Progress Cargo Craft Headed to Station Following Successful Launch

Progress Cargo Craft Headed to Station Following Successful Launch

The Progress 89 cargo craft launches from the Baikonur Cosmodrome in Kazakhstan at 11:20 p.m. EDT Wednesday, Aug. 14. Credit: NASA TV
The Progress 89 cargo craft launches to the space station from the Baikonur Cosmodrome in Kazakhstan at 11:20 p.m. EDT Wednesday, Aug. 14. Credit: NASA TV

The unpiloted Roscosmos Progress 89 spacecraft is headed for the International Space Station following a launch at 11:20 p.m. EDT Wednesday, Aug. 14 (8:20 a.m. Baikonur time, Thursday, Aug. 15), on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan.

After a two-day in-orbit journey to the station, the spacecraft will automatically dock to the aft port of the orbiting laboratory’s Zvezda Service module at 1:56 a.m., Saturday, Aug. 17.

NASA’s coverage of rendezvous and docking will begin at 1 a.m. on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA+ through a variety of platforms including social media.

The spacecraft will deliver about three tons of food, fuel, and supplies to the space station.


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

Get weekly updates from NASA Johnson Space Center at: https://roundupreads.jsc.nasa.gov/

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Abby Graf

Live NASA Coverage Underway of Progress Cargo Craft Launch

Live NASA Coverage Underway of Progress Cargo Craft Launch

The Progress 86 cargo craft is pictured approaching the space station's Poisk module on Dec. 3, 2023.
The Progress 86 cargo craft is pictured approaching the space station’s Poisk module on Dec. 3, 2023.

NASA’s live launch coverage is underway on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA+ through a variety of platforms including social media.

The unpiloted Progress 89 spacecraft is scheduled to launch at 11:20 p.m. EDT Wednesday, Aug. 14 (8:20 a.m. Baikonur time, Thursday, Aug. 15), on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan. The Roscosmos spacecraft will liftoff carrying about three tons of food, fuel, and supplies for the Expedition 71 crew aboard the International Space Station.

After a two-day in-orbit journey to the station, the spacecraft will automatically dock to the aft port of the orbiting laboratory’s Zvezda Service module at 1:56 a.m., Saturday, Aug. 17. NASA’s coverage of rendezvous and docking will begin at 1 a.m. on NASA+, NASA Television, the NASA app, YouTube, and the agency’s website.


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

Get weekly updates from NASA Johnson Space Center at: https://roundupreads.jsc.nasa.gov/

Get the latest from NASA delivered every week. Subscribe here: www.nasa.gov/subscribe

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Abby Graf

Sols 4275-4276: A Familiar View

Sols 4275-4276: A Familiar View

2 min read

Sols 4275-4276: A Familiar View

A grayscale photograph of the Martian surface shows rough, rocky terrain in the foreground and rolling hills and smooth dunes in the background.
NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on sol 4272 — Martian day 4,272 of the Mars Science Laboratory mission – on Aug. 12, 2024 at 12:06:27 UTC.
NASA/JPL-Caltech

Earth planning date: Wednesday, Aug. 14, 2024

The star of today’s plan is SAM’s GCMS, which continues our analysis of the “Kings Canyon” drill sample. As Natalie mentioned, this is a relatively energy-hungry activity, but luckily our last plan left us in a good position to not only complete the GCMS experiment but also fit in some other science around it. Having spent a good deal of time in this location for our drill campaign, we’re getting really familiar with this area in a way we don’t get the opportunity to when we’re driving more often. This means lots of geology targets both near and far — a collection to which we’re adding in today’s plan. Nearby, we have two targets for ChemCam’s laser spectrometer, “Meysan Lake” and “Washburn Lake.” Further afield, ChemCam has long-distance mosaics of “Milestone Peak” and our constant companion for many sols, the Kukenan Butte. Mastcam will also be getting a mosaic of the Wilkerson Butte.

While the atmosphere is always with us, staying in one spot can also grant us good opportunities for keeping an eye on the current environment. We currently have a great view of a nearby sand patch, which you can see in the image above, and we’ve been taking full advantage with lots of dust devil movies, including one in today’s plan. We can also look out for wind-driven movement closer to home, which we’re doing with a Mastcam observation of the drill hole tailings and a Navcam observation of the dust that’s accumulated on the rover deck.

