NASA Webb, Hubble Scientist Marcia Rieke Awarded Gruber Cosmology Prize

NASA Webb, Hubble Scientist Marcia Rieke Awarded Gruber Cosmology Prize

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

Marcia Rieke, a scientist who worked on NASA’s James Webb Space Telescope and Hubble Space Telescope, has received the Gruber Foundation’s 2024 Cosmology Prize. Rieke will receive the award and gold laureate pin at a ceremony August 8, 2024, at the General Assembly of the International Astronomical Union in Cape Town, South Africa.

Headshot of Marcia Rieke with a background of blurred monitors of scientific data
Marcia Rieke is Regents’ Professor of Astronomy at the University of Arizona and was the principal investigator for the Near-Infrared Camera (NIRCam) on the Webb telescope.
University of Arizona

Rieke was awarded the prize “for her pioneering work on astronomical instrumentation to reveal the breadth and details of the infrared universe. Her contributions to flagship space missions have opened new avenues for understanding the history and mechanisms of star and galaxy formation. She enabled the development and delivery of premier instruments providing groundbreaking sensitivity to near-infrared wavelengths to both the Webb and the Hubble telescopes. Through these substantive contributions along with earlier work, Marcia Rieke has had a lasting impact on our understanding of the universe,” according to the Gruber Foundation’s announcement.

The Cosmology Prize honors a leading cosmologist, astronomer, astrophysicist, or scientific philosopher for theoretical, analytical, conceptual, or observational discoveries leading to fundamental advances in our understanding of the universe. Since 2001, the Cosmology Prize has been cosponsored by the International Astronomical Union. Presented annually, the Cosmology Prize acknowledges and encourages further exploration in a field that shapes the way we perceive and comprehend our universe.

Rieke is Regents’ Professor of Astronomy at the University of Arizona and was the principal investigator for the Near-Infrared Camera (NIRCam) on the Webb telescope.

As principal investigator for the NIRCam, Rieke was responsible for ensuring that the instrument was built and delivered on time and on budget. She worked with the engineers at Lockheed Martin who built NIRCam and helped them decipher and meet the instruments’ requirements.

“As principal investigator of the James Webb Space Telescope NIRCam instrument, Dr. Rieke’s vision, dedication, and leadership were inspirational to the entire team and a key contribution to the success of the Webb telescope,” said Lee Feinberg, Webb telescope manager and optics lead at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. 

Rieke’s research interests include infrared observations of the center of the Milky Way and of other galactic nuclei. She has served as the deputy principal investigator on the Near Infrared Camera and Multi-Object Spectrometer for the Hubble Space Telescope (NICMOS), and the outreach coordinator for NASA’s retired Spitzer Space Telescope.

“As a leading scientist on a premiere Hubble Space Telescope science camera, NICMOS, Dr. Rieke’s expertise enabled ground-breaking discoveries on everything from star formation to distant galaxies,” said Dr. Jennifer Wiseman, Hubble Space Telescope senior project scientist at NASA Goddard. “Subsequent cameras on Hubble, and infrared space telescopes like Spitzer and Webb, have built upon Dr. Rieke’s pioneering work.”

“Dr. Rieke has also poured herself into wide international scientific leadership, leading countless scientific panels that envision and shape the best instruments for future powerful astronomical discovery,” Wiseman said.

“There’s a story beginning to emerge,” Rieke said about the science Webb has returned in the first two years of its mission. “But we still need some more pieces to the story.” For the duration of Webb’s lifetime, many of those pieces will emerge from the instrument that Rieke led.

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, ESA (European Space Agency) and CSA (Canadian Space Agency).

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Rob Gutro
NASA’s Goddard Space Flight Center

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Marty McCoy

On the GOES

On the GOES

NOAA's GOES-U satellite (left) and NASA's Vehicle Assembly Building (right) are both lit up at night. GOES-U is a white cylindrical object and the VAB is a tall, square building.
NASA/Ben Smegelsky

On June 14, 2024, NOAA’s (National Oceanic and Atmospheric Administration) last Geostationary Operational Environmental Satellite, GOES-U, started its journey from the Astrotech Space Operations facility to the SpaceX hangar at Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

GOES-U is the final weather-observing and environmental monitoring satellite in NOAA’s GOES-R Series. GOES-U will enhance meteorologists’ ability to provide advanced weather forecasting and warning capabilities. It also will improve detection and monitoring of space weather hazards using a new compact coronagraph instrument.

Get updates on the GOES blog.

Image Credit: NASA/Ben Smegelsky

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Monika Luabeya

Sols 4222-4224: A Particularly Prickly Power Puzzle

Sols 4222-4224: A Particularly Prickly Power Puzzle

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Sols 4222-4224: A Particularly Prickly Power Puzzle

This image was taken by Mast Camera (Mastcam) onboard NASA’s Mars rover Curiosity on Sol 4219 (2024-06-19 02:22:26 UTC).

Earth planning date: Friday, June 21, 2024

All our patient waiting has been rewarded, as we were greeted with the news that our drill attempt of “Mammoth Lakes 2” was successful! You can see the drill hole in the image above, as well as the first place we attempted just to the left. The actual drilling is only the beginning – we want to see what it is we’ve drilled. We’re starting that process this weekend by using our laser spectrometer (LIBS) to check out the drill hole before delivering some of the drilled material to CheMin (the Chemistry & Mineralogy X-Ray Diffraction instrument) to do its own investigations.

