Pic of the Week: The Crystal Ball Nebula

Posted on by onespaceman2000
Image (Credit): An image of NGC 1514, also called the Crystal Ball Nebula, as captured by the Gemini North telescope in Hawaii. (International Gemini Observatory/NOIRLab/NSF/AURA)

This week’s image is from the Gemini North telescope located on the summit of Maunakea in Hawaii. NGC 1514, or the Crystal Ball Nebula, is about 1,500 light-years away. It was first discovered in 1790 by German–British astronomer William Herschel, who classified it as a planetary nebula.

Here is a little more about the nebula from NOIRLab:

Planetary nebulae form when a low- or intermediate-mass star ejects its outer layers near the end of its life, forming a somewhat spherical cloud of gas. They typically have smoother, spherical shapes, making the Crystal Ball Nebula unique for its bumpy shells of gas. As the central star casts away this gas, its inner core is exposed. Radiation from the core energizes the gas, giving it a scorching temperature and chromatic glow…While it may appear in this image as if there is a single shining light source at the heart of the Crystal Ball Nebula, as Herschel saw, it actually contains two stars. These two stars orbit each other with a period of around nine years — the longest known for any binary pair within a planetary nebula. Scientists believe that one of these stars, which was once several times more massive than our Sun, released its outer layers while in the throes of death. As the progenitor star and its binary companion orbit each other, they mold the expanding shell of gas with their strong, asymmetrical winds, forming the lumpy layers we see today.

Pic of the Week: Crescent Mars

Posted on by onespaceman2000
Image (Credit): Mars as captured on May 15, 2026 by NASA’s Psyche mission as it approached the planet for a gravity assist. (NASA/JPL-Caltech/ASU)

This week’s image comes from the Psyche spacecraft that is utilizing Martian gravity for its flight plan on its way to the asteroid Psyche in the asteroid belt. This image of a crescent Mars is one of many drive-by photos for both science and our enjoyment.

Here is more on this Martian part of the mission from NASA:

Because Psyche approached Mars from a high phase angle, the planet appeared as a thin crescent in the days running up to the close approach, lit by sunlight reflecting off its surface. In observations from the spacecraft’s multispectral imager, the crescent appeared brighter and extended farther around the planet’s disk than anticipated because of the strong scattering of sunlight through the planet’s dusty atmosphere. As Psyche passed from Mars’ nighttime skies to daytime, it took a rapid series of pictures of the surface around the time of closest approach.

“We’ve captured thousands of images of the approach to Mars and of the planet’s surface and atmosphere at close approach. This dataset provides unique and important opportunities for us to calibrate and characterize the performance of the cameras, as well as test the early versions of our image processing tools being developed for use at the asteroid Psyche,” said Jim Bell, the Psyche imager instrument lead at Arizona State University (ASU) in Tempe. “As the spacecraft continues its journey after the flyby, we’ll continue calibration imaging of Mars for the rest of the month as it recedes into the distance.”

Pic of the Week: Spiral Arm of Galaxy M51

Posted on by onespaceman2000
Image (Credit): View of an arm of the Messier 51 galaxy from both JWST and the Hubble Space Telescop. (ESA/Webb, NASA & CSA, A. Pedrini, A. Adamo (Stockholm University) and the FEAST JWST team)

This week’s image is from the James Webb Space Telescope (JWST) and Hubble Space Telescope, which together scanned about 9,000 star clusters in the four galaxies. What you are looking at above comes from the spiral arm of one of the galaxies – Messier 51 (M51).

Here is a description from the European Space Agency (ESA) regarding what you are seeing in the image:

A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.

Pic of the Week: Spiral Galaxy NGC 3137

Posted on by onespaceman2000
Image (Credit): Hubble Space Telescope image of NGC 3137, located 53 million light-years away. (ESA/Hubble & NASA, D. Thilker and the PHANGS-HST Team

This week’s image is from the Hubble Space Telescope. It shows spiral galaxy NGC 3137 in all its glory. We are getting a nice inclined view of the galaxy, allowing us to see multiple arms of stars.

The European Space Agency (ESA) describes what we are seeing in this way:

A spiral galaxy seen close up and tilted at an angle, so that its disc fills the view from corner to corner. Its disc is yellow near to the centre and pale blue farther out, showing cooler and hotter stars, respectively. Thin brown clouds of dust, glowing pink spots of star formation, and sparkling blue patches filled with star clusters swirl through the galaxy. Behind it, small orange dots are very distant galaxies.

Pic of the Week: Hubble and the Crab Nebula

Posted on by onespaceman2000
Image (Credit): A 2024 image of the Crab Nebula captured by NASA’s Hubble Space Telescope. (NASA, ESA, STScI, William Blair (JHU); Image Processing: Joseph DePasquale (STScI))

This week’s image is from the Hubble Space Telescope. It is an image of the Crab Nebula taken 25 years after the Hubble’s first image of the nebula. If you want to learn more about this history, a paper titled The Crab Nebula Revisited Using HST/WFC3 can be found in The Astrophysical Journal.

Here is a little more from NASA on earlier sightings of the nebula:

This new Hubble observation continues a legacy that stretches back nearly 1,000 years, when astronomers in 1054 recorded the supernova as an impressively bright new star that, for weeks, was visible even during the day. The Crab Nebula is the aftermath of SN 1054, located 6,500 light-years from Earth in the constellation Taurus…

The supernova remnant was discovered in the mid-18th century, and in the 1950s Edwin Hubble was among several astronomers who noted the close correlation between Chinese astronomical records of a supernova and the position of the Crab Nebula. The discovery that the heart of the Crab contained a pulsar — a rapidly rotating neutron star — that was powering the nebula’s expansion finally aligned modern observations and ancient records.