It’s not just near-surface dust we want to keep an eye on, though. The amount of dust suspended in the atmosphere varies throughout the year, and we’re continuing to keep track of that with regular tau observations. The optical depth, which is usually denoted by the Greek letter tau (hence our observation’s name), is a measure of how opaque or transparent the atmosphere is. At this time of year, in the midst of the dusty season, there tends to be more dust suspended in the atmosphere, meaning we cannot see quite as far, and we say the optical depth, or tau, is higher.  

Written by Alex Innanen, Atmospheric Scientist at York University

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Aug 14, 2024

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Sols 4273-4274: Prep Rally

Sols 4273-4274: Prep Rally

2 min read

Sols 4273-4274: Prep Rally

A close-up, overhead photo of a part of the Curiosity rover shows an enclosure that looks like a backwards “C.” Inside that is a circular, silver metal opening that looks like the wall of a springform cake pan, and inside that is a round opening that looks like a metal duct pipe, the inside of which is dark and you can’t see the bottom. The metal parts appear shiny and clean, but everything else in the image appears covered in brownish-orange dust.
This image from NASA’s Mars rover Curiosity shows the open inlet No. 2 on the rover’s SAM (Sample Analysis at Mars) instrument suite, where Curiosity delivered a sample from the “Kings Canyon” drill hole, for study using SAM’s Evolved Gas Analysis (EGA) mode. This image was taken by Mastcam Right (Mast Camera) aboard Curiosity on sol 4270 — Martian day 4,270 of the Mars Science Laboratory mission — on Aug. 10, 2024 (at 14:16:21 UTC).
NASA/JPL-Caltech/MSSS

Earth planning date: Monday, Aug. 12, 2024

The SAM EGA over the weekend was successful, and that means we’re well on our way to planning the GCMS (Gas Chromatograph Mass Spectrometry) on our “Kings Canyon” drill sample! GCMS is an energy-intensive activity, so we’ll be using today’s two-sol plan mainly for recharging our battery and prepping SAM by cleaning its GC column with high temperatures (like you’d clean your own oven!). We can still afford about 75 minutes of remote sensing over both sols this plan and are using it for our usual ChemCam, Mastcam, and Navcam activities.

On the first sol, ChemCam is kicking things off with a LIBS (Laser Induced Breakdown Spectrometer) on “The Major General” — some crunchy light-toned bedrock about 9 feet away (about 2.8 meters) — then will capture a long-distance 10-frame RMI of the Gediz Vallis channel floor to the south. Mastcam finishes off the first sol’s 72-minute science block with an M100 image of The Major General LIBS spots and a 68-frame stereo mosaic of the midfield terrain to fill in what’s left of the midfield with M100. We’ll nap until about 15:15 local Mars time, when we’ll wake back up to take just two M100 images near the RSM hardstop at the same timing as a previous mosaic to make sure we have continuous coverage across the hardstop. SAM’s GC column clean is planned between 21:00 and 01:00; overnight between our two sols.

On the second sol, we’ll have our second remote sensing block around 11:00 for 73 minutes. ChemCam is planning a second LIBS target on “Dewey Point” — a slab of light-toned bedrock about 13 feet away (about 3.9 meters) — a passive-spectrum observation of a dark float block named “Waller Minaret,” and another long-distance four-frame RMI of southern Kukenan butte to the southeast. Mastcam has just a single M100 image of Dewey Point’s LIBS spots this sol so that Navcam can complete some environmental movies to hopefully capture some dust devils and maybe even some clouds!

Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems

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Aug 14, 2024

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Wildland Fire Management Initiative Description

Wildland Fire Management Initiative Description

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A fire burns in Fishlake National Forest, as part of the Fall 2023 FASMEE prescribed burn. Grace Weikert / Goddard
A fire burns in Fishlake National Forest, as part of the Fall 2023 FASMEE prescribed burn.
NASA/ Grace Weikert

Background

Fire is a natural occurrence in many ecosystems and can promote ecological health. However, wildfires are growing in scope and occurring more often than in the past. Among other causes this is due to human-caused climate impacts and the expansion of communities into areas with wildland vegetation. These blazes continue to significantly harm communities, public health, and natural ecosystems. NASA is leveraging cutting-edge science and technology to better understand wildland fire behavior and provide valuable tools for fire policy, response, and mitigation. 

