Kinkajou interviews
Kinkajou:
Censored.
And for the Truly Intrepid:
Brisbane lies within the south-east corner of Queensland. And believe it or not, the area is a UFO hotspot. I have a number of acquaintances who have lived with in country areas in the region.
They have witnessed a number of UFO phenomena. But it’s one of those things that most people choose not to talk about. To talk is to invite ridicule and publicity. So most people avoid the topic.
To see a UFO requires some preparation. The key issue to observe them is to find an observation point away from the city and away from lights. The night sky in the city is bleached by city light. I think you would be lucky to see first magnitude and second magnitude stars.
So if you want to observe and to believe you need to find an isolated spot, with a high vantage point. Areas in the Gold Coast hinterland especially in some of the more mountainous areas are good.
Areas on the Mount Tambourine region adjacent to the Gold Coast hinterland are also good. Some of the regions around Springbrook, with high vantage points can also be used. South Stradbroke Island has also been mentioned.
They tend to follow a south-west to north-east or a north-west to south-east vector. My acquaintance reports that they may often be seen at the very peripheries of the region’s air traffic radar screens.
When they arrive at the peripheries of the screens they tend to shoot straight up or straight down, avoiding tracking. They can seemingly do this in the blink of an eye. They can go into the ocean.
The UFOs tend to be very interested in human activities in space. Our acquaintance tells the story of seeing approximately 27 UFO lights in the skies on the night the US space station docked with the Russian Mir space station. My acquaintance also tells the story of some very close personal contacts.
A UFO being positioned almost within touching distance of the roof of his house. A UFO accelerating away from their home in rural Mudgeeraba towards the Gold Coast and creating a sonic boom which shook windows out of houses and units in the region.
It was reported at the time but interest has faded in the event. Apparently, the air force even scrambled F111s to investigate the event. Unsuccessfully of course.
UFO at Speed
Now this is where it gets interesting. Our acquaintance gives an eyewitness account of a UFO hovering silently within touching distance and travelling in the blink of an eye noiselessly. However he also has a story about a UFO creating a sonic boom. So the question then becomes: are the silent UFOs travelling vast distances in the blink of an eye actually just lights or holograms.
Fast travel creates turbulence and displaces air: creating noise. Science tells us that moving bodies cannot change direction at right angles. However holograms can. And hence our observational dilemma.
So what are you looking for? Firstly you need to know what a satellite looks like. Satellites in low earth orbit reflect sunlight so have a low luminosity as they travel sedately and slowly across the sky. The rate of travel is approximately 10° of arc in about 20 seconds. They move in straight lines. They do not change direction.
UFOs move considerably faster. And if you observe long enough you should be able to see them change direction at some point in their trajectory. Also, if you see one there are often others.
My acquaintance says that if you stare at the sky for a week of nights you should be able to see one each two or three days. But you have to be awake. You have to be looking. And are not necessarily the brightest objects in the sky.
If you want to improve your odds, pick a night when something is happening in space. For example a satellite launch or something else of the sort.
A Caution
A word of caution. I wouldn’t trust them. Take some precautions to hide your infrared signature from observation. Take some precautions to make you less visible from observation.
Some EMF shielding such as aluminium foil may be a good idea. Prepare yourself a few hiding spots, so you can melt safely into the background.
While they are reputed to be interested in anally probing abductees, I fear their researches are likely to be much more widespread and invasive. It is also unlikely they care much about using anaesthetic for whatever they do. Good luck!
