Saturday, 4 July 2026

NASA’s Hubble Spies Stellar Sparkler for July 4th

3 min read

NASA’s Hubble Spies Stellar Sparkler for July 4th

Hubble image of NGC 6426, a compact grouping of a multitude of stars shine in red, white and blue against the dark background of space. The stars are more densely collected toward the center of the cluster.
Ancient stars shine in red, white and blue from a globular cluster almost as old as the universe itself in this image from NASA’s Hubble Space Telescope.
NASA, ESA, and A. Dotter (Dartmouth College); Processing: Gladys Kober (NASA/Catholic University of America)

Red, white, and blue stars glitter like a sparkler being waved on a dark night in this new image from NASA’s Hubble Space Telescope. NASA released this image to celebrate the United States’ 250th anniversary, as the agency carries forward America’s legacy of exploration.

Located in the outer halo of our Milky Way galaxy, globular cluster NGC 6426 is a spherical collection of stars bound together by their mutual gravity, one of 150 known globular clusters in our galaxy. These groups of stars are thought to form as a unit from the same collapsing cloud of gas, and thus the stars in them typically have similar ages. The stars in globular clusters tend to be ancient. At approximately 13 billion years old, NGC 6426 is one of the Milky Way’s oldest globular clusters and almost as old as the universe itself (13.7 billion years).

In this image, blue indicates the shorter wavelengths that are visible light, while red depicts the longer wavelengths of visible light, as well as some near-infrared light. Colors in Hubble images are chosen based on standard image processing techniques to best represent the wavelengths of light that pass through the filters used in the observation. Because the color and temperature of stars are directly related, we know that the blue stars in this image are hotter and the red stars are cooler.

The stars of NGC 6426 have low metallicity, which means they have fewer elements that are heavier than hydrogen and helium. These conditions resemble those of the early universe, when matter was mostly helium and hydrogen and heavier elements were just beginning to form via nuclear fusion within massive stars.

Researchers have found evidence for two chemically distinct populations of stars in NGC 6426, indicating that the slightly younger and more metallic stars were enriched with material from the explosive deaths of the cluster’s earlier stars. Massive stars that explode as supernovae fling elements heavier than hydrogen and helium into the universe, seeding it with materials to build new stars and planets.

Hubble took this image as part of a study of globular clusters in the Milky Way’s halo intended to determine their ages and shed light on the formation and evolution of the galaxy. Over the past three decades in orbit, Hubble has fundamentally changed our understanding of the universe. Its discoveries are expanded upon and complemented by observations from other NASA missions like the infrared-detecting James Webb Space Telescope and the Nancy Grace Roman Space Telescope, scheduled to launch in late summer.

Explore More


Hubble’s Star Clusters


Exploring the Birth of Stars


Hubble’s Nebulae

Media Contact:

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



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Friday, 3 July 2026

NASA’s Hubble Captures Crimson Cloud Sparkling with White, Blue Stars

3 min read

NASA’s Hubble Captures Crimson Cloud Sparkling with White, Blue Stars

A Hubble image of blue and white stars are sprinkled throughout a landscape of red clouds of gas and dark, swirling lanes of dust. Many additional stars are visible in the dark background of space.
A glowing landscape of gas and dust revealed by NASA’s Hubble Space Telescope is heated and illuminated by a thriving population of young stars in the LH 95 region of the Large Magellanic Cloud.
NASA, ESA, and N. Da Rio (The University of Virginia), G. De Marchi (European Space Agency – ESTEC), and D. Gouliermis (Universitat Heidelberg); Processing: Gladys Kober (NASA/Catholic University of America)

Like fresh fireworks launched against a background of dissipating smoke, blue and white stars shine brilliantly against a crimson background of glowing gas in this image of stellar nursery LH 95 from NASA’s Hubble Space Telescope.

LH 95 is a region in the Large Magellanic Cloud, a dwarf galaxy that orbits the Milky Way. Low-mass infant stars live alongside massive blue giant stars in what is known as a stellar association, one of many in the Large Magellanic Cloud.

