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Summer Heat Hits Southeastern Australia

2026-02-11 05:00

A map of Australia depicts near-surface air temperatures, where most of the country is warm, shown as orange to red. Extreme heat is concentrated over the southeast, and a small cooler blue area appears in Western Australia.
January 29, 2026

While a part of the United States braved extreme winter cold, January 2026 brought sweltering summer conditions to many parts of Australia.

Australia’s area-averaged mean temperature was 1.90 degrees Celsius (3.42 degrees Fahrenheit) above the 1961–1990 average, making it the fourth-warmest January since the start of observations in 1910, according to the Bureau of Meteorology (BoM). Contributing to this was a late-month heatwave in the country’s southeast that was especially intense between January 26 and January 30. During that period, numerous weather stations in South Australia, New South Wales, and Victoria recorded record-high daily temperatures.

The heatwave’s intensity and extent are evident in this map, which shows air temperatures at 03:00 Universal Time (2 p.m. local time in Victoria) on January 29, modeled at 2 meters (6.5 feet) above the ground. It was produced with a version of the GEOS (Goddard Earth Observing System) model, which integrates meteorological observations with mathematical equations that represent physical processes in the atmosphere. The darkest reds are where the model indicates temperatures reaching or exceeding 45°C (113°F).                                                                                                                                                                

According to BoM, the hottest temperatures of January 2026 were measured in two places in South Australia: in the town of Andamooka on the 29th and at the Port Augusta airport on the 30th, where temperatures reached 50.0°C (122.0°F). In both New South Wales and Victoria, the month’s hottest day was on the 27th, when temperatures reached 49.7°C (121.5°F) at a station in Pooncarie and 48.9°C (120.0°F) at stations in Walpeup and Hopetoun.

The heatwave brought significant human and public-health effects, including the increased risk of heat-related illness. Organizers of the Australian Open tennis tournament in Melbourne, Victoria, suspended play on some courts and closed roofs to provide shade as part of an “extreme heat policy” to protect players and spectators, according to news reports.

The recent warmth followed another bout of heat earlier in the month that, combined with strong winds and dry conditions, created dangerous fire conditions. Numerous bushfires were burning across Victoria on January 9 as officials urged people to evacuate. By mid-month, news reports indicated that the fires had destroyed hundreds of structures and killed tens of thousands of livestock.

NASA Earth Observatory image by Lauren Dauphin, using GEOS data from the Global Modeling and Assimilation Office at NASA GSFC. Story by Kathryn Hansen.

References & Resources

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

Extreme January Cold

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Following a significant winter storm, frigid temperatures lingered in late January 2026 across a vast swath of the U.S.

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Summer Heat Lingers in the West

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A prolonged high-pressure weather system brought unusually warm September temperatures to British Columbia and the Pacific Northwest.

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Fires Erupt in South-Central Chile 

2 min read

Tens of thousands of people fled to safety as blazes spread throughout the country’s Biobío and Ñuble regions.

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Curiosity Blog, Sols 4798-4803: Back for More Science

2026-02-10 18:47

2 min read

Curiosity Blog, Sols 4798-4803: Back for More Science

An overhead color photo of the Martian surface shows pale orange-tan, flat, rocky terrain, with the surface a mixture of jagged-edged slabs with fine soil leveling the gaps between them, and small rocks of various sizes scattered around the surface. Near the image center and at lower-right are two drill holes in the rock, each with mounded soil around the opening that had been extracted from the holes during drilling.
NASA’s Mars rover Curiosity acquired this image showing the side-by-side drill holes “Nevado Sajama” (right) and “Nevado Sajama2” (left). Curiosity used its Mast Camera (Mastcam) to capture the image on Jan. 31, 2026 — Sol 4795, or Martian day 4,795 of the Mars Science Laboratory mission — at 22:55:27 UTC.
NASA/JPL-Caltech/MSSS

Written by Michelle Minitti, MAHLI Deputy Principal Investigator

Earth planning date: Friday, Feb. 6, 2026

The results from our first visit to the “Nevado Sajama” drill location were intriguing enough to motivate our return to do a deeper dive into the minerals and compounds locked in this rock with SAM (the Sample Analysis at Mars instrument suite). As explained in the last blog, that deeper dive involves using the second of two vials of a chemical reagent, tetramethylammonium hydroxide (TMAH), that helps makes molecules detectable to SAM that would otherwise be undetectable. This week was focused on completing the many carefully-coordinated steps to apply the TMAH reagent to the rock powder from a drill hole and then analyze the treated sample. As you can see in the image above, we know the drilling necessary to collect the sample was successful, as was delivery of the sample to SAM. We are awaiting word about the first part of the SAM analysis, and are running the second part in the weekend plan. 

