La Asociación Entrerriana de Astronomía (AEA) y la Liga
Iberoamericana de Astronomía (LIADA) invitan al I Encuentro de Astronomía
Lunar, a realizarse el 7 de diciembre de 2015 a las 18 hs. en el Observatorio de
la AEA, Escuela Alberdi, Oro Verde:
sábado, 28 de noviembre de 2015
sábado, 14 de noviembre de 2015
LOS OBSERVADORES LUNARES DE LA ASOCIACIÓN ENTRERRIANA DE ASTRONOMÍA EN LOS NÚMEROS DE NOVIEMBRE DE “THE LUNAR OBSERVER” (ALPO) Y “LUNAR SECTION CIRCULAR” (BAA).
A
pesar de tener una primavera de cielos casi siempre nublados, los observadores
lunares de la Asociación Entrerrianala Asociation of lunar and
planetary observers” (ALPO).
Aparecimos
en la sección bimestral “Focus On”, que hace un análisis de un accidente lunar
en particular, esta vez el cráter Deslandres (pág.8).
También
aparecimos en la Sección
“Lunar Topographical Studies” (págs.14/15), con observaciones de Deslandres,
Mare Nubium, Pallas y Plato (las imágenes de éstas dos últimos fueron incluidas
entre las mejores fotografías).
En
la sección del “Lunar Geological Change Detection Program” (pág.19) se informa
que se utilizaron nuestras observaciones de Deslandres, Mare Crisium, Mare
Nectaris, Plato, Proclus, Alphonsus, Copernicus, Aristarchus y Tycho. Se hizo
especial referencia a la imagen que obtuvimos de Plato el 6-9-2015 y de cómo se
utilizó para cotejar con un reporte de un Fenómeno Lunar Transitorio de 1916
(pág. 20).
En la sección de dedicada al “Lunar Geological Change Detection Program” de la “Lunar Section
Circular” de la British Astronomical9 a 11).
Para
quienes quieran leer ambas revistas:
The Lunar Observer (ALPO):
http://alpo-astronomy.org/
The Lunar Section Circular (BAA):
lunes, 2 de noviembre de 2015
OBSERVACIONES PARA EL PROGRAMA DE DETECCIÓN DE CAMBIOS LUNARES DEL 24-10-15
Desde el
Observatorio de Oro Verde de la Asociación Entrerriana
de Astronomía Francisco Alsina Cardinalli, Juan Manuel Biagi y Alberto
Anunziato realizamos el día 24 de octubre de 2015 una serie de observaciones
lunares con nuestro telescopio Meade LX 200 de 250 mm . y la Webcam Phillips
SPC900NC a foco primario. Observamos Gassendi, Plato y Aristarchus para el
programa de la British Astronomicalla Association of Lunar and
Planetary Observers (ALPO) Lunar Geological Change Detection Program. Subimos
las imágenes y los videos correspondientes a IMAPS Computing Support - Amateur
Astronomy Outreach.
Gassendi:
Name and location of
observer: Francisco Alsina Cardinalli (Oro Verde, Argentina).
Name of feature: Gassendi.
Date and time (UT) of
observation: 10-24-2015: 03.43.
Size and type of telescope
used: 250 mm .
Schmidt-Cassegrain (Meade LX 200).
Filter (if used): Oxigen
III Narrowband Filter-1.25
In .
Medium employed (for photos and electronic images):
Phillips SPC900NC webcam
Seeing: 7/10.
Esta era la
observación requerida:
2015-Oct-24
UT 01:58-03:43 Ill=84% Gassendi observed by Madej_P on 1985-5-30
On 1985 May 30 P.Madej (Huddersfield, UK, 77mm refractor, x111 and x250, seeing II-III, transparency good) whole spectrum of colours seen on the central peak area, visible in both eyepieces, and was more prominent at the higher magnification. Not aware if the observer checked for this effects on other terminator peaks? ALPO/BAA weight =1.
Plato:
Name and location of
observer: Alberto Anunziato (Oro Verde, Argentina).
Name of feature: Plato.
Date and time (UT) of
observation: 10-24-2015: 04.36.
Size and type of telescope
used: 250 mm .
Schmidt-Cassegrain (Meade LX 200).
Filter (if used): None.
Medium employed (for photos and electronic images):
Phillips SPC900NC webcam
Seeing: 7/10.
Esta era la
observación requerida:
2015-Oct-24
UT 04:27-06:39 Ill=84% Plato observed by North_G on 1981-8-11 *
On 1981 Aug 11 at UT21:05-21:36 G. North (England, seeing=poor) detected, in green light, a darkening on the floor of Plato. This effect was not seen elsewhere. J-H Robinson (Teighmouth, Devon, UK) detected on the SSE rim (inner and beyond) a triangle that appeared hazy in a wide range of filters at 21:05UT. However at 21:36UT it was only hazy in green and blue light. No similar effect was seen elsewhere. The Cameron 2006 catalog ID=150 and weight=5. The LPO/BAA
weight=3.
Aristarchus:
Estas eran las observaciones requeridas:
2015-Oct-24
UT 01:38-03:23 Ill=83% Aristarchus
observed by Moore_P on 1985-5-30 . On 1985 May 30 at UT 20:10-23:54
P.Moore (Selsey, UK, 15" reflector)
and at the same time Doherty (Sussex, UK, 15" reflector) observed a
strangely bright and pink/red north rim of Aristarchus crater during UT20:20
and 20:36UT. The effect reduced between ~20:39 and 20:44UT. M.C. Cook (Frimley, UK) found the northern
wall to have a red/purple colour but the
effect vanished after 50 minutes. Cook also saw a "V"- like notch in the NW crater shadow and this
appeared to be bigger than normal. G.
North (Sussex, UK) saw a tinge of pink colour on the northern rim and a bit later a "ruby
red" colour on the north-west wall - again this effect lasted 50 minutes. Moseley
verified the colour. Finally M. Hather
(Yorkshire, UK) suspected the north wall of
Aristarchus to be blue in colour. Cameron suspects that this TLP is not
spurious colour because it is in the wrong place. The Cameron 2006 catalog ID=276 and the weight=5. The
ALPO/BAA weight=4.
2015-Oct-24 UT 03:46-05:26 Ill=84% Aristarchus observed by Foley_PW on 1975-12-14
Aristarchus 1975 Dec 14/15 UT 17:05-00:30
Observed by Foley (Dartford, England, 12" reflector, S=II) and Moore
(Sessex, England, 15" reflector
x250 S=IV) and Argent and Brumder
(Sussex, England) "In early sunrise conditions, W. wall was less
brilliant than usual -- matched only by Sharp, Bianchini, & Marian.
