Pillars of Creation

In 1995, the Hubble Space Telescope released images of the Pillars of Creation — stunning effervescent clouds of interstellar dust and gas, the place where stars are born.


Now, combining data from Hubble and the James Webb Space Telescope, NASA has released a gorgeous 3D visualization of the cosmic structures in both visible and infrared light.


"By flying past and amongst the pillars, viewers experience their three-dimensional structure and see how they look different in the Hubble visible-light view versus the Webb infrared-light view," principal visualization scientist Frank Summers said in a statement.

"The contrast helps them understand why we have more than one space telescope to observe different aspects of the same object," he continue

The Pillars of Creation, which lie about 5,700 light-years from Earth, are composed of cool molecular hydrogen and dust. Due to strong winds and radiation from young nearby hot stars, the pillars are starting to get stripped of their contents. Long, finger-like structures can be seen emerging from the top of the pillars, which are larger than our own solar system.


Inside these structures, hydrogen and dust is gravitationally collapsing into new, infant stars. These new stars will add to the continued dispersion of materials within the pillars. The tallest of the pillars spans 3 light-years from top to bottom — three-quarters of the distance between the sun and our closest star.         READ MORE...

The Problem of an Expanding Universe

A new, precise measurement of the expansion rate of the Universe is in, and it's serving up a huge cosmic pickle.


Using Hubble data and new observations from the James Webb Space Telescope (JWST), a team led by physicist Adam Riess of Johns Hopkins University has confirmed that previous measurements are correct after all, despite years of debate.


Based on immense distances from our Solar System to Cepheid variable stars and Type Ia supernovae, which are used to create a 'cosmic distance ladder', our Universe does indeed appear to be expanding at 73 kilometers per second per megaparsec – a rate known as the Hubble constant.  READ MORE...

NASA Considering Budget Cuts

WASHINGTON — NASA is considering cutting the budget of two of its biggest space telescopes as it faces broader spending reductions for its astrophysics programs.

In an Oct. 13 presentation to the National Academies’ Committee on Astronomy and Astrophysics, Mark Clampin, director of NASA’s astrophysics division, said he was studying unspecified cuts in the operating budgets of the Chandra X-Ray Observatory and Hubble Space Telescope to preserve funding for other priorities in the division.

The potential cuts, he said, are driven by the expectation that his division will not receive the full request of nearly $1.56 billion for fiscal year (FY) 2024 because of legislation passed in June that caps non-defense discretionary spending for 2024 at 2023 levels, with only a 1% increase for 2025.

“We’re working with the expectation that FY24 budgets stay at the ’23 levels,” he said. “That means that we have decided to reduce the budget for missions in extended operations, and that is Chandra and Hubble.”

Clampin declined to say how much the budgets of those two observatories would be cut, or specific impacts on them because of the cuts. He indicated the proposed cuts are still being studied, noting that he was able to make a “positive adjustment” for Chandra just in the last week.

Chandra and Hubble are the two most expensive NASA astrophysics missions to operate after the James Webb Space Telescope. NASA requested $93.3 million for Hubble and $68.7 million for Chandra in its fiscal year 2024 budget proposal, in line with past years’ budgets. Combined, they represent a little more than 10% of the fiscal year 2024 budget request for NASA astrophysics.

They are also among the two oldest NASA missions, with Hubble launched in 1990 and Chandra in 1999. Clampin suggested that was a reason for reducing their budgets. “Chandra has a number of issues right now. It’s becoming increasing difficult to operate,” he said. Insulation on the spacecraft’s exterior is degrading, warming the spacecraft and making operations increasing difficult.

“While Hubble doesn’t have those issues,” he added, “it has been operating for a long time and it is a large piece of the astrophysics budget.”  READ MORE...

Galaxies Newr the Dawn of Time

The small red dot highlighted inside the white box on this James Webb Space Telescope image is an early galaxy, seen as it looked just 350 million years after the Big Bang.       STScI/NASA

New baby pictures of the universe, taken by the James Webb Space Telescope, show that galaxies started forming faster and earlier than expected.

