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Pi Gruis — Double Star in Grus

HIP 110506; Pi Gruis

Magnitude 5.6m DoubleStar Grus (Gru) Visible
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Observe

1Physical Properties

Magnitude 5.62
Spectral Type F3III-IV giant
Star Color Yellow-white (B-V 0.36)
Distance 121 ly

2Position & Identifiers

RA 22h 23m 08.0s
Dec -45° 55' 43.0"
Constellation Grus (Gru)
HR 8524
HIP 110506
HD 212132
SAO 231111
Bayer Pi

3How easy to split?

Primary 5.6 mag Companion 11.4 mag Separation 5.2″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard+ V. hard+ V. hard+
150mm Newt. Hard Hard Hard
C8 203mm Hard+ Hard+ Hard+
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

To reach "Medium" at Bortle 3, you'd need at least a 200 mm reflector.

4Visibility

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Best season Jul – Sep (peak: Aug)

5Multiple Star System

Separation 5.2″
Companion Mag 11.4
Position Angle 223°
Star Colors A: Yellow-white
Discoverer I 382
CPM.

Separation over time

Measured 1901 → 2016 (115 y)
Separation drift 4.6" → 5.2" (+0.60")
Rate +0.0052" / y
PA drift 207° → 223° (+16°, +0.139°/y)

Slow change over generations — observable in lifetime comparisons.

Measured from the WDS observational archive. No orbital solution has been derived — most likely the period is too long to fit an orbit to the available measurement arc.

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 223°

A: 5.6 · B: 11.4 · Sep: 5.2″ · PA: 223° · N up, E right

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

Explore

6

Size Comparison

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7

Compare Stars

8

Spectral Classification

9

Hertzsprung-Russell Diagram

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10

Stellar Lifecycle

11

Blackbody Spectrum

12

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

13

Stellar Fusion

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14Stellar Notes

Also classified F0V.
15

Light Travel Time Machine

16

Relativistic Travel

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