SkyMate
Planetary system · 5 known planets · Pegasus

HR 8799

Its star: above the horizon all nightHighest after dark 23:08 · south · 60°
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HR 8799N ↑ E ← · 36° FIELD

Where is HR 8799?

Times for LondonChange city

Look south, about 60° up at 23:08 in Pegasus.

Rises
15:10
Highest
23:10
Sets
07:11
Best after dark
23:08 · 60°

Can I see HR 8799?

No. The planets of HR 8799 can’t be seen with the eye, binoculars or any amateur telescope: they are lost in their star’s light. What you can do is point toward the star.

From London tonight, the star HR 8799 is above the horizon all night. It’s highest after dark at 23:08, in the south at 60°.

Why is HR 8799 interesting?

HR 8799 has 5 known planets, discovered between 2008 and 2023 by the astrometry and imaging methods.

What can you see?

Eyes

Direction only

Around magnitude 6: at the limit of naked-eye visibility under dark skies.

Binoculars

Visible as a faint star near the Great Square of Pegasus.

Telescope

A white star. The planets themselves can’t be seen with any backyard telescope. Imaging them requires the world’s largest telescopes and special techniques to block the starlight.

What you’re likely to see, not what a space telescope photographs.

About

HR 8799 is a young white star about 130 light-years away in Pegasus. In 2008 it became the first star whose planets were photographed directly as a family: astronomers imaged several giant planets around it.

At least four giant planets orbit the star, each several times the mass of Jupiter, at distances similar to or beyond the outer planets of our Solar System. Because the system is young, the planets still glow from the heat of their formation, which is why they can be imaged.

Sequences of images taken over years show the planets slowly moving around their star.

HR 8799 is only about 30 million years old. Its known planets orbit at distances of roughly 15 to 70 times Earth’s distance from the Sun, taking decades to centuries to go around once.

The system also has belts of dust and debris inside and outside the planets, a little like the asteroid belt and Kuiper Belt around the Sun.

The HR 8799 system

Known planets of HR 8799 (catalog values from exoplanet.eu)
PlanetMassRadiusOrbitFrom starFoundMethod
HR 8799 f11.50 M♃——2.5 AU2023Astrometry
HR 8799 e11.67 M♃1.17 R♃49.3 years15.8 AU2010Imaging
HR 8799 d9.17 M♃1.20 R♃112.4 years25.85 AU2008Imaging
HR 8799 c9.02 M♃1.30 R♃224.9 years43.44 AU2008Imaging
HR 8799 b4.65 M♃1.20 R♃449.7 years68.79 AU2008Imaging

M⊕ / R⊕ = Earth masses / radii; M♃ / R♃ = Jupiter. Masses from radial velocity are often minimum masses. Data: The Extrasolar Planets Encyclopaedia, exoplanet.eu (CC BY 4.0).

Questions

If the planets were photographed, can I see them?
No. The images needed giant observatory telescopes with adaptive optics and careful blocking of the starlight.

Sources: The Extrasolar Planets Encyclopaedia (CC BY 4.0); star chart: Wikidata (CC0). Positions computed for your place and time with astronomy-engine. Data & Licences