The telescope launched back in December and it now orbits the sun about a million miles away from Earth. Its giant mirror allows it to detect faint light that's been traveling for almost the entire history of the 13.8 billion-year-old universe. That means it can effectively see what galaxies looked like way back in time.

The snapshots captured so far have both thrilled and perplexed scientists, because it turns out that many luminous galaxies existed when the universe was very young.

"Just a few hundred million years after the Big Bang, there are already lots of galaxies," says Tommaso Treu, an astronomer at the University of California at Los Angeles. "JWST has opened up a new frontier, bringing us closer to understanding how it all began."

In research papers published in The Astrophysical Journal Letters, Treu and other astronomers report the discovery of one galaxy that dates back to just 450 million years after the beginning, and another that dates back to 350 million years.  READ MORE...

MIRI Anomoly

James Webb Space Telescope MIRI Spectroscopy Animation: The beam of light coming from the telescope is then shown in deep blue entering the instrument through the pick-off mirror located at the top of the instrument and acting like a periscope.Then, a series of mirrors redirect the light toward the bottom of the instruments where a set of 4 spectroscopic modules are located. Once there, the beam of light is divided by optical elements called dichroics in 4 beams corresponding to different parts of the mid-infrared region. Each beam enters its own integral field unit; these components split and reformat the light from the whole field of view, ready to be dispersed into spectra. This requires the light to be folded, bounced, and split many times, making this probably one of Webb’s most complex light paths.  To finish this amazing voyage, the light of each beam is dispersed by gratings, creating spectra that then projects on 2 MIRI detectors (2 beams per detector). An amazing feat of engineering! Credit: ESA/ATG medialab

Mid-Infrared Instrument Operations Update
The James Webb Space Telescope’s Mid-Infrared Instrument (MIRI) has four observing modes. 

During setup for a science observation on August 24, a mechanism that supports one of these modes, known as medium-resolution spectroscopy (MRS), exhibited what appears to be increased friction. 

This mechanism is a grating wheel that allows astronomers to select between short, medium, and longer wavelengths when making observations using the MRS mode. 

Following preliminary health checks and investigations into the issue, an anomaly review board was convened on September 6 to assess the best path forward.  READ MORE...

Photos of an Alien World

The HIP 65426 b gas giant planet photographed by the James Webb Space Telescope on the 

background of the Digitized Sky Survey (Image credit: NASA/ESA/CSA, A Carter (UCSC), 

the ERS 1386 team, and A. Pagan (STScI))

The James Webb Space Telescope took its first direct image of a planet orbiting a distant star, proving its potential to revolutionize exoplanet research.


The absolute majority of exoplanets have only been observed through temporary dips in brightness of the stars they orbit; only about two dozen have been imaged directly. But that might soon change. Less than two months after it started its science operations, the James Webb Space Telescope has delivered its first direct photo of a planet beyond our solar system.


The planet, a gas giant orbiting the star called HIP 65426 some 385 light-years from Earth, appears in the image as a tiny splotch close to the glowing star. Webb photographed the exoplanet using its Near-Infrared Camera (NIRCam) and the Mid-Infrared Instrument (MIRI), each of which focuses on a different flavor of infrared light.

"This is a transformative moment, not only for Webb but also for astronomy generally," Sasha Hinkley, an astronomer at the University of Exeter in the U.K. who led these observations, said in a statement(opens in new tab).


Scientists had discovered the planet in 2017 with the Very Large Telescope in Chile; Webb isn't tailored to discovering new exoplanets and will instead excel at teaching scientists about worlds other observatories identified.

Exoplanets are extremely difficult to observe directly because they are so much fainter than the stars they orbit. This one, HIP 65426 b, could only be spotted thanks to a combination of factors. First, it's extremely far away from its parent star, 100 times the distance from the sun to Earth (for comparison, Pluto orbits only 40 sun-Earth distances from the sun). Second, HIP 65426 b is also extremely massive — 12 times the size of Jupiter, the solar system's largest planet.  READ MORE...

