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Iota Crateris — Double Star in Crater

Magnitude 5.5m DoubleStar Crater (Crt) Visible
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1Physical Properties

Magnitude 5.48
Spectral Type F7V
Star Color Yellow (B-V 0.52)

2Position & Identifiers

RA 11h 38m 40.1s
Dec -13° 12' 07.0"
Constellation Crater (Crt)
HR 4488
HIP 56802
HD 101198
SAO 156802
Bayer Iota
Flamsteed 24 Crt

3How easy to split?

Primary 5.5 mag Companion 11.0 mag Separation 1.1″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard V. hard V. hard
150mm Newt. V. hard V. hard V. hard
C8 203mm V. hard V. hard V. 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 840 mm reflector.

4Visibility

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Best season Feb – Apr (peak: Mar)

5Multiple Star System C: optical

Separation 1.1″
Companion Mag 11.0
Position Angle 248°
Star Colors A: Yellow
Discoverer KUI 58

Separation over time

Measured 1934 → 2014 (80 y)
Separation drift 2.0" → 1.1" (-0.90")
Rate -0.0112" / y
PA drift 220° → 248° (+28°, +0.350°/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 248°

A: 5.5 · B: 11.0 · Sep: 1.1″ · PA: 248° · N up, E right

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

Explore

6

Size Comparison

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Compare Stars

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Spectral Classification

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Hertzsprung-Russell Diagram

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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

Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

Visibility scores assume a 150 mm Newton at Bortle 4.

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