Vulpecula Constellation: The Ultimate Guide

Vulpecula (Little Fox)

Vulpecula is a constellation located in the northern hemisphere of the Earth. The constellation's name comes from Latin, meaning "little fox."

The constellation Vulpecula is near the north pole next to Cygnus and Aquila's constellations.

Vulpecula is a small constellation with very faint stars in brightness. It is difficult to see with the naked eye, so it is advisable to use binoculars.

Vulpecula's brightest star is Anser (α Vulpeculae/α Vul/6 Vulpeculae) with a magnitude of +4.44.

Despite being a relatively small constellation, Vulpecula has important deep-sky objects for astronomy, such as planetary nebulae and globular clusters.

There are no occurrences of meteor showers within the boundaries of the constellation Vulpecula.

Starregistration.net adaption of a painting of Vulpecula Constellation from Uranographia celestial atlas by Johannes Hevelius. Starregistration.net adaption of a painting of Vulpecula Constellation from Uranographia celestial atlas by Johannes Hevelius.

The Mythology And History Of The Vulpecula Constellation

Ancient Egypt

A human and a camel in an Egyptian desert under the starry night sky. A human and a camel in an Egyptian desert under the starry night sky.

Vulpecula is one of the most minor and faintest constellations in the sky; due to this, it is also one of the most recent to be introduced into astronomical calendars and celestial maps.

In turn, Vulpecula also has no myths or associated stories of antiquity, as it was not considered an independent constellation until the seventeenth century.

Early Modern Period

People in the renaissance period watch a meteor shower in a town. People in the renaissance period watch a meteor shower in a town.

During the seventeenth century, the Polish astronomer Johannes Hevelius introduced ten new constellations on his celestial globe; among these new constellations was Vulpecula.

Although it was initially known as Vulpecula cum ansere, meaning "the little fox with the goose," as a fox was shown with a small goose in its mouth, later catalogs only stayed with the fox.

Thus Vulpecula became a new constellation independent of others.

Nowadays

The milk-way in the starry night sky over the modern building of a scientific space center. The milk-way in the starry night sky over the modern building of a scientific space center.

Vulpecula currently ranks 55th in size among the 88 constellations in the night sky, spanning a 268-square-degree region of the sky.

In scientific research, Vulpecula is a region with exciting age plan nebulae that have served to study the evolution of stars and planetary systems.

How To Find The Vulpecula Constellation?

Visibility By Region

World map with latitudes showing the visibility of the Vulpecula Constellation in the Southern and Northern hemispheres. World map with latitudes showing the visibility of the Vulpecula Constellation in the Southern and Northern hemispheres.

The constellation of Vulpecula resides in the fourth quadrant of the northern hemisphere (NQ4), at latitudes between 55° S and 90° N, which means that we can see the constellation in the night sky in all countries of the world, the only exception is Antarctica.

Vulpecula is visible in the USA, Europe, Russia, China, and Japan in the northern hemisphere.

In the southern hemisphere, Vulpecula is visible in all countries such as Brazil, Argentina, Australia, New Zealand, except Antarctica.

Visibility By Season

Vulpecula is a constellation near the north pole, so it is visible throughout the year for the northern hemisphere countries; even so, the best time to see it is in September.

For the southern hemisphere countries, a section of the constellation is no longer seen in spring. Still, it is generally one of the constellations with more excellent permanence in the sky all year round.

Finding Vulpecula Constellation

The shape and the main stars of Vulpecula constellation alongside the neighboring constellations in outer space. The shape and the main stars of Vulpecula constellation alongside the neighboring constellations in outer space.

To locate the constellation Vulpecula, look to the north of the celestial vault.

Vulpecula is a small constellation with very faint stars, so you will probably have to use binoculars to find it if you live in an urban area with a lot of light pollution around you.

In terms of navigation, the best way to find the constellation Vulpecula is with the help of the constellation Cygnus. Vulpecula is a few degrees near the star Gaia DR2 2026 of Cygnus's constellation, so once you find Cygnus, you will also find Vulpecula.

Related Constellations

The location of the Vulpecula Constellation is displayed in a star map by IAU from the Sky & Telescope magazine. The location of the Vulpecula Constellation is displayed in a star map by IAU from the Sky & Telescope magazine.

The constellations bordering Vulpecula are Cygnus, Lyra, Hercules, Sagitta, Delphinus, and Pegasus.

In addition, the constellation Vulpecula belongs to the Hercules family of constellations; these include Aquila, Ara, Centaurus, Corona Australis, Corvus, Crater, Crux, Cygnus, Hercules, Hydra, Lupus, Lyra, Ophiuchus, Sagitta, Scutum, Sextans, Serpens, and Triangulum.

Stars in Ursa Minor Constellation

Officially Vulpecula has 68 stars recognized by the International Astronomical Union, of which 6 are part of the central figure of the fox, these are Anser, 23 Vulpeculae, 13 Vulpeculae, 31 Vulpeculae, 15 Vulpeculae, and 1 Vulpeculae.