Extraordinary detail could be seen on this wall. Also noted intense & distinctly blue color
entire length of W. wall. 3 others corroborated detail, but not color. Moore
found things normal & saw Aris.
brightest at 2030-2125h tho Argent & Brumder
made it < Proclus" NASA
catalog weight=4. NASA catlog ID #1422.
ALPO/BAA weight=1.
2015-Oct-24 UT 04:33-05:26 Ill=84% Aristarchus observed by Zeller_P on 2013-4-22
On 2013 Apr
22 UT 01:39-02:37 P. Zeller (Indianapollis, USA, 10" f/4 reflector, x200,
seeing 6, Transparency 3 - scattered cirrus) observed visually (depicted in sketch)
the two closely spaced NW wall dark
bands) to have a rusty-red hue. The colour of these bands did not change over
the period of the observing session. Images were taken, but resolution and
image S/N is not sufficient to resolve separate bands here, or to detect
colour. The ALPO/BAA weight=2.
2015-Oct-24 UT 05:17-05:26
Ill=84% Aristarchus.
ALPO Request: On 2013 Apr 22 Paul Zellor noticed that the
two closely spaced NW dark bands in Aristarchus had some (non-blue) color to
them. Can we confirm his observation of natural colour here? Ideally you should
be using a telescope of 10" aperture,or larger.
Pudimos observar
Aristarchus de 01.30 a
01.55 (04.30 a 04.55 UT).
Las 3 primeras observaciones requeridas correspondían a http://users.aber.ac.uk/atc/tlp/tlp.htm,
la última al Lunar Observing Schedule y era la más prioritaria. Nuestras
observaciones cubrieron parte del horario correspondiente a la segunda y a la
tercera, se realizaron con posterioridad al horario de la primera y no
alcanzaron a cubrir el horario de la última, ya que las nubes cubrieron por
completo Aristarchus a las 01.55, como quedó registrado en video.
sábado, 10 de octubre de 2015
LOS RAYOS DE ARISTARCHUS
Obtenida desde el Observatorio de la Asociación Entrerriana de Astronomía el 6 de septiembre de 2014.
Reportada a la Asociation of Lunar and Planetary Observers (ALPO), aparecida en el número de octubre/2015 de "The Lunar Observer".
Reportada a la Asociation of Lunar and Planetary Observers (ALPO), aparecida en el número de octubre/2015 de "The Lunar Observer".
martes, 6 de octubre de 2015
DE PASEO POR PLATO CERCA DEL TERMINADOR
Durante
la madrugada del domingo 6 de septiembre de 2015 (escuchando discos de
Kraftwerk) observamos distintos accidentes lunares con el telescopio principal
del Observatorio de Oro Verde de la Asociación Entrerriana250 mm , usando una webcam Phillips SPC900NC. La
imagen corresponde al cráter Plato. El profundo, plano y oscuro fondo de este
gigantesco cráter no permitió que observáramos los cinco pequeños cráteres que
son uno de los desafíos de los observadores lunares. Las altas paredes de esta
verdadera “llanura amurallada” muestran los signos de los derrumbes. En la
pared occidental (a la derecha en la foto), observamos un bloque de 50 kilómetros
cuadrados que se ha desprendido y deslizado hacia el fondo. Plato es famoso por
las sombras que proyectan sus altas murallas. En la fotografía vemos como las
sombras del terminador avanzan sobre las paredes del flanco occidental, que
brillan reflejando la luz del Sol que se pone. La sombra que proyecta el pico
más alto de la pared occidental (de 2000 metros de altura) puede observarse
nítidamente. Las sombras en el interior de Plato son muy cambiantes, cada
observación de ellas capta un momento único: “The appearance and orientation
of the shadows within Plato are never the same from one lunation to the next
because of the effects of libration and the change in the direction of
illumination by the Sun that it causes” (“La apariencia y la orientación de las
sombras en el interior de Plato nunca son las mismas de una lunación a la
siguiente, debido a los efectos de la libración y el cambio de dirección de la
iluminación solar que ocasiona”). (“The moon and how to
observe it”, Peter Grego, Springer, 2005). En la parte
inferior vemos el Mare Frigoris, los cráteres más prominentes son Plato A y
Fontenelle. En el lado sur, en el Mare Imbrium, se observan puntos iluminados
que son las cumbres más altas de los Montes Teneriffe. En el extremo superior
izquierdo de la imagen, al suroeste, la ladera iluminada del Mons Pico brilla
como un triángulo de luz. En la sombra, los puntos brillantes son las cimas de
los Montes Alpes más cercanas.
Aparecido en "The Lunar Observer" del mes de octubre de 2015
ÚLTIMAS APARICIONES DE LA SECCIÓN LUNAR DE LA AEA EN “THE LUNAR OBSERVER (ALPO) Y “LUNAR SECTION CIRCULAR” (BAA)
La
aparición de nuestras observaciones y fotografías lunares en la revista
"The lunar observer" de la Association of Lunar and Planetary
Observers (ALPO) se ha transformado en una reciente tradición. En los números
de agosto y septiembre aparecieron fotografías de Francisco Alsina Cardinalli
del cráter Dionysius. En el número de octubre aparecieron fotografías de Juan
Manuel Biagi (Alphonsus y Copernicus), Francisco Alsina Cardinali (Deslandres,
Aristarchus y Tycho) y Alberto Anunziato (Deslandres y Plato más un dibujo de
Theophilus). Además, aparecimos en la Sección dedicada al Lunar Geological
Change Detection Programa con la mención del video obtenido de Plato el 23 de
agosto. Ese mismo video aparece mencionado también la sección dedicada al mismo
programa en la "Lunar Section Circular" de la British Astronomical
Association (BAA).
Los dejamos con
una fotografía correspondiente a la sesión de observación del 6 de septiembre,
el cráter es Copernicus:
viernes, 18 de septiembre de 2015
LA LUZ CENICIENTA
Impúdicamente, descubrimos lo que la Luna no nos quiere mostrar.
Como diría Felisberto Hernández: “No podía hacerme la idea de que yo admiraba
un paisaje que no fuera de la Tierra y me parecía que aquel atrevimiento lo
tendría que pagar con la locura”.
