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Wasat — Double Star in Gemini

HIP 35550; Delta Geminorum; 55 Geminorum

Observable Double Star Excellent (64/100)

Sep: 5.5", Companion: mag 8.2

Magnitude 3.5m DoubleStar Gemini (Gem) Visible
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About Wasat

Description

Wasat, Delta Geminorum, is an F-type subgiant of spectral class F2 V Fe-0.5 about 60 light-years away, notable for being a subgiant at a close, bright distance. It shines at magnitude 3.53 and is a known radial-velocity variable, with a very long-period companion suggested by decades of monitoring. Wasat is approaching the end of its main-sequence life.

Observing Tips

Wasat is in the middle of Gemini's body, between Castor and Pollux to the north and Alhena to the south. In binoculars it appears crisp and pale yellow-white. Wasat famously lies very near the ecliptic — the Sun, Moon, and planets pass close by frequently, producing occultations. Best observed December through April.

History

The name Wasat is Arabic for "the middle," referring to its position in the body of the celestial Gemini twins.

Fun Facts

Pluto was discovered only 0.3 degrees from Wasat by Clyde Tombaugh in 1930 — the star served as a key reference point in the photographic plates that led to the discovery. Wasat has been used as a target in occultation-timing campaigns to measure the angular diameters of asteroids.

Observe

1Physical Properties

Magnitude 3.53
Spectral Type F2V Fe-0.5
Star Color Yellow-white (B-V 0.34)
Distance 60 ly

2Position & Identifiers

RA 07h 20m 07.4s
Dec +21° 58' 56.0"
Constellation Gemini (Gem)
HR 2777
HIP 35550
HD 56986
SAO 79294
Bayer Delta
Flamsteed 55 Gem
Double Cat 5983

3How easy to split?

Primary 3.5 mag Companion 8.2 mag Separation 5.5″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard Hard Hard
150mm Newt. Medium+ Medium+ Medium+
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Dec – Feb (peak: Jan)

5Multiple Star System Triple

Components 3 (triple)
Component IDs O
Separation 5.5″
Companion Mag 8.2
Companion Sp K6V
Position Angle 229°
Star Colors A: Yellow-white B: Red
Discoverer STF1066
AB 3.55 F0IV, 8.18 K3V, 1200y, a = 6.975". Component A is SB, 3.7, 5.7v, sep. 0.2".

Separation over time

Measured 1822 → 2018 (196 y)
Separation drift 7.1" → 5.5" (-1.60")
Rate -0.0082" / y
PA drift 198° → 229° (+31°, +0.158°/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 229°

A: 3.5 · B: 8.2 · Sep: 5.5″ · PA: 229° · N up, E right

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

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

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

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Stellar Fusion

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15Stellar Notes

ADS 5983A, 2238.6d, K 27.1k/s, V0 +4.1k/s, asini 781. SB character has, however, been questioned by occultation | data. Unresolved by speckle interferometry 1978.96 and 1983.93.
Variously classified A9III, F0IV, F2IV.
0.039".
Wasat; Wesat.
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Light Travel Time Machine

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Relativistic Travel

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