first astronauts on Mars could encounter.

The biggest event occurred on May 20, 2024, with a solar flare later estimated to be an X12—X-class solar flares are the strongest of several types—based on data from the Solar Orbiter spacecraft, a joint mission between the European Space Agency (ESA) and NASA. The flare sent out X-rays and gamma rays toward the Red Planet, while a subsequent coronal mass ejection launched charged particles. Moving at the speed of light, the X-rays and gamma rays from the flare arrived first, while the charged particles trailed slightly behind, reaching Mars in just tens of minutes.

The unfolding space weather was closely tracked by analysts at the Moon to Mars Space Weather Analysis Office at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. It flagged the possibility of incoming charged particles following the coronal mass ejection.

If astronauts had been standing next to NASA’s Curiosity Mars rover at the time, they would have received a radiation dose of 8,100 micrograys — equivalent to 30 chest X-rays. While not deadly, it was the biggest surge measured by Curiosity’s Radiation Assessment Detector, or RAD, since the rover landed 12 years ago.

RAD’s data will help scientists plan for the highest level of radiation exposure that might be encountered by astronauts. They would need to use the Martian landscape for protection.

“Cliffsides or lava tubes would provide additional shielding for an astronaut from such an event. In Mars orbit or deep space, the dose rate would be significantly more,” said RAD’s principal investigator, Don Hassler of Southwest Research Institute’s Solar System Science and Exploration Division in Boulder, Colorado. “I wouldn’t be surprised if this active region on the Sun continues to erupt, meaning even more solar storms at both Earth and Mars over the coming weeks.”

During the May 20 event, so much energy from the storm struck the surface that black-and-white images from Curiosity’s navigation cameras danced with “snow”—white streaks and specks caused by charged particles hitting the cameras.

NASA’s Jet Propulsion Laboratory in Southern California leads the Curiosity mission.

For more about Curiosity, visit:

http://mars.nasa.gov/msl


Image Credit: NASA/JPL-Caltech 

Release Date: June 10, 2024


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