The LH 95 region’s most massive stars, possessing at least three times the mass of the Sun and visible here as the largest and brightest blue stars, expel ultraviolet radiation and stellar winds that both heat and shape the surrounding hydrogen gas. Dark filaments stand out in sharp contrast against the glowing hydrogen where denser dust lanes resist erosion.

In this image, blue indicates the shorter wavelengths that are visible light, while red depicts the longer wavelengths of visible light, as well as some near-infrared light. Colors in Hubble images are chosen based on standard image processing techniques to best represent the wavelengths of light that pass through the filters used in the observation. The gas of the nebula glows crimson due to hydrogen-alpha emissions.

Hydrogen-alpha is an excellent indicator of star formation, allowing astronomers to identify very young stars embedded in this glowing gas. Researchers found developing stars still gathering material from the disks of gas and dust around them. In fact, LH 95 is home to an extraordinary 2,500 stars that have accumulated almost all of their critical mass but have not yet “turned on” by beginning fusion reactions. These stars, called “pre-main-sequence stars,” have formed from collapsing clouds of gas and are still contracting. They will soon begin burning hydrogen in their cores to become full stars.

By studying these forming stars, researchers confirmed that the stars’ accretion rate ― the rate at which they accumulate matter ― decreased with age, as expected. However, they also learned that accretion can persist for several million years, longer than sometimes assumed. This information helps refine our understanding of how young stars keep growing and how their disks evolve.

Researchers noted that distinct generations of stars in LH 95 exist side-by-side, indicating that rather than forming stars in a single event, the region produces multiple stellar generations over an extended period.

The most massive star in LH 95 (above center, slightly left) has about 60-70 times the mass of the Sun and is about a million years younger than the rest of stars in the system, which appear to be around 4 million years old. Massive stars like these burn through their fuel quickly and die in supernova explosions.

With its rich stellar population, LH 95 is valued by astronomers for providing a way to observe forming stars at relatively close range in an environment with less obscuring dust than similar regions of the Milky Way.

As one of NASA’s flagship observatories, Hubble has produced a wealth of scientific discoveries over more than 30 years in orbit. Its observations are expanded upon and enhanced by observations with other NASA missions, including the infrared-detecting Webb Space Telescope and the upcoming Nancy Grace Roman Space Telescope, which is scheduled to launch in late summer.

Explore More


Hubble’s Nebulae


Exploring the Birth of Stars


Hubble’s Star Clusters

Media Contact:

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



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NASA’s Hubble Spots Star-Spangled Cosmic Scene

3 min read

NASA’s Hubble Spots Star-Spangled Cosmic Scene

A packed, roughly spherical cluster of red, white and blue stars shines against the black background of space. The stars are clustered most densely toward the center of the cluster.
This image from NASA’s Hubble Space Telescope shows Messier 3, a densely packed cluster of stars whose origins may be a merger between globular clusters in the early universe.
NASA, ESA, and A. Sarajedini (Florida Atlantic University); Processing: Gladys Kober (NASA/Catholic University of America)

More than 500,000 stars blaze red, white, and blue in this image from NASA’s Hubble Space Telescope, released in celebration of the United States’ 250th anniversary. The image showcases Messier 3 (M3), one of the Milky Way galaxy’s most massive globular clusters, or spherical collections of gravitationally bound stars. Globular clusters are made up of ancient stars that formed at roughly the same time from the same cloud of gas, giving those stars similar ages. Around 150 known globular clusters are sprinkled around the outer regions of the Milky Way.

In addition to its significant mass, M3 is unusual because it lies relatively far from the galactic center and has more than 240 RR Lyrae variable stars, the most of any globular cluster in our galaxy. RR Lyrae variables are some of the galaxy’s oldest stars and are of special interest to astronomers, due to their age and because their light fluctuates over time in a way that tells us their intrinsic brightness. This true brightness can be used to measure distances in the cosmos, just as knowing the brightness of car headlights on a dark road can help estimate the distance to an oncoming vehicle.

