Hobart, Australia
Tier 4 · needs Kp 6 · Bortle 6. Live answer for Hobart tonight.
Crunching NOAA Kp, cloud cover, moon phase and darkness for Melbourne…
connecting to NOAA SWPC + Open-Meteo…
Melbourne looks south into the aurora australis, the southern counterpart of the northern lights, and its behaviour is governed by the same geomagnetic activity that drives displays over the Arctic.
Melbourne needs Kp 8 — a severe storm — and at 38°S it is the hardest of the southern cities in our data. Sightings from Melbourne itself are rare events that make the news, and the practical strategy is to travel south and west out of the city toward the coast on the rare nights when a G4 storm coincides with a clear sky.
There is no dark season to plan around at Melbourne: the sun reaches at least 18° below the horizon on every night of the year, so the sky can be genuinely black in any month you choose. What varies is the length of the usable window and the weather — the southern winter simply gives you more hours of darkness per night to work with.
Even at mid-winter the sun only reaches 75.6° below the horizon at Melbourne, and the nights stay dark enough for aurora watching right through the year. Here the practical constraint is never daylight — it is weather and how the geomagnetic field happens to be behaving.
You need to leave the city entirely and head south-west toward the coast; even then, a Kp 8 display will be a low glow over the southern horizon rather than something overhead.
Everything you are looking for is in the southern sky over the magnetic pole, so the practical requirement is simple: an unobstructed southern horizon with no artificial light in your line of sight. The "best window" shown above picks the first hour where cloud cover drops under roughly 40% while the sky here is genuinely dark.
Here is what each Kp value would actually put in Melbourne's sky — the row that matters is the one at Kp 8, which is where this city's magnetic latitude of -37.8° places its threshold:
| Kp index | What you'd see from Melbourne |
|---|---|
| Kp 0 | Not visible here. On these nights a trip south would be the only option. On those nights the forecast at the top of this page will say NO, and that is the honest answer. |
| Kp 1 | No display at this latitude; the activity is confined south of Melbourne. Nothing to plan around — save the trip for a stronger forecast. |
| Kp 2 | Not visible here. On these nights a trip south would be the only option. Worth knowing so that a quiet night reads as expected rather than disappointing. |
| Kp 3 | Nothing from Melbourne — the oval stays too far south. On those nights the forecast at the top of this page will say NO, and that is the honest answer. |
| Kp 4 | Not visible here. On these nights a trip south would be the only option. Nothing to plan around — save the trip for a stronger forecast. |
| Kp 5 | Not visible here. On these nights a trip south would be the only option. Worth knowing so that a quiet night reads as expected rather than disappointing. |
| Kp 6 | Possible as a low smudge from a dark-sky site — the city's own light will beat it. A camera will pull more colour out of this than your eyes will. |
| Kp 7 | Possible as a low smudge from a dark-sky site — the city's own light will beat it. Check the cloud forecast before committing to the drive. |
| Kp 8 | Visible low on the southern horizon from Melbourne — active arcs, and movement you can see with the naked eye. Worth clearing an evening for if the cloud cooperates. |
| Kp 9 | A good display: brighter arcs, rays climbing higher, curtains beginning to form overhead. Get out early — the best structure often arrives in the first hour. |
The most common reason people in Melbourne miss a display is not a bad forecast — it is staying inside the city. At Bortle class 9, a Kp 8 event that would be obvious from open country can be completely invisible from a lit street. If the answer above says GO or MAYBE, treat the drive out of town as part of the plan rather than an optional extra.
The score above is built from five weighted factors, each using Melbourne's own figures rather than a regional default: Kp against a local threshold of 8 (35%), cloud cover averaged across the dark hours at -37.81°, 144.96° (25%), moon illumination (15%), this latitude's astronomical darkness window (15%) and Bortle 9 light pollution (10%). How the score is built, where the numbers come from and where the method can go wrong are all set out on our methodology page. There is nothing to install and nothing to sign up for: the calculation runs in your browser against NOAA and Open-Meteo. The only third parties are anonymous analytics and Google's ad script — our privacy page lists what each one does.
Put Melbourne's threshold at Kp 8 — the first level at which the auroral oval typically stretches to a magnetic latitude like this one (-37.8°). At that level you are looking for a low arc rather than something overhead; Kp 9 and above is where it becomes hard to miss.
It is a weighted composite of the NOAA Kp forecast against a local threshold, Open-Meteo cloud cover at Melbourne's exact coordinates, the moon, and the darkness and light-pollution situation at this latitude (Bortle 9). Because cloud dominates so many nights, the score is designed to come back LOW or MAYBE more often than GO.
Dark enough all year. On the darkest night the sun reaches 75.6° below the horizon, and it clears 18° on every night of the year, so Melbourne never has a bright-night problem.
Not from the middle of town, no. Bortle 9 means Melbourne's own glow is brighter than a Kp 8 aurora, so the display is there and you simply cannot see it. Twenty to forty minutes of driving is often the difference between a wasted evening and a good one.
Melbourne has astronomical darkness on all 365 nights of the year, so there is no dark season to plan around — the limiting factors are cloud and geomagnetic activity. On a strong night, 21:00–01:00 local is statistically the most active window.
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