NASA’s Stake in Wildfire

NASA’s contributions to wildland fire management span decades. This includes research to better understand the role fire plays in Earth’s dynamic atmosphere, and airborne and spaceborne sensors to analyze fire lifecycles. Much of this research and technology is still used by wildfire agencies across the globe today. NASA is building on this research and technology development with the Wildland Fire Management Initiative (WMI).  

WMI leverages expertise across the Agency in space technology, science, and aeronautics to improve wildfire research and response. Through this effort, NASA and its partners will continue to provide tools and technologies for improved predictive fire modeling, risk assessment, fire prevention, suppression and post-fire recovery operations. NASA’s WMI aims to equip responders with improved tools for managing these fires

How NASA is Tackling Wildfire

NASA is collaborating with other government agencies, academia, and commercial industries to build a concept of operations for the future of wildland fire management. This means identifying gaps in current wildland fire technologies and procedures and laying out clear solutions to address those challenges.  

NASA will perform a demonstration of wildland fire technologies – including X – in the coming years. 

To provide a well-rounded toolkit for improving wildland operations, NASA and is tackling every aspect of wildland fire response. These efforts include: 

Pre-Fire 

  • Fuel fire maps with improved accuracy  
  • Tools that identify where and when safe, preventative burn treatments would be most effective 
  • Airspace management and safety technologies to enable mainstream use of uncrewed aircraft systems in prescribed burns 

Active Fire 

  • Fire detection and tracking imagery  
  • Improved fire information management systems 
  • Models for changing fire conditions, including fire behavior, and wind and atmospheric tracking for quality forecasts 
  • Uncrewed aircraft and high-altitude balloons for real-time communications for fighting fires in harsh environments 
  • Uncrewed Aircraft Systems Traffic Management (UTM) to expand use of uncrewed aircraft systems in fire response, particularly in environments where traditional air traffic control technologies aren’t available 
  • An airspace awareness and communications system to enable remotely piloted aircraft to identify, monitor, and suppress wildfires 24 hours a day 

Post-Fire 

  • Improved fire impact assessments, including fire severity, air and water quality, risks of landslides, debris flows, and burn scars 
  • Ground-based, airborne, and spaceborne observations to develop monitoring systems for air quality and map burn severity and develop and enhance models and predictions of post-fire hazards 

NASA’s Disasters Response Coordination System (DRCS) supports all three fire response aspects listed above. The DRCS, developed under the Agency’s Earth Science Division’s Disasters Program, provides decisional support to international and domestic operational response agencies. This support includes products for understanding wildfire movement and potential pathways, burn-area maps, and impacts of fire, ash, and smoke to population and critical infrastructure. DCRS tools also provide assessments of post-fire flooding and debris flow susceptibility. 

NASA’s Investment in New Wildland Fire Technologies  

NASA’s WMI offers grants, contracts, and prizes to small businesses, research institutions, and other wildland technology innovators. Some related technology development activities underway include: 

  • Testing communications technologies for incident response teams in areas with no cellphone coverage via a high-altitude balloon 60,000 feet above ground level 
  • Developing wildfire detection systems and instruments for crewed and uncrewed aircraft  
  • Funding early-stage technology development for remote sensing instruments and sensor systems 
  • Developing and flight testing integrated, compact systems for small spacecraft and other platforms for autonomous detection, location tracking, and data collection of transient smoke plumes, early wildfires and other events 
  • Licensing technologies relevant to wildland fire management and hosting wildland fire webinars to promote NASA technology licensing 

Partners 

The NASA Wildland Fire Management Initiative team collaborates with industry, academia, philanthropic institutions, and other government agencies for a more fire-resilient future. These include:  

  • U.S. Forest Service 
  • The California Department of Forestry and Fire Protection 
  • The National Oceanic and Atmospheric Administration 
  • The Federal Aviation Administration 
  • The Department of Homeland Security 
  • The Department of Defense 
  • The National Wildfire Coordinating Group 

WMI Deliverables

Through these combined efforts, NASA aims to address urgent wildland fire management challenges and ensure communities are better prepared for wildland fires. NASA will continue to expand partnerships within wildland fire management agencies for technology development and adoptions. 

For more information, email: Agency-WildlandFiresInitiative@mail.nasa.gov 

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Hillary Smith