Navi: The Star Behind the Ghost of Cassiopeia

Image of Cassiopeia constellation in a starry sky.

The backyard becomes a quiet outpost at the edge of evening. Darkness stretches across the yard as nearby porch lights vanish one by one. And above the roofline, half of Cassiopeia edges into view.

Out of the constellation Cassiopeia with the middle star identified as Navi, also known as Gamma Cassiopeiae.
Gamma Cassiopeiae (Navi) in the middle of Cassiopeia

And there it is — Navi, my favorite star, known on charts as Gamma Cassiopeiae. Pinned to the center of the Queen’s celestial “W,” the star’s silver-blue light carries the same hue as a summer lightning bolt.

Blue-white star of Navi, also known as Gamma Cassiopeiae, lighting up nearby IC 63 Ghost Nebula.
Photo: Kees Scherer | Public Domain

“That light left more than five centuries ago,” I whisper to myself, peering through the scope.

The Aztec and Inca Empires flourished, the Ming Dynasty ruled, and a young Leonardo da Vinci first picked up his brush and pencil, honing the skills that would one day make him legendary.

High above in that cathedral of night, Navi spins at nearly one million miles per hour. Its equator bulges and flickers with uncontainable energy, flinging matter outward into a swirling disk of gas that makes the star brighten and fade over time. How I wish I could step up to the firmament and witness this force!

IC 63: The Ghost of Cassiopiea

Beneath a frosty Heidelberg sky on December 30, 1893, the German astronomer Max Wolf discovered the ethereal wisps of nebulae near Navi, in the region Sh 2-185. Those faint patches, now known as IC 69 and IC 53, are clouds of ionized gas shaped by the fierce stellar winds of this restless star.

Black and white photo of Max Wolf, German astronomer who discovered IC 63.
Max Wolf | Public Domain

From our view on Earth, IC 63 sits just behind Navi, with its nearest edge about 7.5 light-years away. The star itself sculpts and illuminates this ghostly nebula. IC 63 glows red at the tip where its hydrogen gas is excited by the star’s intense ultraviolet radiation. Meanwhile, the soft blue light comes from Navi’s starlight scattering off tiny dust particles.

Showing the red and blue color of the Ghost of Cassiopeia, officially known as IC 63
NASA, ESA, and STScI
Acknowledgment: H. Arab (University of Strasbourg)

Nearby lies the related nebula IC 59, also discovered by Wolf that same night. It appears dimmer and less red, casting a beautiful blue of Navi’s starlight. Astronomers note that the nebulae are slowly evaporating under the star’s relentless radiation.

Photo shows the blue light reflecting off the IC 59 nebula from the star Navi.
IC 59 | Adam Block/Mount Lemmon SkyCenter/University of Arizona | Creative Commons

Navi: Gus Grissom’s Navigational Star

Gamma Cassiopeiae earned its nickname from astronaut Gus Grissom, whose full name was Virgil Ivan “Gus” Grissom.

Black and white image of astronaut Gus Grissom by his Liberty Bell 7 spacecraft.
Astronaut Virgil “Gus” Grissom prepares to enter his Liberty Bell 7 spacecraft, July 1961. Photo: NASA | Public Domain

It so happens that “Navi” is his middle name spelled backward, and he slipped a playful twist into NASA’s navigational star charts. According toEric Jones, Gamma Cassiopeiae became Navi for Grissom; Gamma Velorum became Regor for Roger B. Chaffee; and Iota Ursae Majoris became Dnoces for Ed White II.

After the tragic Apollo 1 fire took the lives of the three astronauts, NASA kept the star names as a quiet tribute to the crew. You can see them on the Apollo 11 star charts and on the Apollo 12 flight list.

My Observations

Tonight, I observe Navi through my telescope while using the Seestar S50 to image the Ghost Nebula. Due to light-polluted skies, I’m unable to see the faint nebula in the 8-inch scope.

Shows the star Navi (Gamma Cassiopeiae) with nearby IC 63 Ghost Nebula taken with Seestar S50 over 83 minutes of exposure.
IC 63 gets washed out by light pollution for the scope, but I’m thankful for the Seestar S50 breaking through Bortle 7-8 skies to capture the faint wisp of the nebula. Image by Wayne McGraw, 83-minute exposure, with minimal post-processing in the Seestar. Taken on November 22, 2025, at 11:30 p.m. outside of Tampa, Florida.

I’ve often visited the star over the years. For me, it has a unique beauty, and I’m always taken aback knowing it’s spinning in place while centuries vanish below it. It has been a silent witness to empires, artists, and astronauts. In a world where moments pass and things disappear, Navi continues to shine.

Key Stats

ConstellationCassiopeia
Best ViewingAutumn
Visual Magnitude2.47 – 3.03 (variable)
Absolute Visual Magnitude-3.41
Distance from Earth~550 light-years
Milky Way LocationOrion Spur
My Viewing GradeA
DesignationsSAO 21247, α Cas (Gamma Cas), HIP 32549, HR 264, HD 5394, 18 Cas, GC 792, Navi

Sources and Notes

NASA. (n.d.). IC 63 Ghost Nebula. NASA Science. Retrieved November 24, 2025, from https://science.nasa.gov/asset/hubble/ic-63-ghost-nebula/

Sh 2‑185. (n.d.). In Wikipedia. Retrieved November 24, 2025, from https://en.wikipedia.org/wiki/Sh_2-185

The Editors of Encyclopaedia Britannica. (2025, September 29). Max Wolf. In Encyclopaedia Britannica. Retrieved November 24, 2025, from https://www.britannica.com/biography/Max-Wolf

Seestar S50 image by Wayne McGraw

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