Virgo constellation in the spring night sky

Finding & Observing Virgo

The Maiden — Largest Zodiac Constellation

Virgo is the second largest constellation in the night sky and dominates the spring heavens. Its brightest star, Spica, shines at magnitude 0.97 and serves as a crucial wayfinding star. This sprawling constellation represents Demeter or Justice, and contains some of the most spectacular deep-sky objects visible from the UK: the Virgo Galaxy Cluster, M87 with its famous black hole, and the iconic Sombrero Galaxy (M104). Follow this guide to locate Virgo, understand its mythology across cultures, and explore its treasures from naked eye to telescope.

Abbreviation
Vir
Area
1,294 sq°
Brightest Star
Spica (0.97)
Visibility
Mar – Jun
Best Month
April
Zodiac Sign
Sep 16 – Oct 31
Neighbouring
7 constellations
Special Feature
Virgo Cluster

How to Find Virgo

N↑ E← β η γ δ ε θ α ζ μ Virgo Cluster M104

Use the Spring Arc

Follow the arc of the Big Dipper's handle to orange Arcturus, then continue the curve to reach blue-white Spica. This famous "Arc to Arcturus, Speed to Spica" rule makes locating Virgo straightforward in spring.

Find Spica First

Spica is the brightest star in Virgo (magnitude 0.97) and the 15th brightest star in the entire sky. Once you spot this brilliant blue-white star low in the southeast on spring evenings, you've found Virgo's anchor point.

Trace the Maiden

From Spica, trace northward (upward on the sky) through Heze and Porrima toward the distinctive kite-shaped upper body. Epsilon is a golden star marking one wing; Zavijava lies far to the west.

Spot the Clusters

With binoculars, scan the area between Porrima and Epsilon—this is the heart of the Virgo Galaxy Cluster, the nearest large galaxy cluster. Faint fuzzy patches indicate galaxies.

Month Direction Altitude Visibility
February East-Southeast Low (15°) Rising late, challenging
March Southeast 20–25° Improving throughout month
April Due South 30–35° (Excellent) Best month for observation
May South-Southwest 30–32° Still excellent, gradually lower
June Southwest 20–25° Fading into twilight by 11pm
July West-Southwest Low (10–15°) Twilight observer only

Key Stars of Virgo

Spica α Virginis

Mag: 0.97 Type: B1 V + B2 V Distance: 250 ly

The 15th brightest star in the night sky and Virgo's unmistakable anchor. Spica is a close binary pair so gravitationally bound they're egg-shaped from mutual tidal forces, orbiting each other every 4 days. Hipparchus used Spica's position to discover the precession of Earth's axis in 127 BCE. Its name means "ear of grain"—Virgo holds a sheaf of wheat.

Porrima γ Virginis

Mag: 2.74 (combined) Type: F0 V + F0 V Distance: 38 ly

One of the most celebrated double stars in the sky—two identical F-type stars orbiting each other over 169 years. The pair was closest (~0.4" separation) in 2005 and is now steadily widening; currently a fine split in 15cm telescopes. Observing this pair year after year reveals its slow orbit—a profound demonstration of stellar mechanics.

Vindemiatrix ε Virginis

Mag: 2.83 Type: G8 IIIab giant Distance: 102 ly

The distinctive golden-yellow star marking Virgo's upper wing. The name means "grape harvester"—its heliacal rising announced the grape harvest to ancient Greeks. One of the reference stars in Greek astronomical tradition, used by Hipparchus and others for naked-eye star cataloguing.

Zavijava β Virginis

Mag: 3.61 Type: F8 V subgiant Distance: 36 ly

One of the nearest stars to Earth in Virgo at just 36 light-years. Because it lies near the Sun's apex (the direction the Sun moves through space), it was used in early 20th century measurements of solar velocity. A subgiant nearing the end of its main sequence life.

Auva δ Virginis

Mag: 3.38 Type: M3 III giant Distance: 197 ly

An obvious red-orange M-class giant visible through binoculars. The name may derive from Arabic for "the barker"—a reference to dog-related constellations near the ecliptic. A slow irregular variable showing subtle magnitude changes over months and years.

Heze ζ Virginis

Mag: 3.37 Type: A3 V + G5 V Distance: 75 ly

A wide binary system with a fast-rotating A-type primary and a slower G-type companion. Part of the "body" section of Virgo, it connects the distinctive skirt sweeping from Porrima down to Spica. Well-separated in binoculars.

Mythology & History

Greek & Roman

Virgo typically represents Demeter (or Ceres), the goddess of the harvest, holding a sheaf of wheat (Spica). The myth of Persephone explains the seasons: when Persephone descends to Hades, Demeter grieves and winter comes; when she returns, spring arrives. Alternatively, Virgo is Justice (Dike or Astraea), the last immortal to abandon humanity when the Golden Age ended.

Mesopotamian

The Babylonians called this region "The Furrow" (AB.SIN)—the furrow of a ploughed field, associated with Shala, goddess of grain. Spica was "the star of the Furrow," and Virgo herself was linked to Ishtar in her aspect as grain goddess. Deeply agricultural, reflecting the importance of the harvest to Mesopotamian civilization.

Egyptian

Associated with Isis, who held the star Spica, called "she who was brought." Spica was linked to Sopdet (the star goddess). The heliacal rising of Spica near the autumn equinox was crucial to Egyptian calendar-keeping and the annual flooding of the Nile.

Hindu & Vedic

Virgo contains the nakshatra Chitra ("the brilliant"), anchored by Spica. Chitra was one of the most important lunar mansions, linked to Tvastar, the cosmic architect who shapes reality. Also contains Svati (Arcturus area) and Vishakha. Festival of Chitrapurnima celebrates this star.