Se trata de la luz cenicienta (“earthshine”), la tenue luz
que ilumina la parte de la
Luna que no es bañada por la luz del Sol y que normalmente no
vemos desde la Tierra. Es
Es un fenómeno no muy fácil de atrapar fotográficamente,
pero lo consiguió el miembro de nuestra AEA Juan Manuel Biagi en la prehistoria
de nuestra Sección Lunar. Tenemos un gran archivo de fotografías y videos
lunares sin procesar que de a poco iremos desempolvando y sacando del arcón,
éste es el primero. Fue obtenida a las 5.59 del 21 de septiembre de 2014 a mano
alzada, apoyando la cámara sobre el telescopio.
sábado, 29 de agosto de 2015
OBSERVACIÓN DEL CRÁTER PLATO EN BÚSQUEDA DE CONFIRMACIÓN DE REPORTE DE FENÓMENO LUNAR TRANSITORIO
SÁBADO
22 de agosto de 2015.
Desde
el Observatorio de Oro Verde de la Asociación Entrerriana de Astronomía
observamos el cráter Plato desde las 02.35 (UT) hasta las 03.21 (UT). Lo
hicimos con la Webcam Phillips SPC900NC a foco primario. La observación fue
realizada a pedido de la British
Astronomicalla
Association of Lunar and Planetary Observers (ALPO),
en el marco del programa Lunar Geological Change Detection Program.
Esta
era la observación requerida:
2015-Aug-23 UT
02:40-03:15 Ill=52% Plato
BAA Request: It has been
noticed that a bright craterlet can
appear very suddenly on the floor of Plato in between needle like shadows, during local lunar sunrise.
This happens in the
space of just a minute or
so, and can look really quite dramatic.
This effect was first
spotted by Brian Halls on 2014 Oct 31. Please send any high resolution images,
detailed scetches, or visual descriptions to: a t c @ a b e r . a c. u k .
Desde el inicio y la finalización de la observación la Luna estuvo cubierta por
nubes que permitían la observación pero en malas condiciones. Calculamos un
seeing de 4 en escala 1-10, un II en la escala de Antoniadi.
Los
integrantes de la Sección Lunar
Reporte:
Name and location of
observer: Francisco Alsina Cardinali, Camilo Satler, Alberto Anunziato (Oro
Verde, Argentina).
Name of feature: Plato.
Date and time (UT) of
observation: 08-23-2015-02.35 to 03:21.
Size and type of telescope
used: 250 mm. Schmidt-Cassegrain (Meade LX 200).
Filter (if used): None.
Medium employed (for photos and electronic images): Phillips
SPC900NC webcam
Seeing: 4/10.
El
registro en video de la observación (de 02.40 a 03.21 UT) puede descargarse
aquí:
sábado, 22 de agosto de 2015
NUESTRO PRIMER REPORTE A LA ALPO FUE PUBLICADO EN THE LUNAR OBSERVER
En el número de agosto de 2015 de la revista "The lunar observer", publicada por la Association of lunar and planetary observers" (ALPO) puede leerse, en la página 12, la mención a un reporte de un miembro de nuestra asociación (Francisco Alsina Cardinali). Se trata de una fotografía (1 toma única) del cráter Dionysius.
LA REVISTA, AQUÍ: http://alpo-astronomy.org/
La ALPO había solicitado en números anteriores de "The lunar observer" realizar todas las observaciones posibles de ese cráter y específicamente entre las 0,10 y las 10.56 (en tiempo univeral) del día 5 de julio en el marco del "Lunar Geological Change Detection Program". Este programa busca compilar reportes de fenómenos lunares transitorios (FLT) nuevos y revisar reportes antiguos.
Para la revisión de reportes antiguos se solicitan observaciones de un accidente lunar en las mismas condiciones de iluminación solar y libración que las que se dieron al momento del reporte del FLT. Esas condiciones sólo se dan desde determinadas coordenadas geográficas y en determinado horario. El análisis de la fotografía nueva puede dilucidar si se dan en la misma los mismos fenómenos reportados como FLT. Si se repiten en la nueva fotografía es probable que no sean un FLT sino que se deban a las condiciones de iluminación de la Luna en ese momento. Si no se observan los fenómenos (lo que parece haberse dado en nuestra observación de Dionysius) se suma una certeza sobre el reporte antiguo de FLT. Esto quiere decir que nuestra observación tiene el valor de sumar un grano de historia a la ciencia astronómica, al permitir dicha verificación. Y más si solamente desde nuestra zona del continente y a la hora indicada se podía comprobar. Tal es el objetivo de la cooperación entre astronomía amateur y astronomía profesional: los amateurs colaboramos con la compilación de datos (si nuestras observaciones son de calidad) que usaran eventualmente los científicos.
Este reconocimiento efectuado por ALPO, la entidad de observadores planetarios y lunares más prestigiosa del mundo, en la biblia de los observadores lunares, como es "The lunar observer", fue una gran alegría para nuestra querida Asociación Entrerriana de Astronomía y un incentivo para seguir con la observación lunar.
Aquí va nuestro reporte:
Name and location of observer: Francisco Alsina Cardinali (Oro Verde, Argentina).
Name of feature: Dionysius.
Date and time (UT) of observation: 07-05-2015-07.20.
Size and type of telescope used: 250 mm. Schmidt-Cassegrain (Meade LX 200).
Magnification (for sketches): 106 x (Via Telextender).
Filter (if used) : None.
Medium employed (for photos and electronic images) : Eos Digital Rebel XS.
Y aquí la foto del cráter Dyonisius, en la madrugada del 5 de julio de 2015, con una luna iluminada en un 88% (furiosa Luna llena), lo que no ayuda precisamente a la claridad de la imagen.´
viernes, 29 de mayo de 2015
FENÓMENOS LUNARES TRANSITORIOS A CONFIRMAR. 30 Y 31 DE MAYO
Amigos Lunáticos:
He aquí una lista
de accidentes lunares que podremos observar durante el sábado y el domingo en
las mismas condiciones que se dieron en pasados reportes de fenómenos lunares
transitorios. Las observaciones permiten registrar si lo que se observó se
repite (lo que seguramente indicaría que no estamos en presencia de un FLT sino
de un fenómeno producido por las condiciones de iluminación de la superficie) o
no se repite (indicio de un FLT).
Recuerden que a los
horarios en UT hay que descontarles 3 horas para tener el horario argentino.
Selección para
telescopios de aficionado.
30 de mayo:
Mancha roja en Timocharis:
2015-May-30 UT 00:37-02:25 Ill=87% Timocharis
observed by Firsoff on 1954-10-8. Observed by Firsoff (Somerset, England,
6.5" reflector? x240) "Red glow." NASA catalog weight=4 (high). NASA catalog ID #573.