As you can imagine, running a mass spectrometer and chemistry experiment remotely on another planet takes a lot of energy, but throughout the week, the team took advantage of whatever spare power there was to include additional science observations. ChemCam planned two attempts at targeting the Nevado Sajama2 drill-hole interior, analyzed “Tiquipaya,” one of the family of rocks broken by the rover wheels that expose bright white material, and measured the chemistry of the atmosphere with a passive sky observation. They also planned an RMI mosaic of layers near the base of the “Mishe Mokwa” butte to our east. MAHLI and APXS paired up to image and analyze the ground-up tailings around the drill hole for the most direct measure of chemistry of what SAM analyzes. As Mastcam acquired a full 360-degree mosaic the first time we were at Nevado Sajama, they did not have many rock observations to plan. Instead, they turned their eyes toward the sky to measure the amount of dust in the atmosphere. Navcam made complementary measurements of atmospheric dust and planned movies and imaging surveys of clouds and dust devils. Ever watchful, RAD and REMS made their regular measurements of the Martian environment while DAN regularly monitored the Martian subsurface. 

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

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Last Updated

Feb 10, 2026

Related Terms

CubeSats’ Missions Begin

2026-02-10 17:03

Two CubeSats, one silver and one with a red face, are ejected from the International Space Station (bottom left) into the blackness of space.
NASA/Chris Williams

NASA astronaut Chris Williams pointed a camera out a window on the cupola as a set of CubeSats were deployed outside the Kibo laboratory module by a small satellite orbital deployer into Earth orbit. Students from Mexico, Italy, ThailandMalaysia, and Japan designed the shoe-boxed satellites for a series of Earth observations and technology demonstrations.

CubeSats are a class of nanosatellites – small spacecraft weighing 1-10 kilograms – that use a standard size and form factor. The development of CubeSats has advanced into its own industry with government, industry and academia collaborating for ever increasing capabilities.  CubeSats now provide a cost-effective platform for science investigations, new technology demonstrations and advanced mission concepts.

Image credit: NASA/Chris Williams

Grants

2026-02-10 16:56

5 Min Read

Grants

The NSSC supports the Agency’s internal effort to create an environment conducive to streamlining and simplifying grants and cooperative agreements. The National Aeronautics and Space Administration (NASA), through the establishment of the NSSC, has transitioned to a consolidated model for the award and administration of all Agency grants and cooperative agreements. The consolidation is designed to achieve efficient and effective service, improve data quality, standardize processes, leverage skills and investments, and provide economies of scale.

Grants Status Requests

To submit a request, visit NASA General Information Request Form and complete the form. You will receive an automated email with the most commonly requested grant status information.

Important Instructions:

  • Ensure you enter a valid email address, as replies will only be sent via email.
  • The confirmation email may take a few minutes to arrive in your inbox.

How to Fill Out the Form:

  1. Category: Select “Procurement including Grants & Cooperative Agreements.”
  2. Procurement Area: Choose “Grants/Agreements.”
  3. Grants/Agreements Activity: Select “Grant Status.”
  4. Required Information: Provide either a Grant Number, Purchase Requisition Number, or both.

Memorandum for NASA Grantee Community

Guidance Regarding OMB Memorandum M-25-14 and Recent Temporary Restraining Orders

Update on Diversity, Equity, Inclusion, and Accessibility (DEIA) Executive Orders – January 29, 2025
On January 23, 2025, NASA’s Office of Procurement (OP) released a memorandum for the NASA contractor and grant community regarding Executive Order “Initial Rescission of Harmful Executive Orders and Actions” and the Office of Personnel Management’s (OPM) memorandum “Initial Guidance Regarding DEIA Executive Orders.”

Per OP’s memo, NASA grant and cooperative agreement recipients shall immediately cease and desist all DEIA activities required for their grant. This work may include but is not limited to: DEIA plan requirements, training, workshops, reporting, considerations for staffing, or any other direct or indirect grant activity related to DEIA. All grant recipients shall notify their cognizant Grant Officer if they identify requirements within their grants that are in violation of this guidance. Your Grant Officer’s contact information can be found on your NF 1687, Notice of Award for Grant and Cooperative Agreement (NOA).

Thank you for your work and partnership with NASA. 

NASA Grant and Cooperative Agreement Terms and Conditions

In FY2025, NASA separated the Terms and Conditions from the GCAM to create a standalone document. This document outlines both the general and specific terms and conditions and applies to all awards issued under 2 CFR 1800 (NASA’s adoption of 2 CFR 200.)
NASA Grant and Cooperative Agreement Terms and Conditions – January 2026

Request for Supplemental Grant and Cooperative Agreement Actions

Administrative Supplement Requests Templates :

 (No-Cost Extensions, Administrative Changes, Prior Approvals)

Submit via email to NSSC-ADMIN-SUPPLEMENT REQUEST

PI Transfer Requests:

Submit via email to NSSC-Grants-PI-Transfer

NASA Insignia Guidelines

Grantees are strongly encouraged to use the NASA Insignia Format identified in the guidelines at NASA Insignia Guidelines for NASA Grantees. These guidelines aim to increase awareness of NASA’s mission activities via Grantee partnerships for a broader and more diverse population.