Phantom Galarxy Looks Like A Wormhole

The James Webb Space Telescope's imagery of NGC 628 (the "Phantom Galaxy") shows glowing 

dust in this citizen science image. (Image credit: NASA/ESA/CSA/Judy Schmidt)

A fresh image based on brand-new deep-space data appears to show a wormhole spinning before our very eyes.

The appropriately named "Phantom Galaxy" glows eerily in a new image by Judy Schmidt based on James Webb Space Telescope data collected nearly a million miles away from our planet using the observatory's mid-infrared instrument (MIRI).

"I've been doing this for 10 years now, and [Webb] data is new, different, and exciting," Schmidt told Space.com. "Of course I'm going to make something with it."

The image highlights the dust lanes in the galaxy, which is more properly known as NGC 628 or Messier 74. Dubbed the "perfect spiral" by some astronomers because the galaxy is so symmetrical, the Phantom Galaxy is scientifically interesting because of the intermediate-mass black hole scientists believe is embedded at its heart.

The galaxy has been imaged professionally many times before, including by space observatories such as the Hubble Space Telescope and the Wide-field Infrared Survey Explorer (WISE). 

What makes Webb imagery stand apart from these past efforts is the mid-infrared range that highlights cosmic dust, along with the power of its unique 18-segment hexagonal mirror and deep-space location.

Webb observed M74 earlier this week. The data was also shared on Twitter(opens in new tab) (with different filtration) by Gabriel Brammer, an astronomer at the Cosmic Dawn Center in the Niels Bohr Institute at the University of Denmark.  READ MORE...

Watching Space in High Definition

This artist’s view shows a planet orbiting the young star Beta Pictoris. 

(Image credit: ESO L. Calçada/N. Risinger)

Researchers are looking forward to a glimpse of colliding worlds in action from NASA's cutting-edge space observatory.

After the James Webb Space Telescope finishes its commissioning period and releases its first operational images on July 12, the observatory will dive into science in earnest. And one of the telescope's first-year investigations will include a close-up view of the strange neighborhood of Beta Pictoris.

The young star, just 63 light years away from us, is surrounded by a dusty disc full of debris left over from its formation. It's a crowded space, hosting "at least two planets [and] a jumble of smaller, rocky bodies," researchers said in a 2021 press release(opens in new tab) about the investigation.

While the research has numerous directions, one key aspect is watching a young planetary system evolving as planetesimals (the predecessors to planets) collide. Because Beta Pictoris is wreathed in dust, researchers will be using Webb's infrared light to peer through the debris and see what is happening in high definition.

Webb will have decades of past work to draw upon, including ground-based observatories and space observations from the Hubble Space Telescope. We know from such studies that Beta Pictoris hosts at least two gigantic planets, both much more massive than Jupiter. Researchers also glimpsed the first known exocomets, or comets beyond our solar system, whirling in the debris cloud.  READ MORE...

5,000 Worlds Outside

In January 1992, two cosmic objects forever changed our galaxy.

For the first time, we had concrete evidence of extrasolar planets, or exoplanets, orbiting an alien star: two rocky worlds, whirling around a star 2,300 light-years away.

Now, just over 30 years later, that number has exploded. This week, March 21 marked the hugely significant milestone of over 5,000 exoplanets confirmed. To be precise, 5,005 exoplanets are now documented in the NASA exoplanet archive, every one with its own unique characteristics.

Each and every one of these exoplanets has appeared in peer-reviewed research, and been observed using multiple detection techniques or methods of analysis.

The pickings are rich for follow-up study to learn more about these worlds with new instruments, such as the recently launched James Webb Space Telescope, and upcoming Nancy Grace Roman Space Telescope.

"It's not just a number," says astronomer Jessie Christiansen of the NASA Exoplanet Science Institute at Caltech. "Each one of them is a new world, a brand-new planet. I get excited about every one because we don't know anything about them."  READ MORE...