Mars Explorers
Above also features on orbitalenginetrue.html
Known star systems within 5.0 parsecs (16.3 light-years) | ||||
Altair, designation α Aquilae, is the brightest star in the constellation of Aquila | ||||
and the twelfth brightest star in the night sky. It is currently in the G-cloud | ||||
—a nearby interstellar cloud, an accumulation of gas and dust | ||||
Distance 16.73 Light Years | ||||
Designation | Distance[6] | |||
(light-years (±err)) | ||||
System | Star | |||
Solar System | Sun (Sol) | 0.0000158 | ||
Alpha Centauri | Proxima Centauri (V645 Centauri) | 4.2441±0.0011 | ||
(Rigil Kentaurus) | α Centauri A (HD 128620) | 4.3650±0.0068 | ||
α Centauri B (HD 128621) | ||||
Barnard's Star (BD+04°3561a) | 5.9577±0.0032 | |||
Luhman 16 |
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6.5029±0.0011 | ||
(WISE 1049−5319) | ||||
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7.26±0.13[18] | |||
Wolf 359 (CN Leonis) | 7.856±0.031 | |||
Lalande 21185 (BD+36°2147) | 8.307±0.014 | |||
Sirius | Sirius A | 8.659±0.010 | ||
(α Canis Majoris) |
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Luyten 726-8 | Luyten 726-8 A (BL Ceti) | 8.791±0.012 | ||
Luyten 726-8 B (UV Ceti) | ||||
Ross 154 (V1216 Sagittarii) | 9.7035±0.0019 | |||
Ross 248 (HH Andromedae) | 10.2903±0.0041 | |||
Epsilon Eridani (BD−09°697) | 10.446±0.016 | |||
Lacaille 9352 (CD−36°15693) | 10.7211±0.0016 | |||
Ross 128 (FI Virginis) | 11.0074±0.0026 | |||
EZ Aquarii | EZ Aquarii A | 11.109±0.034 | ||
(Gliese 866, Luyten 789-6) | EZ Aquarii B | |||
EZ Aquarii C | ||||
61 Cygni | 61 Cygni A (BD+38°4343) | 11.4008±0.0012 | ||
61 Cygni B (BD+38°4344) | ||||
Procyon | Procyon A | 11.402±0.032 | ||
(α Canis Minoris) |
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Struve 2398 | Struve 2398 A (HD 173739) | 11.4880±0.0012 | ||
(Gliese 725, BD+59°1915) | Struve 2398 B (HD 173740) | |||
Groombridge 34 | Groombridge 34 A (GX Andromedae) | 11.6182±0.0008 | ||
(Gliese 15) | Groombridge 34 B (GQ Andromedae) | |||
DX Cancri (G 51-15) | 11.6780±0.0056 | |||
Tau Ceti (BD−16°295) | 11.753±0.022 | |||
Epsilon Indi | Epsilon Indi A | 11.869±0.011 | ||
(CPD−57°10015) |
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GJ 1061 (LHS 1565) | 11.9803±0.0029 | |||
YZ Ceti (LHS 138) | 12.1084±0.0035 | |||
Luyten's Star (BD+05°1668) | 12.199±0.036 | |||
Teegarden's Star (SO025300.5+165258) | 12.496±0.013 | |||
SCR 1845-6357 | SCR 1845-6357 A | 12.571±0.054 | ||
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Kapteyn's Star (CD−45°1841) | 12.8294±0.0013 | |||
Lacaille 8760 (AX Microscopii) | 12.9515±0.0029 | |||
Kruger 60 | Kruger 60 A | 13.0724±0.0052 | ||
(BD+56°2783) | Kruger 60 B (DO Cephei) | |||
|
13.1932±0.0066 | |||
Ross 614 | Ross 614A (LHS 1849) | 13.424±0.049 | ||
(V577 Monocerotis, Gliese 234) | Ross 614B (LHS 1850) | |||
|
13.43±0.13 | |||
Wolf 1061 (Gliese 628, BD−12°4523) | 14.0458±0.0038 | |||
Wolf 424 | Wolf 424 A | 14.05±0.26 | ||
(FL Virginis, LHS 333, Gliese 473) | Wolf 424 B | |||
|
14.0744±0.0023 | |||
Gliese 1 (CD−37°15492) | 14.1725±0.0037 | |||
|
14.30±0.56[note 4] | |||
L 1159-16 (TZ Arietis, Gliese 83.1) | 14.5843±0.0070 | |||
Gliese 674 (LHS 449) | 14.8387±0.0033 | |||
Gliese 687 (LHS 450, BD+68°946) | 14.8401±0.0022 | |||
LHS 292 (LP 731-58) | 14.885±0.011 | |||
|
16.3±4.2 | |||
LP 145-141 (WD 1142-645, Gliese 440) | 15.1182±0.0023 | |||
G 208-44 | G 208-44 A (V1581 Cyg) | 15.2090±0.0050 | ||
G 208-45 | G 208-45 | |||
(GJ 1245) | G 208-44 B | |||
Gliese 876 (Ross 780) | 15.2504±0.0054 | |||
LHS 288 (Luyten 143-23) | 15.7703±0.0056 | |||
GJ 1002 | 15.8164±0.0098 | |||
Groombridge 1618 (Gliese 380) | 15.8797±0.0026 | |||
|
15.885±0.020 | |||
Gliese 412 | Gliese 412 A | 15.983±0.013 | ||
Gliese 412 B (WX Ursae Majoris) | ||||
Gliese 832 | 16.1939±0.0034 | |||
AD Leonis | 16.1970±0.0055 | |||
GJ 1005 | GJ 1005 A | 16.26±0.76[note 4] | ||
GJ 1005 B | ||||
System | Star | Distance[6] | ||
(Light-years (±err)) | ||||