The M3 globular cluster also contains around 70 identified “blue straggler” candidates, which are stars that shine with a bright, blue light that makes them look like younger stars than the typical, redder residents of globular clusters. This was the first cluster in which these oddball stars were located. These stars are thought to have gravitationally pulled mass from companion stars, rejuvenating them and making them appear bluer and younger despite their true age.

The unusual characteristics of M3 may arise from its origins. The globular cluster, which contains two distinct populations of stars, may be the result of a merger of two globular clusters. These two clusters were members of the same dwarf galaxy, which was later swallowed up by the Milky Way.

Hubble has taken several images of M3, also known as NGC 5272, documenting its complicated and intriguing characteristics. In this image, blue indicates the shorter wavelengths that are visible light, while red depicts the longer wavelengths of visible light, as well as some near-infrared light. Colors in Hubble images are chosen based on standard image processing techniques to best represent the wavelengths of light that pass through the filters used in the observation. Because the color and temperature of stars are directly related, we know that the blue stars in this image are hotter and the red stars are cooler.

This image is part of a Hubble Treasury program survey designed to observe approximately half of the Milky Way’s globular clusters to construct a detailed chronology of how the Milky Way galaxy formed. With over 30 years of observations, Hubble is one of NASA’s flagship observatories and works in complement with its sibling space missions, including the infrared-detecting Webb Space Telescope and the upcoming Nancy Grace Roman Space Telescope, to weave together a comprehensive picture of our vast universe.

Explore More


Exploring the Birth of Stars


Hubble’s Star Clusters


Hubble’s Nebulae

Media Contact:

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



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The Birthplace of the United States

2013-06-01 00:00:00
June 1, 2013
2013-06-01 00:00:00

Editor’s note: In honor of America’s 250th birthday, Earth Observatory is revisiting stories about the landscapes that helped shape U.S. history. The images and text on this page were originally published on July 4, 2017. Explore the full collection here.

Situated between the Schuylkill and Delaware rivers, Philadelphia was founded in 1682 by William Penn as the seat of a Quaker colony. Later, its location just upstream of the Delaware Bay and Atlantic Ocean made it an industrial, commercial, and cultural hub of the American colonies.

When the area’s original inhabitants, the Lenni Lenape (Delaware) Indians, lived here, much of the land was forested. Swedish and Dutch settlers had already traveled in the area when Penn finally came to it and signed a treaty with the Lenape to establish a city. He called his colony—now the state of Pennsylvania—Sylvania, after its sylvan, wooded appearance. Current-day Philadelphia had “a high and dry land next to the water, with a shore ornamented with a fine view of pine trees growing upon it,” according to a historical account.

More than 300 years after Penn’s arrival, this landscape remains verdant, despite its urban development. The natural-color image above shows Philadelphia and the surrounding area as it appeared on June 1, 2013, when the Operational Land Imager (OLI) on the Landsat 8 satellite passed overhead.

Nearly a hundred years after Philadelphia was established, the Founding Fathers of the United States met in this thriving city roughly at the geographic center of the 13 colonies. It was here that they debated, composed, and signed the documents that would become the blueprints of the American government. In 1776, they signed the Declaration of Independence in Carpenter’s Hall, not far from the red-brick building that then housed Pennsylvania’s colonial government; in 1787, they signed the Constitution in the same place. (Carpenter’s is now known as Independence Hall.) Between 1781 and 1788, it was also the seat of the U.S. government.

Today, Philadelphia is the fifth largest city in the U.S., with more than 6 million people living in its metropolitan area. The city saw its heyday as a manufacturing hub in the 1800s. Currently, its largest sectors include education and health services.

Traces of the city’s history remain embedded in its landscape. A belt of large, tall buildings makes up Center City, the area around Independence Hall. To the south lies a dense grid of smaller houses—South Philadelphia, home to the city’s Italian Market. At one point, this was a satellite town to the city; the two merged in 1854, when the area’s population surged. It remains a diverse area today, home to a large African American community, as well as the remnants of once sizable Italian, Irish, and Jewish immigrant populations.

NASA Earth Observatory images by Jesse Allen, using Landsat data from the U.S. Geological Survey. Story by Pola Lem.

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NASA’s Hubble Spies Stellar Sparkler for July 4th

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