Payment Management System

NASA uses a service provider, currently the Department of Health and Human Services (HHS) Payment Management System (PMS), to provide Federal funds to recipients. PMS will provide instructions to the recipients for registering and requesting funds through the system.
 

Routine Monitoring

NASA is responsible for routine post-award monitoring on all awards, regardless of the award’s risk determination. At a minimum, routine monitoring includes reviewing award recipients’ annual performance reports, semi-annual Federal Financial Report (FFR), and Transactions Testing Review.

Research Performance Progress Reports

All NASA award recipients must submit annual performance reports. Annual reports are due to NASA 60 days prior to the annual anniversary of the award’s POP start date (e.g., if the POP of an award is October 1 – September 30, the report would be due 60 days prior to October 1.)

  • Final Performance Reports: Submit via email to NSSC-CloseOut@mail.nasa.gov
  • Performance Reports: Submit via email to NSSC-Grant-Report@mail.nasa.gov

Federal Financial Reports (SF-425)

Recipients will submit their semi-annual FFRs in PMS:

Period 1 (October 1 – March 31): Due by April 30 each year.

Period 2 (April 1 – September 30): Due by October 30 of each year.

Final FFRs are due 120 days after the end of the POP

Additional information and training are available on the Payment Management System website at https://pms.psc.gov/. The PMS help desk number is 1-877-614-5533. 

Forms

Post-Award Certifications and Representations

NASA Biographical Sketch Form

Current and Pending Support (CPS) Form

NASA Pre-Award and Post-Award Disclosure Requirements

Regulations and Guidance

Regulations

Electronic Code of Federal Regulations

Guidance

NASA Grant and Cooperative Agreement Manual (GCAM): NASA’s Grant Manual for Proposers and Recipients

The NASA Grant and Cooperative Agreement Manual (GCAM) provides pre and post award policy guidance to NASA proposers and award-managing personnel and award recipients to implement government-wide and NASA-specific regulations for applying for, awarding and administering grants and cooperative agreements with educational and non-profit organizations; State, local, and Indian tribal governments; and for-profit organizations.

NASA Grant and Cooperative Agreement Terms and Conditions

In FY2025, NASA separated the Terms and Conditions from the GCAM to create a standalone document. This document outlines both the general and specific terms and conditions and applies to all awards issued under 2 CFR 1800 (NASA’s adoption of 2 CFR 200.)

Research Terms and Conditions (For Research Awards Issued Prior to October 1, 2024)

NASA implemented the Federal-wide research terms and conditions for all research and research-related grant and cooperative agreement awards issued under 2 CFR 1800 (NASA’s adoption of 2 CFR 200). The Research Terms and Conditions implement the requirements of the Uniform Guidance and includes three companion documents:

RTC Appendix A: Prior Approval Matrix, RTC Appendix B: Subaward Requirements, and RTC Appendix C: National Policy Requirements).

The Research Terms and Conditions and companion documents are accessible on the NSF website.

NASA Office of Inspector General

To file a complaint regarding denial of equal opportunity or discrimination based on race, color, national origin, sex, disability, or age; go to

https://oig.nasa.gov/hotline.html
1-800-424-9183
300 E Street, S.W. Suite 8V39
Washington, DC 20546-0001
NASA OIG Hotline
 http://missionstem.nasa.gov/filing-a-complaint.html​​​​​​​

Resources

Grants.gov
NSSC Grants Payment Package
NASA Research Opportunities Online (NSPIRES)
System for Award Management (SAM)

NASA’s Hubble Captures Light Show Around Rapidly Dying Star

2026-02-10 15:00

4 Min Read

NASA’s Hubble Captures Light Show Around Rapidly Dying Star

In the image center, an opaque oval cloud of gray gas aligned from 1 o’clock to 7 o’clock hides a star. Two strong beams of light from the star emerge from large holes in both sides of the cloud, forming narrow cones extending toward 10 o’clock and 4 o’clock. The central cloud is surrounded by concentric, wispy shells of gas illuminated by the star’s light. The shells reflect extra light where they’re hit by the twin beams. A crowd of smaller stars with cross-shaped spikes over them surrounds the nebula on a black background.

NASA’s Hubble Space Telescope reveals the clearest view yet of the Egg Nebula.