Manchas circulares en Aristarco:
2015-May-30 UT 00:38-02:26 Ill=87% Aristarchus
observed by Grego_P on 1987-1-11. On 1987 Jan 11 at UT 18:15-23:00 P. Grego
(Birmingham, UK, 6" reflector, seeing=III) sketched Aristarchus crater and
saw two luminous circular patches on the exterior west wall - these were less
bright than the inner wall but brighter than the outer wall. The Cameron 1978 catalog ID=292 and weight=5.
Oscurecimiento en
Plato:
2015-May-30 UT 00:38-02:26 Ill=87% Plato observed by Moore_P on 1987-1-11. On 1987 Jan 11 at UT P. Moore (Sussex, UK) found the the floor of Plato was much more drk than the adjacent Mare Imbrium. Furthemore there was a blurring of detail over the northeast wall and onto the nearby floor. Detail elsewhere in the crater was OK. By 23:00UT there was less lack of detail effects. M. Cook (Frimley, UK) at 21:55UT noted the obscured area but decided that it was narrower than the same effect one month ago and suspected that she may have been observing towards the end of this TLP. The effect gradually dimmed between 21:55 and 22:45UT. Other craters were normal. G. North was affected by poor seeing conditions. Davies detected a slight obscurtion on the north east corner - it was a misty gray feature at x200. The Cameron 2006 catalog extension ID was 292 and the weight was 5. Tha ALPO/BAA weight was 4.
Mancha oscura en Gassendi:
2015-May-30 UT 00:48-02:42 Ill=87% Gassendi
observed by Unknown_Observer on 1889-5-11. n 1889 May 11 at 22:00? UT an
unknown observer saw an ink black spot
on the rampart of Gassendi. It had not been seen before ar at the next
lunation or indeed ever again. Cameron 1978 catalog ID=261
and wight=3. ALPO/BAA weight=2.
Oscurecimiento del suelo del cráter Proclus:
2015-May-30 UT 03:09-04:55 Ill=87% Proclus
observed by Bartlett on 1970-10-12. Proclus 1970 Oct 12 UT 00:54 Observed by
Bartlett (Baltimore, MD, USA, 4" reflector, 51x-181x) "Floor darkened
to intensity 1.5 deg (albedo) & c.p. became invis. Next day c.p. reappared
& was 5 deg bright & 6deg bright on 15th" NASA catalog weight=4
(high). NASA catalog ID #1277.
Mancha luminosa, como un pico, en las sombras del cráter
Herodoto:
2015-May-30 UT 03:32-05:29 Ill=87% Herodotus observed by Bartlett on 1957-9-6. Observed by Bartlett (Baltimore, MD, USA, 5" reflector x180, S=1-5,T=5) Pseudo peak visible within floor shadow at 03:10h" NASA catalog weight=4 (high). NASA catalog ID #671. ALPO/BAA weight=3.
Oscurecimiento en
Herodoto:
2015-May-30 UT 03:54-05:48 Ill=87% Herodotus observed by Haas_W on 2002-2-24. On 2002 Feb 24 UT 05:15-05:35 W. Haas (Las Cruces, NM, USA) observed an obscuration in Herodotus - the shadown was, almost, but not completely black. ALPO/BAA weight=2.
Mancha luminosa en
Schickard:
2015-May-30 UT 04:13-05:54 Ill=87% Schickard observed by Watkins_E on 1972-9-19. Schickard 1972 Sep 19 UT 19:45-20:25, 20:00-23:30 Observed by Watkins (Herts., Eng. 4.5" reflector, x225, S=G) Amery (Reading, Eng.m 12" reflector?), Fitton (Lancashire, Emg., 8.5" reflector) and Moore (Selsey, Eng., 12.5" reflector?, 4.5" refractor 45-225x, S=P) "Luminous, nebulous spot attracted Watkin's att'n. Got brighter. Checked 'scope--not instru. Obj. had greenish-gray color, size @ 15km. Amery & Fitton with blink devices noted nothing unusual at later times (2000-2330h). Aris., Plato, Gass. were neg. at 1930-2025h (date not given, guessed at fr. available info.). Turbulence, lasting secs. at a time." NASA catalog weight=2. NASA catalog ID # 1344. ALPO/BAA weight=2.
Una neblina sospechosa en Mons Pico:
2015-May-30 UT 05:40-05:54 Ill=88% Mons_Pico observed by Rawstron on 1933-10-1. On 1933 oct 01 at UT 03:00 Rawstron (USA, 4" refractor, x330) observed the following in Mons Pico B: "Haze -- much narrower & elongated than on Sep. 1". The Cameron 1978 catalog ID=407 and weight=3. The ALPO/BAA weight=2.
Una raya luminosa y pasajera en Aristarco:
2015-May-30 UT 22:17-00:10 Ill=92% Aristarchus observed by Johnson on 1937-9-17. Johnson, of Des Moines, Iowa, USA, using a 7" reflector and an 8" refractor, saw a bight streak. The observer looked later, but it was no longer visible. Cameron thinks that it might have been a reflection from the wall. Cameron 1978 catalog ID=423 and weight=1. ALPO/BAA weight=1.
31 de mayo:
Un raro fenómeno en Plato:
2015-May-31 UT 03:19-07:13 Ill=93% Plato observed by Moore_P on 1984-2-14. On 1984 Feb 14 P. Moore (Selsey, UK) observed that Plato was darker than the nearby mare and no detail could be seen on the floor or the eastern wall - the later was obscured. At 23:40UT some dimming was still present on the north east wall and still no detail on the floor of Plato. Cook noticed that the eastern floor close to the wall was misty and also noted no detail on the floor. Amery though noted that all parts of the floor were sharp although some darkening was visible in the north west and a hint of obscurtion. The east wall though was quite sharp. Mosely could see the central craterlet but from 8-6 o'clock tricky to define (Foley says that this effect has been seen at this colongitude before). Streak ray across the floor of Plato seen (North) - filter measurements made. Cameron 2006 catalog extension ID= 241 and weight=5. ALPO/BAA weight=2.
Oscurecimiento de Gassendi:
2015-May-31 UT 04:09-05:52 Ill=93% Gassendi observed by Robinson_JH on 1977-5-30. On 1977 May 30 at 21:04-02:13UT J.H.-Robinson noted a loss of detail inside Gassendi, however he did not regard this as a TLP. The effect was also seen by P.W. Foley. Cameron 2006 extension catalog TLP ID=16 and weight=0 ALPO/BAA weight=1.