Chinese

Spica (角宿一) was the "First Star of Horn," the first of the 28 lunar mansions. The Horn mansion was the entrance to the eastern palace of the sky, associated with the Azure Dragon. Crucial for Chinese calendar reform and celestial navigation.

Deep-Sky Objects

M87 — Giant Elliptical & Black Hole

Type: Elliptical galaxy Mag: 8.6 Distance: 53 million ly
Medium

Home of one of the most massive black holes known—6.5 billion solar masses, famously photographed by the Event Horizon Telescope in 2019 as the first-ever image of a black hole shadow. Immense jets of plasma stream from the nucleus. Visible in small telescopes as a round, featureless glow; knowing what lurks in its core profoundly changes the viewing experience.

M104 — Sombrero Galaxy

Type: Spiral galaxy Mag: 8.0 Distance: 29 million ly
Medium

One of the most photographed galaxies in the sky—a brilliant nucleus with a wide dark dust lane resembling a hat brim. Located on Virgo's southern edge. A 10cm telescope shows the elongated core; 20cm hints at the dust lane structure. Best observed in April and May.

Virgo Cluster (Markarian's Chain)

Type: Galaxy cluster Mag: variable Distance: ~53 million ly
Medium

The nearest large galaxy cluster contains over 1,300 galaxies. Markarian's Chain is an elegant curved arc of bright galaxies (M84, M86, NGC 4438, etc.) visible in the same 1° binocular field. A sweep with any telescope reveals a galaxy every few arcminutes—a genuine low-power sweep object unmatched elsewhere in the sky.

M58 — Barred Spiral Galaxy

Type: Spiral galaxy Mag: 9.7 Distance: 60 million ly
Medium

The brightest spiral galaxy in the Virgo Cluster and one of the brightest Messier objects north of the equator. Shows bar and spiral structure in 20cm+ aperture under good conditions. A satisfying target for medium-sized telescopes in dark skies.

Porrima γ Virginis — Binary

Type: Double star Mag: 3.48 + 3.53 Separation: ~3" (2026)
Easy

Two essentially identical F-type stars, a pearl-white pair. In 2026 they are well-separated and widening after their closest approach in 2005. Beautiful in 10cm at 100× magnification—equal brightness components moving around a 169-year orbit. Track their motion year after year.

M49 — Elliptical Galaxy

Type: Elliptical galaxy Mag: 8.4 Distance: 56 million ly
Easy

The brightest member of the Virgo Cluster and the first Virgo Cluster galaxy discovered by Messier in 1771. Easy in small telescopes; appears as an out-of-focus star at low magnification. A good entry point into cluster galaxy observing.

Beginner Observing Guide

  1. Find the spring arc: In April, locate the handle of the Big Dipper in the northwest. Trace the curve of the handle downward and eastward—it points to orange Arcturus. Continue this arc; you'll reach blue-white Spica, the brightest star in Virgo.
  2. Locate the main figure: From Spica, look northward (upward on the sky). You'll see Heze, then Porrima (a golden star), then Delta and Epsilon—forming a distinctive kite or upper-body shape. These five stars define Virgo's main frame.
  3. Scan for cluster galaxies: Point binoculars at the area around Porrima and slightly north toward Epsilon. This is the heart of the Virgo Galaxy Cluster. In dark skies, you'll notice faint fuzzy patches—these are galaxies at 50+ million light-years distance.
  4. Resolve Markarian's Chain: With a 15cm+ telescope at low power (50×), aim near Porrima and find the curved arc of bright galaxies known as Markarian's Chain (M84, M86, NGC 4438). A stunning sight—multiple galaxies in a single field of view.
  5. Hunt the Sombrero: M104 lies in southern Virgo, toward the border with Corvus. Star-hop south from Spica using nearby star fields. A 20cm+ scope reveals the striking dark dust lane—one of the most visually distinctive galaxies from the ground.
  6. Compare galactic forms: Over the course of an observing session, view M87 (featureless elliptical), M104 (spiral with dust lane), and M49 (another elliptical). Recognize how galaxy morphology varies and relate each to its distance and orientation.

Essential Kit

Naked Eye
Spica, main figure
Binoculars
Virgo Cluster haze
8cm Refractor
M104, M49, M87
15cm+ Dobsonian
Galaxy detail, Porrima split
Telescope Camera
Markarian's Chain
Best Time
Apr, 10pm

Advanced Observing

M87 Black Hole

Knowing you can see (faintly) the galaxy containing the first-ever photographed black hole is extraordinary. The Event Horizon Telescope's 2019 image and subsequent refinements in 2024 provide unprecedented context. When viewing M87, visualize the 6.5 billion solar mass black hole at its core.

Porrima's Orbit

Check Porrima's separation each year. The pair will continue widening until around 2090 before closing again. Become part of a centuries-long observational record. Record your measurements and compare with other amateurs—you're tracking orbital mechanics in real time.

Virgo Cluster Sweep

The Virgo Cluster spans approximately 8°—equivalent to 16 full moons placed edge to edge. Using a low-power wide-field eyepiece, systematically sweep the area north of Porrima. Count the galaxies visible; compare counts over multiple nights and different apertures.

M104 Dust Lane Detail

The Sombrero's dust lane requires 20cm+ aperture from a dark site. At high magnification (150×+) under perfect conditions, the dark lane becomes a striking visual feature. Sketch its extent and structure; photograph it through different filters to enhance contrast.

Pro Tip:

Virgo contains the highest concentration of bright galaxies visible from mid-northern latitudes. Devote multiple observing sessions to this region—you'll develop skill at identifying galactic structure, recognizing morphological types, and understanding large-scale cosmic structure.