3D Portrait of a 37000 K Hot Star at 2.2 kpc

In Space ·

3D visualization of a distant hot star within Gaia DR3 data

Data source: ESA Gaia DR3

3D Portrait of Gaia DR3 4056588540932900096: a 37,000 K beacon in three dimensions

In the vast tapestry of the Milky Way, a single hot star can serve as a striking anchor point for a three-dimensional map of our galaxy. The Gaia DR3 4056588540932900096—recorded by the European Space Agency’s Gaia mission—offers a vivid example. With a surface temperature around 37,000 K, this blue-white powerhouse shines with extraordinary energy, even as its light travels across thousands of parsecs to reach Earth. In a 3D visualization, it appears as a teal-blue beacon several thousand light-years away, bridging the near neighborhood and the broader disk of the Milky Way.

A measure of distance, brightness, and color

The star sits at a distance listed as roughly 2,228.5 parsecs from us, which translates to about 7,300 light-years. Those numbers place it well within the Milky Way’s disk, far beyond the immediate solar neighborhood. In three-dimensional maps, this distance helps astronomers compare its position to nearby stars, star-forming regions, and the grand spiral structure of our galaxy.

Its apparent brightness, given by phot_g_mean_mag of 15.09, indicates that Gaia DR3 4056588540932900096 is far too faint to be seen with the naked eye under typical dark-sky conditions. A modest telescope or a long-exposure sky image would be needed to capture it. The Gaia blue photometry (phot_bp_mean_mag ~ 17.12) and red photometry (phot_rp_mean_mag ~ 13.65) tell a nuanced story: the star appears unusually red in this color index, a consequence of interstellar dust along the line of sight preferentially absorbing blue light. Even so, the high effective temperature reveals its intrinsic blue-white nature.

The temperature, listed as about 37,229 K, marks this star as a true hot star. Such temperatures place it among the early-type stars, often categorized as O- or B-type. For Gaia DR3 4056588540932900096, the temperature suggests a blue-white surface that radiates enormous energy. When combined with the radius estimate of roughly 6.3 solar radii, a simple energy-estimation view emerges: the star hums with tens of thousands of times the Sun’s luminosity. In rough terms, L ≈ (R/R⊙)^2 × (T/T⊙)^4 points toward a luminous, compact, hot superstar—an excellent showcase for 3D visualization of stellar properties.

Sizing up the star in the context of space

  • : ~37,000 K. This is a hallmark of blue-white hot stars that bathe their surroundings in high-energy ultraviolet photons. In color-coded 3D renderings, this star would glow cool blue-white rather than sunset-orange.
  • : ~6.3 R⊙. While not enormous by giant standards, this radius is substantial for a hot, early-type star and supports a high luminosity.
  • : Gaia G-band magnitude ~15.1. Not visible to the naked eye, but accessible to mid-range telescopes under dark skies or with longer exposures in citizen-science imagery.
  • : RA 268.49°, Dec −29.10°. In the southern celestial hemisphere, this star sits outside the most crowded summer fields, offering a striking punctuation mark in a 3D map of the local galaxy.

Why this star matters for 3D visualization

A 3D portrait in Gaia data is not just about static coordinates. It’s about the space around the star—the line of sight through dust, the star’s motion through the disk, and how distance anchors it within the Milky Way’s architecture. Gaia DR3 4056588540932900096 provides a vivid test case: a hot, luminous beacon that anchors a distant point in a three-dimensional canvas. Its extreme temperature contrasts with its moderate apparent brightness, hinting at the dust that threads through the Galactic plane and highlights the importance of extinction when interpreting color information in Gaia's photometric system.

In a classroom or studio setting, visualizing such a star helps bridge the abstract numbers to tangible cosmic scale. Imagine a 3D orbiting map where this star stands as a bright blue anchor, its position calibrated by precise parallax and its color hinting at the starlight that arrives after crossing interstellar dust. The result is not just data; it’s a story of how light travels across the Galaxy, how we translate that light into position, and how distance reshapes our sense of the cosmos.

“In a well-crafted 3D map, a star like Gaia DR3 4056588540932900096 shines as a blue beacon, reminding us that distance is part of the beauty of celestial geometry.”

Take a step toward the sky

If you’re curious to explore this star and its neighbors in a 3D Gaia-inspired visualization, you can start by imagining the Vue of the Milky Way in layers: a disk of stars, a dusty plane, and the bright lines of hot, luminous beacons like this one. The combination of high temperature, modest apparent brightness, and substantial distance makes Gaia DR3 4056588540932900096 a compelling anchor for storytelling in three dimensions—an invitation to wander the galaxy without leaving your chair.

To bring that sense of wonder home, consider delving into Gaia data visualizations or stargazing apps that map parallax to distance and color to temperature. Each star is a point in a vast mosaic—a reminder that the sky is not a flat backdrop, but a three-dimensional tapestry you can explore stretch by stretch, light by light.

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This star, though unnamed in human records, is one among billions charted by ESA’s Gaia mission. Each article in this collection brings visibility to the silent majority of our galaxy — stars known only by their light.

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