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Called Iota Pup in Argelander's atlas — Star in Puppis

HIP 39757; Rho Puppis; 15 Puppis

Magnitude 2.8m Star Puppis (Pup) Visible
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About Called Iota Pup in Argelander's atlas

Description

Rho Puppis is a yellow-white giant of spectral type F6IIp at magnitude 2.81 in Puppis. Located about 63 light-years from Earth, it has a luminosity of roughly 22 times solar. It is a Delta Scuti variable star, pulsating with a period of about 3.4 hours. Despite its Rho designation, it is one of the brightest stars in Puppis.

Observing Tips

Rho Pup lies in the northern part of Puppis, not far from the bright star cluster M47. It appears as a warm white star. Its pulsation period is too short and amplitude too small to detect visually. Best observed January through April from the southern hemisphere and low northern latitudes.

History

Rho Puppis was misidentified as Iota Puppis in Argelander's atlas, causing lasting confusion. As a nearby bright Delta Scuti pulsator, it has been extensively studied for asteroseismology.

Fun Facts

Rho Pup is one of the brightest Delta Scuti variable stars known, making it a cornerstone for studying these short-period pulsating stars. Its pulsations probe the star's interior structure, much like seismic waves reveal Earth's internal layers.

Observe

1Physical Properties

Magnitude 2.81
Range 2.76 - 2.86
Period 3.4 hours
Variable Type Delta Scuti (Pulsating)
Spectral Type F5IIkF2IImF5II supergiant
Star Color Yellow-white (B-V 0.43)
Distance 64 ly

2Position & Identifiers

RA 08h 07m 32.6s
Dec -24° 18' 15.0"
Constellation Puppis (Pup)
HR 3185
HIP 39757
HD 67523
SAO 175217
Bayer Rho
Flamsteed 15 Pup
Variable ID Rho Pup

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
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 Dec – Feb (peak: Jan)

5Survey Image

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Size Comparison

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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

Delta Sct 2.68 - 2.78v, 0.14088143d.
0.14088143d over 60 yr. interval.
High Fe abundance. Violet shifted CaII K emission at some phase of light curve.
Called Iota Pup in Argelander's atlas, and in Bayer.
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Light Travel Time Machine

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Relativistic Travel

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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