Top 5 Rare DXCC Entities to Chase This Season

Recent Trends in DXing
This season has seen renewed interest in rare DXCC entities, driven by improving propagation conditions on the higher bands and a series of announced (and rumored) DXpeditions. Many active operators are shifting focus from common entities to those that fill critical gaps for mixed-mode or band-specific awards. Log submissions to major online databases show increased activity toward historically scarce locations in the Pacific, South Atlantic, and central Asia.

Sunspot activity continues to support long‑path openings, making late‑afternoon and early‑morning windows more productive for chasing entities that are only accessible via specific paths. At the same time, solar flux indices remain variable, prompting operators to adjust schedules based on real‑time propagation tools rather than fixed calendars.
Background on DXCC Entity Difficulty
The DXCC (DX Century Club) list currently includes over 340 entities, but a small fraction remain genuinely rare due to geographic isolation, political restrictions, or extremely limited access for amateur operation. Entities that qualify as rare often have fewer than 50 active stations per year and may go years without any activity at all.

Based on recent activity logs, pending DXpedition schedules, and historical scarcity, the following five entities are widely considered the most rewarding to chase this season:
- Pitcairn Island (VP6) – Typically activated only by multi‑yearly DXpeditions; landing and licensing remain challenging. Clusters often show 3–5 active callsigns per season.
- Navassa Island (KP1) – Strict US Fish & Wildlife restrictions limit access. Past DXpeditions required specialised permits; no regular activity expected until a new expedition is organised.
- Mellish Reef (VK9M) – Remote atoll in the Coral Sea with extremely short operating windows due to weather and military airspace. Last major activation was several years ago; any news of a new expedition is highly anticipated.
- Mount Athos (SV/A) – Requires permission from the monastic community and Greek authorities. Only a handful of operators receive licenses each year; most activity occurs during short, pre‑arranged DXpeditions.
- Burundi (9U) – Landlocked African entity with limited amateur infrastructure. Few resident operators exist; external DXpeditions face logistical hurdles with equipment transport and local regulations.
User Concerns with Rare Entities
Many DXers express frustration with two recurring issues: the unpredictability of activation schedules and the difficulty of working a rare entity during the brief windows when it is on air. Even when a DXpedition is announced, competition for limited slots in pile‑ups can lead to operator burnout and poor signal‑to‑noise conditions.
- Lack of real‑time, accurate updates on licencing and landing approvals.
- High demand often leads to QRM and excessive calling, reducing success rates.
- Cost of catching a rare entity via remote stations or web‑controlled receivers remains a barrier for some users.
Another concern is the validity of QSL cards or LotW confirmations from entities that have limited infrastructure; operators must verify that the station’s call sign and operation dates match official DXCC requirements.
Likely Impact on Ham Radio Operations
If propagation holds, the upcoming season could yield a moderate increase in QSL confirmations for the top five entities, especially if any of the rumored DXpeditions materialise. This would allow intermediate DXers to advance toward mixed‑mode or band‑based endorsements they have been missing for years.
Conversely, if solar activity declines faster than predicted, the most accessible bands (20m and 17m) may degrade, pushing operators to rely on lower bands where noise levels are higher. That shift could reduce the percentage of contacts made with rare entities, as many are only reachable on higher bands during good conditions.
DXpedition teams will also be monitoring geopolitical stability in certain regions; any changes in travel restrictions or visa processes could delay or cancel planned operations for entities like Burundi or Mount Athos.
What to Watch Next
Keep an eye on the following developments over the next three to four months:
- Official announcements from major DXpedition foundations regarding Navassa Island and Mellish Reef – any confirmed dates will drive immediate cluster demand.
- Changes in solar flux and K‑index; sudden enhancements often open brief windows for high‑band paths to Pitcairn and similar Pacific entities.
- Licencing updates from the Hellenic Amateur Radio Association concerning Mount Athos; periodic permits are sometimes issued in late summer.
- Online logs from active remote stations that may provide early indications of rare entity activity before it hits major clusters.
Operators who prepare flexible schedules and maintain real‑time alert feeds will be best positioned to work these coveted entities before the season closes.