The next step in a drill campaign is usually to continue the analysis with SAM (the Sample Analysis at Mars instrument suite), which tends to be quite power hungry. As a result, we want to make sure we’re going into the next plan with enough power for that. That meant that even though we’ve got a lot of free time this weekend, with three sols and CheMin taking up only the first overnight, we needed to think carefully about how we used that free time. Sometimes, when the science teams deliver our plans, we’re overly optimistic. At times this optimism is rewarded, and we’re allowed to keep the extra science in the plan. Today we needed to strategize a bit more, and the midday science operations working group meeting (or SOWG, as it’s known) turned into a puzzle session, as we figured out what could move around and what we had to put aside for the time being.

An unusual feature of this weekend’s plan was a series of short change-detection observations on “Walker Lake” and “Finch Lake,” targets we’ve looked at in past plans to see wind-driven movement of the Martian sand. These were peppered through the three sols of the plan, to see any changes during the course of a single sol. While these are relatively short observations – only a few minutes – we do have to wake the rover to take them, which eats into our power. Luckily, the science team had considered this, and classified the observations as high, middle, or low priority. This made it easy to take out the ones that were less important, to save a bit of power.

Another power-saving strategy is considering carefully where observations go. A weekend plan almost always includes an “AM ENV Science Block” – dedicated time for morning observations of the environment and atmosphere. Usually, this block goes on the final sol of the plan, but we already had to wake up the morning of the first sol for CheMin to finish up its analysis. This meant we could move the morning ENV block to the first sol, and Curiosity got a bit more time to sleep in, at the end of the plan.

Making changes like these meant not only that we were able to finish up the plan with enough power for Monday’s activities, but we were still able to fit in plenty of remote science. This included a number of mosaics from both Mastcam and ChemCam on past targets such as “Whitebark Pass” and “Quarry Peak.” We also had two new LIBS targets: “Broken Finger Peak” and “Shout of Relief Pass.” Aside from our morning block, ENV was able to sneak in a few more observations: a dust-devil movie, and a line-of-sight and tau to keep an eye on the changing dust levels in the atmosphere.

Written by Alex Innanen, Atmospheric Scientist at York University

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Jun 21, 2024

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NASA’s SLS Rocket: Block 1 vs. Block 1B Configuration

NASA’s SLS Rocket: Block 1 vs. Block 1B Configuration

This infographic labeled “SLS Block 1B Infographic” depicts the SLS (Space Launch System) in the Block 1B configuration that will be used beginning with Artemis 4. The left side of the graphic explains the difference between the Block 1 and Block 1B designs and shows a person standing next to the rocket showing the difference in size. On the top right side of the graphic, there is a graphic depicting the Lunar I-Hab. Below is a breakdown of the internal design of the SLS. It also details a few advantages this configuration of the rocket will have and discusses the capability of having two or more payloads launched by the same rocket.
NASA/Kevin O’Brien

NASA’s SLS (Space Launch System) rocket in the Block 1B cargo configuration will launch for the first time beginning with Artemis IV. This upgraded and more powerful SLS rocket will enable SLS to send over 38 metric tons (83,700 lbs.) to the Moon, including NASA’s Orion spacecraft and its crew, along with heavy payloads for more ambitious missions to deep space. While every SLS rocket retains the core stage, booster, and RS-25 engine designs, the Block 1B features a more powerful exploration upper stage with four RL10 engines for in-space propulsion and a new universal stage adapter for greater cargo capability and volume. 

As NASA and its Artemis partners aim to explore the Moon for scientific discovery and in preparation for future missions to Mars, the evolved Block 1B design of the SLS rocket will be key in launching Artemis astronauts, modules or other exploration spacecraft for long-term exploration, and key components of  Gateway lunar space station.

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Lee Mohon

Hypersonic Technology Project Overview

Hypersonic Technology Project Overview

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A steel model of a hypersonic vehicle and sensor in front of a window in a wind tunnel labeled the 20 inch Mach 6 Tunnel.
A steel model of a hypersonic vehicle and sensor in front of a window in a wind tunnel labeled the 20 inch Mach 6 Tunnel.

Vehicles that travel at hypersonic speeds fly faster than five times the speed of sound. NASA studies the fundamental science of hypersonics to understand it better and applies this understanding to enable point-to-point and space access hypersonic vehicles. These vehicles would use airbreathing engines, which utilize oxygen in the atmosphere. In the long term, NASA envisions reusable hypersonic vehicles with efficient engines for routine flight across the globe.

Vision: Enable routine, reusable, airbreathing hypersonic flight 

Mission: Advance core capabilities and critical technologies underpinning the mastery of hypersonic flight to support U.S. supremacy in hypersonics 

Approach: Conduct fundamental and applied research to enable a broad spectrum of hypersonic systems and missions 

A pointed, narrow airplane flies above the clouds. The sun shines through many, tiny passenger windows.
Artist rendering of a high-speed point-to-point vehicle.
NASA Langley

In the coming decade, NASA envisions the development of enabling technologies for a first-generation reusable airbreathing vehicle capable of cruising at hypersonic speeds. This work supports potential emerging markets in high-speed flight.

By 2050, NASA envisions the development of a next-generation reusable hypersonic vehicle that could serve as the first stage in a two-stage space access vehicle.

Unique Hypersonics Facilities and Expertise

NASA maintains unique facilities, laboratories, and subject matter experts who investigate fundamental and applied research areas to solve the challenges of hypersonic flight. The Hypersonic Technology project coordinates closely with partners in industry, academia, and other government agencies to leverage relevant data sets to validate computational models. These partners also utilize NASA expertise, facilities, and computational tools. Partnerships are critical to advancing the state of the art in hypersonic flight.

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Jun 21, 2024

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Shannon Eichorn