Anser (α  Vulpeculae / α  Vul / 6  Vulpeculae)

Located 297 light-years from Earth, Anser is the brightest star in the constellation Vulpecula with a visual magnitude of +4.44.

It is a red giant star with a surface temperature of 3850 K and 56 times larger than the sun.

23 Vulpeculae  (23  Vul / HD 192806)

23 Vulpeculae is an orange giant of spectral type K3III located 329 light-years from the solar system; it is the second brightest star in the constellation Vulpecula with magnitude +4.52.

13 Vulpeculae  (13  Vul)

It is the third brightest star in the constellation with a magnitude of +4.58; it is a double star whose main component is a bluish-white giant.

Other Vulpecula Stars:

  • 1 Vulpeculae,  bluish-white subgiant of magnitude 4,76.
  • 3 Vulpeculae, a blue giant of magnitude 5.22; it is a slow pulsating B star (SPB).
  • 15 Vulpeculae  (NT  Vulpeculae), the variable of the typeAlfa2  Canum  Venaticorum, white star.
  • 21 Vulpeculae  (NU  Vulpeculae),Delta Scuti variable of magnitude 5.20.
  • 28 Vulpeculae,  bluish-white subgiant of magnitude 5.04. 
  • 29 Vulpeculae, white star of magnitude 4.82.
  • 30 Vulpeculae, orange giant, and spectroscopic binary of magnitude 4.93.
  • 31 Vulpeculae, yellow giant of magnitude 4.58.
  • T Vulpeculae, Is a Cepheid variable whose brightness ranges between magnitude 5.41 and 6.09.
  • U Vulpeculae, Cepheid variable star; its brightness varies between magnitude 6.73 and 7.54.
  • Z Vulpeculae, eclipsing binary star of variable brightness.
  • RR Vulpeculae, eclipsing binary star of magnitude 10.00.
  • SV Vulpeculae,long-period Cepheid star.
  • WW Vulpeculae,  Is a star  Herbig  Ae surrounded by a circumstellar disk. 
  • EP Vulpeculae,  Is an S-type star and irregular variable.
  • ER Vulpeculae,  Is a binary star of magnitude 7.36.
  • PY Vulpeculae,  Is a pulsating white dwarf.
  • QR Vulpeculae,  Is a variable star of mean apparent magnitude 4.76.
  • HD 189733,  Is a yellow-orange main-sequence star with a gas giant exoplanet.
  • HD 188015,  Is a  yellow subgiant star 172 light-years away, with an exoplanet in the habitable zone.
  • Gliese 794,  Is a  hot white dwarf of magnitude 11.55 48 light-years from Earth.
  • WR 126, Is a Wolf-Rayet star located more than 14,000 light-years away.
  • PSR B1919+21, the first pulsar discovered in 1967.

Deep Sky Objects

Vulpecula is also home to deep sky objects. Deep-sky objects are celestial bodies different from stars, such as nebulae (interstellar cloud bodies) or galaxies.

In the case of Vulpecula, it is a tiny constellation that only has five identifiable deep-sky bodies, these are:

  • M27 Planetary Nebula or Dumbbell Nebula was the first planetary nebula discovered. It has a magnitude of +7.5 and an estimated age of 9,800 years.
  • NGC 6820 is an emission nebula surrounding the open cluster NGC 6823.
  • SNR G057.2+00.8: Supernova remnant hosts magnetar, the most active known.
  • NGC 6885: Distant open cluster 1950 light-years.
  • NGC 7052: An elliptical galaxy with an apparent magnitude of 13.4, approximately 191 million light-years away. This galaxy is an essential source of radio signals.
  • Asterism Collinder  399: Also known as "The Perch" due to its shape, it is an open cluster of distant stars.

Conclusion

Vulpecula is a constellation of the northern celestial hemisphere; its name comes from Latin and means "Little Fox."

Although it is in the Northern Hemisphere, Vulpecula can be observed from all countries in the world except Antarctica.

The best month to see the constellation Vulpecula Is in September.

Vulpecula's brightest star is Anser (α Vulpeculae/α V ul/6 Vulpeculae) with a magnitude of +4.44.

The best way to find the constellation Vulpecula is with the help of the constellation Cygnus. Vulpecula is a few degrees near the star Gaia DR2 2026 of the constellation Cygnus, so once you find Cygnus, you'll also find Vulpecula.

Vulpecula does not have any associated meteor showers.

Frequently asked questions

What is the brightest star in the constellation Vulpecula?

Vulpecula's brightest star is Anser (α Vulpeculae / α Vul / 6 Vulpeculae) with a magnitude of +4.44.

What is the English meaning of the Latin constellation Vulpecula?

The constellation's name comes from Latin and in English translates as "Little Fox."

When can you see the constellation Vulpecula?

Vulpecula is a constellation close to the north pole, so it is visible throughout the year for the northern hemisphere countries; even so, the best time to see it is in September.

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