“An improved appropriation for FY 2025 of $9 billion for SMD will give the agency the necessary resources to pursue Decadal priorities such as the Earth System Observatory, Geophysical Dynamics Constellation, Habitable Worlds Observatory, and Mars Sample Return, while maintaining our nation’s highly-skilled workforce and fleet of operating and developing spacecraft including the Chandra X-Ray Observatory, Hubble Space Telescope, Perseverance and Curiosity rovers, among others. These investments in our high-tech STEM workforce and university systems will provide positive value to every congressional district.”
-Statement in a May 1, 2024 letter to the House Appropriations Subcommittee on Commerce, Justice, Science, and Related Agencies from 44 Members of Congress regarding increased funding to NASA related to its Science Mission Directorate (SMD). The letter notes that “…the FY 2025 President’s Budget Request of $7.6 billion for NASA Science represents a $1.1 billion decrease in purchasing power from its peak in FY 2020 and would be the smallest budget in eight years when adjusted for inflation.”
Image (Credit): The Little Dumbell Nebula as captured by the Hubble Space Telescope. (NASA, ESA, STScI)
This week’s image comes from the NASA/European Space Agency’s Hubble Space Telescope. It shows what is called the Little Dumbbell Nebula, more formally called Messier 76, M76, or NGC 650/651, which is about 3,400 light-years away. The image is being shared as part of the celebration of Hubble’s 34th anniversary, which is discussed in this video.
M76 is classified as a planetary nebula, an expanding shell of glowing gases that were ejected from a dying red giant star. The star eventually collapses to an ultra-dense and hot white dwarf. A planetary nebula is unrelated to planets, but have that name because astronomers in the 1700s using low-power telescopes thought this type of object resembled a planet.
M76 is composed of a ring, seen edge-on as the central bar structure, and two lobes on either opening of the ring. Before the star burned out, it ejected the ring of gas and dust. The ring was probably sculpted by the effects of the star that once had a binary companion star. This sloughed off material created a thick disk of dust and gas along the plane of the companion’s orbit. The hypothetical companion star isn’t seen in the Hubble image, and so it could have been later swallowed by the central star. The disk would be forensic evidence for that stellar cannibalism.
The primary star is collapsing to form a white dwarf. It is one of the hottest stellar remnants known at a scorching 250,000 degrees Fahrenheit, 24 times our Sun’s surface temperature. The sizzling white dwarf can be seen as a pinpoint in the center of the nebula. A star visible in projection beneath it is not part of the nebula.
Pinched off by the disk, two lobes of hot gas are escaping from the top and bottom of the “belt,” along the star’s rotation axis that is perpendicular to the disk. They are being propelled by the hurricane-like outflow of material from the dying star, tearing across space at two million miles per hour. That’s fast enough to travel from Earth to the Moon in a little over seven minutes! This torrential “stellar wind” is plowing into cooler, slower-moving gas that was ejected at an earlier stage in the star’s life, when it was a red giant. Ferocious ultraviolet radiation from the super-hot star is causing the gases to glow. The red color is from nitrogen, and blue is from oxygen.
Given our solar system is 4.6 billion years old, the entire nebula is a flash in the pan by cosmological timekeeping. It will vanish in about 15,000 years.
New research suggests there’s less oxygen on the icy surface of Jupiter’s moon Europa than thought — and that could affect what, if any, life might be lurking in the moon’s underground ocean. Even with little or no oxygen, microbes might still be bustling around in the ocean believed to exist miles beneath Europa’s frozen crust. As for what else, “who knows,” said NASA scientist Kevin Hand, who was not involved in the study published Monday in Nature Astronomy.
The best measurements from Hubble show the universe is now expanding faster than predicted based on observations of how it looked shortly after the big bang. These observations were made by the Planck satellite mapping of the cosmic microwave background radiation – sort of a blueprint for how the universe would evolve structure after it cooled down from the big bang. The simple solution to the dilemma is to say that maybe Hubble observations are wrong due to some creeping inaccuracy in its deep-space yardstick. Then along came the James Webb Space Telescope to crosscheck Hubble’s results. Webb’s sharp infrared views of Cepheids agreed with Hubble data. Webb confirmed that the Hubble telescope’s keen eye was right all along.
A trio of small rovers that will explore the Moon in sync with one another are rolling toward launch. Engineers at NASA’s Jet Propulsion Laboratory in Southern California recently finished assembling the robots, then subjected them to a punishing series of tests to ensure they’ll survive their jarring rocket ride into space and their travels in the unforgiving lunar environment.Part of a technology demonstration called CADRE (Cooperative Autonomous Distributed Robotic Exploration), each solar-powered rover is about the size of a carry-on suitcase.
“This would be the first time that we can directly show through an atmospheric detection, that these planets with water-rich atmospheres can actually exist around other stars…This is an important step toward determining the prevalence and diversity of atmospheres on rocky planets.”
–Statement by Björn Benneke of the Trottier Institute for Research on Exoplanets at Université de Montréal. He was referring to the Hubble space telescope’s detection of water vapor in the atmosphere of exoplanet GJ 9827d. The exoplanet is about twice the Earth’s diameter and approximately 97 light-years from Earth. You can read more about the Hubble discovery here.
Image (Credit): The Hubble Space Telescope’s view of Galaxy UGC 8091. ( ESA/Hubble, NASA Y. Choi (NOIRLab), K. Gilbert (Space Telescope Science Institute), J. Dalcanton (Flatiron Institute and University of Washington))
The image this week is from the NASA/European Space Agency’s (ESA) Hubble Space Telescope. It shows an irregular dwarf galaxy, UGC 8091, that is about seven million light-years away. What I see appears to be jellyfish within some cloudy water. I also the variety of other galaxies you can see throughout the image (see below).
A collection of stars and galaxies fill the scene against a dark background. The image is dominated by a dense collection of stars that make up the irregular galaxy UGC 8091. The stars span a variety of colours, including blue and orange, with patches of blue occupying the central part of the galaxy. There are also visible circular regions of red/pink gas within the galaxy.
Image (Credit): Section of the above image – upper left hand corner. (ESA/Hubble, NASA Y. Choi (NOIRLab), K. Gilbert (Space Telescope Science Institute), J. Dalcanton (Flatiron Institute and University of Washington))
Our Awesome Universe 