Aumento de brillo en Aristarco:
2015-May-31 UT 05:01-06:49 Ill=93% Aristarchus observed by Louderback_D on 1988-1-2. On 1988 Jan 02 at 06:41-07:08 UT D. Louderback (South Bend, WA, USA, using a 8" reflector, seeing 4 out of 10) observed that at 06:56 UT Aristarchus floor (point F) brightened rapidly from an intensity of 5.2 to 6, however at 07:08 UT the spot returned to normal. He also noticed that the bands on the walls varied every few minutes. A mist like appearance was seen on the floor of Aristarchus. Through a red filter he could see through the haze, but floor detail could not be seen through a blue filter. Cameron 2006 extension catalog ID=316 and weight=4. ALPO/BAA weight=3.
Una anomalía luminosa
en Daniell:
2015-May-31 UT 22:12-23:59 Ill=97% Daniell observed by Unknown_Observer on 1982-3-8. Unknown observer. A colour and brightness anomaly was seen a TLP alert was put out. Cameron 2006 catalog extension weight=165 and weight=3. ALPO/BAA weight=2.
miércoles, 15 de abril de 2015
FENÓMENOS LUNARES TRANSITORIOS A CONFIRMAR EN ABRIL
En la entrada
anterior nos referíamos al “gran enigma lunar”, los “fenómenos lunares
transitorios”. Quien quiera conocerlos un poco más, puede leer una antigua
entrada en nuestra web (http://astroentrerios.com.ar/web/page/197/?option=com_content&task=view&id=471&Itemid=81
).
El estudio de
este enigma es una enorme oportunidad para el aficionado. Su tarea no se limita
a la observación directa de un fenómeno tan elusivo. También puede contribuir a
la confirmación de FLT producidos con anterioridad. ALPO publica mensualmente
un catálogo con la información día por día sobre fenómenos lunares transitorios
producidos en el pasado y cuyas condiciones de iluminación se reproducen para
observadores ubicados en una determinada zona geográfica y en un horario
determinado. La observación de la zona lunar indicada en el horario indicado
(que es siempre UT o en castellano TU, tiempo universal) ayuda a confirmar de
que se trató de un FLT o de lo que se observó como tal es una rasgo de la zona
observada que se vuelve a observar en las mismas condiciones. Este estudio es
fascinante, porque nuestra observación será única y tendrá un valor poco común
para una observación amateur.
A continuación,
la información brindada por ALPO para lo que resta de abril:
Ill is percentage illumination of the Moon
*Indicates a repeat illumination and libration event to within +/- 1 deg for both
A non-* indicates just repeat illumination to within +/-0.5 deg
*Indicates a repeat illumination and libration event to within +/- 1 deg for both
A non-* indicates just repeat illumination to within +/-0.5 deg
2015-Apr-15 UT 08:18-09:53 Ill=15% Earthshine:
sporadic meteors
2015-Apr-16 UT 09:27-09:54 Ill=8% Earthshine: sporadic meteors
2015-Apr-21 UT 21:49-21:55 Ill=12% Earthshine: Lyrids: ZHR=18 & Eta Puppids & (radio) Delta Piscids
2015-Apr-22 UT 21:18-21:46 Ill=20% Picard observed by Unknown_English_Observer on 1909-5-23
2015-Apr-16 UT 09:27-09:54 Ill=8% Earthshine: sporadic meteors
2015-Apr-21 UT 21:49-21:55 Ill=12% Earthshine: Lyrids: ZHR=18 & Eta Puppids & (radio) Delta Piscids
2015-Apr-22 UT 21:18-21:46 Ill=20% Picard observed by Unknown_English_Observer on 1909-5-23
In 1909 May 23 at UT 18:00? an unknown English observer observed a
bright spot east of Picard. The Cameron 1978 catalog ID=330 and the
weight=1. The ALPO/BAA weight=1.
2015-Apr-22 UT 21:18-21:45 Ill=20% Aristarchus observed by Bornhurst on 1965-12-27
On 1965 Dec 27 at UT Bornhurst (Monterey Park, CA, USA, 10" reflector)
and (Harris (Whittier? CA, USA, 19" reflector?) observed brightening of
Aristarchus in Ashen light. Cameron says that this is an independent
confirmation? The Cameron 1978 catalog ID=918 and weight=4. The
ALPO/BAA weight=2.
2015-Apr-22 UT 21:48-22:47 Ill=21% Earthshine: Lyrids: ZHR=18 & Eta Puppids & (radio) Delta Piscids
2015-Apr-23 UT 21:34-23:03 Ill=29% Aristarchus observed by Miles_H on 1990-1-1
On 1990 Jan 01 at UT 16:55-18:45 H. Miles (Cornwall, UK) observed that
Aristarchus was seen in Earthshine at 16:55UT before the limb (was
visible in Earthshine?). "1705 Aris>>1723 fading 1727 > again." Then:
"1740 Aris << and just visible at 1845". Apparently Foley suspects that
Aristarchus had brightened up before 16:55UT (shwen H. Miles started to
observe) and then gradually retruned to normal. The Cameron 2006
catalog ID=385 and the weight=0. The ALPO/BAA weight=1.
2015-Apr-23 UT 22:07-23:37 Ill=30% Copernicus observed by Miles_H on 1990-1-1
On 1990 Jan 01 at UT 17:29 H. Miles (Cornwall, UK) observed that
Copernicus had a faint glow in it. The Cameron 2006 catalog ID=385 and
the weight=0. ALPO/BAA weight=1.
2015-Apr-23 UT 23:24-23:40 Ill=30% Aristarchus observed by Struve_F on 1822-1-27
On 1822 Jan 27 at UT 20:00? F. Struve (Pulkovo Observatory? Russia)
observed near Aristarchus an 8th magnitude star-like point. Seen
through overcast! (Klado gave date as 1821 but must be in error
according to cameron). The Cameron 1978 catalog ID=95 and the weight=4.
The ALPO/BAA weight=2.
2015-Apr-23 UT 23:39-23:40 Ill=30% Aristarchus observed by Celis on 1969-10-16
On 1969 Oct 16 at UT 00:00-00:30 Celis (Quilpue, Chile, 3" refractor,
x60, seeing=very good) observed brilliant points at 8.5 magnitude in
Aristarchus. This was not seen the next night or the one after, nor
after 5 days age. The Cameron 1978 catalog ID=1204 and weight=1. The
ALPO/BAA weight=1.
