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Iota Serpentis — Double Star in Serpens

Magnitude 4.5m DoubleStar Serpens (Ser) Visible
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1Physical Properties

Magnitude 4.52
Spectral Type A1V
Star Color White (B-V 0.04)
Distance 297 ly

2Position & Identifiers

RA 15h 41m 33.1s
Dec +19° 40' 13.0"
Constellation Serpens (Ser)
HR 5842
HIP 76852
HD 140159
SAO 101682
Bayer Iota
Flamsteed 21 Ser
Double Cat 9744

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Medium+ Medium Medium
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Apr – Jun (peak: May)

5Multiple Star System Quadruple

Components 4 (quadruple)
Component IDs AB
Separation 0.2″
Companion Mag 5.2
Companion Sp A1V
Position Angle 64°
Star Colors A: White B: White
Discoverer HU 580
AB 5.2 A1V, 5.3 AIV, 11.07y, a = 0.117". AB combined mag., color. Resolved by speckle interferometry 1986.45, | sep. 0.05".

Separation over time

Period: 21.9 y Eccentricity: 0.094 Now: 0.17", PA 73° -0.06" in 5 years
0.00" 0.06" 0.12" 0.18" 0.24" 2016 2020 2024 2028 2032 2036 0.17"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

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6

Size Comparison

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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

Pleiades group.
0.012" to 0.026".
15

Light Travel Time Machine

16

Relativistic Travel

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