Credits:
NASA, ESA, Bruce Balick (UWashington)

This stunning image from NASA’s Hubble Space Telescope reveals a dramatic interplay of light and shadow in the Egg Nebula, sculpted by freshly ejected stardust. Located approximately 1,000 light-years away in the constellation Cygnus, the Egg Nebula features a central star obscured by a dense cloud of dust — like a “yolk” nestled within a dark, opaque “egg white.” Only Hubble’s sharpness can unveil the intricate details that hint at the processes shaping this enigmatic structure.

It is the first, youngest, and closest pre-planetary nebula ever discovered. (A pre-planetary nebula is a precursor stage of a planetary nebula, which is a structure of gas and dust formed from the ejected layers of a dying, Sun-like star. The term is a misnomer, as planetary nebulae are not related to planets.) 

In the image center, an opaque oval cloud of gray gas aligned from 1 ou2019clock to 7 ou2019clock hides a star. Two strong beams of light from the star emerge from large holes in both sides of the cloud, forming narrow cones extending toward 10 ou2019clock and 4 ou2019clock. The central cloud is surrounded by concentric, wispy shells of gas illuminated by the staru2019s light. The shells reflect extra light where theyu2019re hit by the twin beams. A crowd of smaller stars with cross-shaped spikes over them surrounds the nebula on a black background.
NASA’s Hubble Space Telescope reveals the clearest view yet of the Egg Nebula. This structure of gas and dust was created by a dying, Sun-like star. These newest observations were taken with Hubble’s Wide Field Camera 3.
NASA, ESA, Bruce Balick (UWashington)

The Egg Nebula offers a rare opportunity to test theories of late-stage stellar evolution. At this early phase, the nebula shines by reflecting light from its central star, which escapes through a polar “eye” in the surrounding dust. This light emerges from a dusty disk expelled from the star’s surface just a few hundred years ago.

Twin beams from the dying star illuminate fast-moving polar lobes that pierce a slower, older series of concentric arcs. Their shapes and motions suggest gravitational interactions with one or more hidden companion stars, all buried deep within the thick disk of stardust.

Stars like our Sun shed their outer layers as they exhaust their hydrogen and helium fuel. The exposed core becomes so hot that it ionizes surrounding gas, creating the glowing shells seen in planetary nebulae such as the Helix, Stingray, and Butterfly nebulae. However, the compact Egg Nebula is still in a brief transitional phase — known as the pre-planetary stage — that lasts only a few thousand years. This makes it an ideal time to study the ejection process while the forensic evidence remains fresh.

The symmetrical patterns captured by Hubble are too orderly to result from a violent explosion like a supernova. Instead, the arcs, lobes, and central dust cloud likely stem from a coordinated series of poorly understood sputtering events in the carbon-enriched core of the dying star. Aged stars like these forged and released the dust that eventually seeded future star systems, such as our own solar system, which coalesced into Earth and other rocky planets 4.5 billion years ago.

Hubble has turned its gaze towards the Egg Nebula before. A first visible-light image from the telescope’s WFPC2 (Wide Field and Planetary Camera 2) was complemented in 1997 by a near-infrared NICMOS (Near Infrared Camera and Multi-Object Spectrometer) image, giving a closer look at the light given off by the nebula. In 2003, Hubble’s ACS (Advanced Camera for Surveys) yielded a new view of the Egg, showing the full extent of the ripples of dust around it. A further image from WFC3 (Wide Field Camera 3) in 2012 zoomed in on the central dust cloud and dramatic gas outflows. This new image combines the data used to create the 2012 image with additional observations from the same program to deliver the clearest look yet at this intricate cosmic egg.

The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.


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Details

Last Updated

Feb 10, 2026

Editor
Andrea Gianopoulos
Contact

Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov

Ann Jenkins, Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

TechCrunch - Latest

With co-founders leaving and an IPO looming, Elon Musk turns talk to the moon

2026-02-11 05:23

According to The New York Times, which reports that it heard the meeting, Musk told employees that xAI needs a lunar manufacturing facility, a factory on the moon that will build AI satellites and fling them into space via a giant catapult.
OpenAI policy exec who opposed chatbot’s “adult mode” reportedly fired on discrimination claim

2026-02-11 02:15

The executive has denied the allegation that she engaged in discrimination.
Okay, now exactly half of xAI’s founding team has left the company

2026-02-11 01:50

Whatever the cause of the departures, the cumulative impact is alarming. There is a lot of work left to do at xAI, and an IPO will bring more scrutiny than the lab has ever faced before.
Amazon may launch a marketplace where media sites can sell their content to AI companies

2026-02-10 23:16

A new report claims the e-commerce giant is looking to create a pipeline of licensable content between media publishers and AI companies.
An ice dance duo skated to AI music at the Olympics

2026-02-10 22:31

Czech ice dancers Katerina Mrazkova and Daniel Mrazek are learning the hard way that LLMs sometimes spit out straight-up plagiarism.
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