2015-Apr-23 UT 21:47-23:42 Ill=30% Earthshine: Lyrids: ZHR=18 & Eta Puppids & (radio) Delta Piscids
2015-Apr-24 UT 21:16-00:08 Ill=39% Kant observed by Trouvelot on 1873-1-4 *
Kant 1873 Jan 04 UT 23:00? Observed by Trouvelot (Cambridge, Mass, 8"
refractor) "Luminous puplish vapors" NASA catalog weight=3 (average).
NASA catalog ID #180.
2015-Apr-24 UT 21:24-22:43 Ill=39% Posidonius observed by Cook_AC on 1984-12-28
Posidonius 1984 Dec 28 UT 18:52-18:54 Observed by Cook (Frimley, UK,
Moon Blink used, Seeing V, Transparency very poor) "Spurious colour on
W. Proclus. Posidonus nothing apart from prominent spurious colour on
small bright craterlets. 18:54-18:57 Censorinus - Blue on N red on S.
Almost 100% sure that the effect seen in Posidonius was spurious
colour" ALPO/BAA weight=1.
2015-Apr-24 UT 21:39-23:12 Ill=39% Proclus observed by Darling_D on 1989-2-11
On 1989 Feb 11 at UT23:30-01:39 D. Darling (Sun Praire, WI, USA, 12.5"
reflector, x159, seeing=7/10) observed a linear east to west feature in
Proclus. D. Weier (WI, USA, 11" reflector, x378) found the NNW part of
the crater to be brighter than expected and confirmed the prescence of
the east to west feature - this crossed the shadow on the east floor
and over into Mare Crisium. R. Manske (WI, USA) detected another
"streak" parallel to this. All observers suspect that the linear
features were due to raised topography on the floor of Proclus -
however Cameron comments that there does not seem to be any linear
features on the floor of Proclus to cause these effects. The Cameron
2006 catalog ID=351 and the weight=5. The ALPO/BAA weight=2.
2015-Apr-24 UT 21:53-23:30 Ill=39% Aristarchus observed by Johnson_G on 1985-4-26
G Johnson of Swanton, MD, USA used a 2" refractor at f/12.
Aristachus revealed as a red spot on a photo of the Moon. This
was similar to another photo obtained on 1988 Apr 21st. Frame (with 3
exposures present)reveals a dim star like point near Campanus on
exposure 1. Expsoure 2 shows it a little east on the Earth-lit
part. Exposure 3 shows it off the south-east limb. Apparently 20
minutes later took 2 exposures and frame 18 was a double. The
second exposure revealed an object farther from the limb but the
first exposure does not show the object. The two high power exposures
do not show it. Cameron could not see the spots that Johson describes
on his slides, but did see several spots (defects?) on the
8 and 12 second exposures near Hevelius and also on the 20 second
exposure near to Hecataeus only. BAA members observed star like
flashes a few hours earlier - near Aristarchus. One BAA member, Madej,
had seen a green glow in Arisarchus in two places in two eyepieces.
Cameron 2006 Catalog extension ID=265 and weight=2.
2015-Apr-24 UT 21:53-23:30 Ill=39% Campanus observed by Johnson_G on 1985-4-26
G Johnson of Swanton, MD, USA used a 2" refractor at f/12.
Aristachus revealed as a red spot on a photo of the Moon. This
was similar to another photo obtained on 1988 Apr 21st. Frame (with 3
exposures present)reveals a dim star like point near Campanus on
exposure 1. Expsoure 2 shows it a little east on the Earth-lit
part. Exposure 3 shows it off the south-east limb. Apparently 20
minutes later took 2 exposures and frame 18 was a double. The
second exposure revealed an object farther from the limb but the
first exposure does not show the object. The two high power exposures
do not show it. Cameron could not see the spots that Johson describes
on his slides, but did see several spots (defects?) on the
8 and 12 second exposures near Hevelius and also on the 20 second
exposure near to Hecataeus only. BAA members observed star like
flashes a few hours earlier - near Aristarchus. One BAA member, Madej,
had seen a green glow in Arisarchus in two places in two eyepieces.
Cameron 2006 Catalog extension ID=265 and weight=2.
2015-Apr-24 UT 21:53-23:30 Ill=39% Hecataeus observed by Johnson_G on 1985-4-26
G Johnson of Swanton, MD, USA used a 2" refractor at f/12.
Aristachus revealed as a red spot on a photo of the Moon. This
was similar to another photo obtained on 1988 Apr 21st. Frame (with 3
exposures present)reveals a dim star like point near Campanus on
exposure 1. Expsoure 2 shows it a little east on the Earth-lit
part. Exposure 3 shows it off the south-east limb. Apparently 20
minutes later took 2 exposures and frame 18 was a double. The
second exposure revealed an object farther from the limb but the
first exposure does not show the object. The two high power exposures
do not show it. Cameron could not see the spots that Johson describes
on his slides, but did see several spots (defects?) on the
8 and 12 second exposures near Hevelius and also on the 20 second
exposure near to Hecataeus only. BAA members observed star like
flashes a few hours earlier - near Aristarchus. One BAA member, Madej,
had seen a green glow in Arisarchus in two places in two eyepieces.
Cameron 2006 Catalog extension ID=265 and weight=2.
2015-Apr-24 UT 21:53-23:30 Ill=39% Hevelius observed by Johnson_G on 1985-4-26
G Johnson of Swanton, MD, USA used a 2" refractor at f/12.
Aristachus revealed as a red spot on a photo of the Moon. This
was similar to another photo obtained on 1988 Apr 21st. Frame (with 3
exposures present)reveals a dim star like point near Campanus on
exposure 1. Expsoure 2 shows it a little east on the Earth-lit
part. Exposure 3 shows it off the south-east limb. Apparently 20
minutes later took 2 exposures and frame 18 was a double. The
second exposure revealed an object farther from the limb but the
first exposure does not show the object. The two high power exposures
do not show it. Cameron could not see the spots that Johson describes
on his slides, but did see several spots (defects?) on the
8 and 12 second exposures near Hevelius and also on the 20 second
exposure near to Hecataeus only. BAA members observed star like
flashes a few hours earlier - near Aristarchus. One BAA member, Madej,
had seen a green glow in Arisarchus in two places in two eyepieces.
Cameron 2006 Catalog extension ID=265 and weight=2.
2015-Apr-24 UT 22:20-23:54 Ill=39% Aristarchus observed by Classen on 1967-4-15
On 1967 Apr 15 at UT 19:15-21:00 Classen (Pulsnitz Observatory, East
Germany, 8" refractor) found that Aristarchus was very bright and the
atmospheric seeing was very good until 21:00UT. Nothing unsual was seen
on 16th and 17th April. Cameron reports that this was the first TLP
seen by this group. The Cameron 1978 catalog ID=1022 and the weight=3.
The ALPO/BAA weight=2.
2015-Apr-24 UT 22:56-00:37 Ill=40% Aristarchus observed by Stretton on 1794-3-7
On 1794 Mar 07 at UT 20:00 Stretton, Wilkins and Msekelyn (England, UK)
observed Aristarchus appearing as a light like a star in Earthsine
(independent confirmation according to Cameron?). According to Cameron,
Maskelyne observed the effect for ~15 minutes. The Cameron 1978 catalog
ID=73 and 74 and the weight=5. The ALPO/BAA weight=3.
2015-Apr-24 UT 21:46-00:39 Ill=40% Earthshine: sporadic meteors
2015-Apr-25 UT 21:15-21:57 Ill=49% Unknown observed by Gaboreau on 1895-9-25
On 1895 Sep 25 at UT 20:00? Gaboreau (Paris, France) observed on the
Moon s shaft of light (same observation as Cameron's TLP report #281
and further more it is on the same day and month as it was back in
1893. The Cameron 1978 catalog ID=286 and weight=0. The ALPO/BAA
weight=1.
2015-Apr-26 UT 00:11-00:39 Ill=50% Ross_D observed by Cross on 1964-6-17
On 1964 Jun 17 at UT 04:15-05:01 Cross et al. (Whittier, CA, USA, 19" ?
reflector, S=7-8) observed near Ross D: "Gas cloud. Motion". The
Cameron 1978 catalog ID=818 and weight=4. The ALPO/BAA weight=4.
2015-Apr-25 UT 21:45-01:08 Ill=50% Earthshine: sporadic meteors
2015-Apr-26 UT 01:14-01:35 Ill=50% Agrippa observed by Bartlett on 1966-11-19
Agrippa 1966 Nov 19/20 UTC 23:58-00:14 Observed by Bartlett (Baltimore,
MD, USA, 5" reflector x283, S=4, T=5) "Faint bluish tinge seen at base
of NW wall beneath landslip" NASA catalog weight=4 (high). NASA catalog
ID #995.
2015-Apr-26 UT 01:34-03:01 Ill=50% Unknown observed by Paolo_F on 1997-4-14 *
On 1997 Apr 14 at UT 20:00-22:00 F. Paolo (Legnano, Italy)
photographed a lunar flare on the lunar limb.
2015-Apr-26 UT 21:13-22:51 Ill=59% Ptolemaeus observed by Cook_AC on 1978-4-15
Ptolemaeus 1978 Apr 15 UTC 21:54-22:20 Observed by A.Cook
(Frimley, Surrey, UK, 12" reflector x240, S=IV (Antoniadi))
"Small triangular area on the NW floor of the crater, at the
foot of the rim, was slightly brighter in blue light than in red
(Moonblink used). Suspected this was due to the poor observing
conditions. Certainly blink reaction was not unmistakable".
ALPO/BAA weight=2.
2015-Apr-26 UT 22:02-22:33 Ill=59% Archimedes observed by Hill_EG on 1966-3-29
Archimedes 1966 Mar 29 UT 21:00 Observed by Hill (England, 24"
reflector, x250, S=E) "Brightening of E-W bands across floor.
(Obscuration accord. to Moore)" NASA catalog ID #923. NASA
catalog weight=3. ALPO/BAA weight=2.
2015-Apr-26 UT 22:59-00:56 Ill=59% Mons_Pico observed by Quinn on 1986-11-9
On 1986 Nov 09 at UT 23:00 Quinn (Glebview, IL, USA, 8" reflector, x49-
x305) found ïn the vicinity of an unnamed ridge points toward Pico- two
bright points about 5 magnitudes brighter than any other part of the
Moon. The Alpine valley points directly between these two points. "Came
from apparently featureless area. Both points about the same size, but
different shapes ~ width of alpine valley" The observer used 4
different eyepieces and the points were brightest in the lowest power.
Other specks of light could be seen in the darkness wound the N point.
The Cameron 2006 catalog ID=289 and the weight=3. The ALPO/BAA
weight=2.
2015-Apr-26 UT 23:36-01:23 Ill=59% Archimedes observed by Burnerd on 1922-5-4
In 1922 May 04 at UT Burnerd (England?) discovered three long mounds in
Archimedes crater (rays?). The Cameron 1978 catalog ID=385 and weight=
0. The ALPO/BAA weight=1.
2015-Apr-27 UT 00:41-02:26 Ill=60% Plato observed by Carle on 1952-2-4
On 1952 Feb 04 at UT 02:00? J. Carle (USA, 8" reflector, x180) observed
the following in Plato: "A shadow in a depression, or a cloud, or an
optical illus.? Oval dark area nr. center, disappeared in 15m clear &
prominenet at first then vanished 4 of 14 spots nr. center continuously
seen while remaining ones seen only momentarily. (seeing?) Drawing
includes sketch on March 7. His sketch shows 18 spots, 13 same as
here". The Cameron 1978 catalog ID=549 and the weight=2. The ALPO/BAA
weight=2.
2015-Apr-27 UT 00:48-01:56 Ill=60% Alphonsus observed by Wise on 1967-4-17
Alphonsus and limb 1967 Apr 17 UTC 21:30 Observed by Wise (England,
6.5" reflector, x90) "3 dark patches (Alphonsus) prominent. Suspected
red patch (blink ?). (indep. confirm. of Cross 1h later?)." NASA
catalog weight=3 (average). NASA catalog ID #1024.
2015-Apr-27 UT 00:48-01:56 Ill=60% Plato observed by Wise on 1967-4-17
Plato 1967 Apr 17 UTC 21:30 Observed by Wise (England, 6.5" reflector,
x90) "Suspected a blink, (red?)" NASA catalog weight=2 (low). NASA
catalog ID #1025.
2015-Apr-27 UT 00:48-01:56 Ill=60% W_Limb observed by Wise on 1967-4-17
On 1967 Apr 17 UT 21:30 Observed by Wise (England, 6.5" reflector, x90)
saw a brilliant object nr. E(ast. ?) limb (West Lim IAU?) for 15m.
Check on star maps neg. (indep. confirm. of Cross 1h later?)." NASA
catalog weight=3 (average). NASA catalog ID #1024.
2015-Apr-27 UT 00:59-02:09 Ill=60% Montes_Teneriffe observed by Hart on 1854-12-27
nr. Plato in Teneriffe Mountains 1854 Dec 27 UT 18:00-23:00 Observed by
Hart & others (Glasgow, Scotland, 10" reflector) "2 luminous fiery
spots on bright side on either side of a ridge, contrasting color.
Seemed to be 2 active volcanoes. Ridge was normal color. Spots were
yellow or flame color. Never seen before in 40 yrs. of observing." NASA
catalog weight=4 (high). NASA catalog ID #129. ALPO/BAA weight=4.
2015-Apr-27 UT 01:02-02:27 Ill=60% Alphonsus observed by Jasmin_G on 2003-4-10
On 2003 Apr 10 at 00:40UT a GLR observer G. Jasmin (Quebec, Canada,
using a 10" F-10 Schmidt Cassegrain) took a photograph of Alphonsus
crater on Kodak 400ASA film with an exposure of 1/30th sec. There was a
light visible (diameter 10 km ) inside Alphonsus and the effect was
present for 5 minutes. The observer commented that they have seen a
light in this crater many times before, but never as long as 5 minutes.
This report was submitted to the GLR group in Italy. The ALPO/BAA
weight=2.
2015-Apr-27 UT 01:19-02:32 Ill=60% Theaetetus observed by Moore_P on 1952-12-24
Thaetetus 1952 Dec 24 UT 20:00? Observed by Moore (England?)
"Bright spot, hazy line of light" NASA catalog weight=4. NASA
catalog ID 556. ALPO/BAA weigh=2.
2015-Apr-27 UT 01:55-02:32 Ill=60% Plato observed by Lade on 1889-6-6
On 1889 Jun 06 at 22:00 UT Lade of France (8" refractor) saw two
extremely bright spots (Plato B & D). Cameron 1978 catalog ID=262 and
weight=2. ALPO/BAA weight=1.
2015-Apr-27 UT 01:59-02:32 Ill=60% Proclus observed by Darling_D on 1989-2-14
On 1989 Feb 14 at UT03:45-04:38 D. Darling (Sun Praire, WI, USA, 12.5"
reflector, 3" refractor, x90, seeing=3/10 and transparancy=5) noted
that there was a dark patch of brightness 4.5 on the south east of
Proclus - it was not as dark as it was on 1988 Jul 22. Cameon comments
that the dark patch is normal. The north rim of Proclus was 9.0 in
brightness, the floor had a brightness of 6.0, the west rim and south
wall were both 7.5. The Cameron 2006 catalog ID=352 and the weight=0.
The ALPO/BAA weight=1.
2015-Apr-27 UT 02:00-02:32 Ill=60% Chacornac observed by Khachatryan_S on 2009-8-28
On 2009 Aug 28 at UTC 17:00:15-17:00:42 S. Khachatryan (Yerevan,
Armenia, 127mm Maksutov-Cassegrain, x171, seeing 9 (1=worst and 10-
best), Transparency 5-6 on a scale of 1 to 6) observed in the Chacornac
area a series of fiery sparks (dot like with tiny rays), slightly
elongated with the multitudinal rays orientated towards the south west
direction. The colour was mostly red, with some yellow. The final flash
was the most clear. The TLP was tiny in area, but "was distinctly
bright against any other object on the Moon". The positional
uncertainty of the location of the spark effect was approximately +/-
150 km , based upon an examination of an atlas afterwards. Just prior to
the spark effect, something dark, small and fuzzy (only just discrnable
to the eye, through the eyepiece) was seen to pass from the west across
the Moon in a slight curve, round the surface of the Moon to the east
(post observation estimate: seen for 3.5 sec and covered roughly 8% of
the lunar diameter in that time). The area of the dark object was
comparable in size to (or slightly less than?) craters such as
Autolycus F (diameter 3km) or le Monnier E (diameter 4km) i.e. on the
limits of vision of the scope used. The location of the flash was not
exactly at the same location as the dark object passed across, but gave
the impression of starting from it? A back of the envelope calculation
of the lunar diameter covered in the time quoted gives an approximate
speed (at the lunar distance) of 80km/s or on the very high end of
typical meteor streams that pass by. At closer distances, and
recalculated velocities, it is unlikely to be a satellite in low Earth
orbit (20m/sec at 100km distance), but could perhaps be a bird or
insect at a few km range? So was this dark object something in our
atmosphere by chance passing across the field of view close to the time
of the TLP flare or was at the lunar distance and related to the TLP?
Incidentally, no attempt was made during this observation to move the
scope to check that the TLP remained stationary against the Moon. The
ALPO/BAA weight=2.
2015-Apr-27 UT 02:13-02:32 Ill=60% Aristarchus observed by Foley_PW on 1988-2-25
On 1988 Feb 25 at UT20:00? P.W. Foley (Kent, UK, 12" reflector) found
that Aristarchus was very bright (especially in the UV end of the
spectrum) despite other features not being seen in Earthshine. The
cameron 2006 catalog ID=318 and the weight=1. The ALPO/BAA weight=1.
2015-Apr-27 UT 22:10-23:31 Ill=68% Aristarchus observed by Madej_P on 1984-12-31
Although the crater was on the night side, a small bright spot
was seen. This was blue, almost UV, and equivalent to a star of
magnitude 2. It flashed over intervals of about 30 seconds
and changed in colour from UV to blue. The BAA Lunar Section
TLP network was alerted. Mobberly and J.Cook did not see much
although J. Cook may have seen something, but located else where?
Cameron lists this as a confirmed? observation? The Cameron
2006 TLP xtension catalog has this TLP with an ID No. of 258
and a weight of 4. The ALPO/BAA weight is 2.
2015-Apr-28 UT 00:11-01:10 Ill=69% Plato observed by Moore_P on 1995-9-3
On 1995 Sep 03 at UR19:40-20:15 P. Moore (Selsey, UK, 15" reflector at
x400) observed that the floor of Plato was much darker than he would
normally expect and futhermore no interior craterlets were seen. there
was however a white patch that was barely visible at the location of
the central craterlet should have been. G. North (UK) attempted to
observe nut the Moon was too low and seeing terrible. F. Doherty
reported Plato normal. Cameron 2006 catalog ID=475 and weight=3.
ALPO/BAA weight=2.
2015-Apr-28 UT 00:33-02:24 Ill=69% Linne observed by Tacchini on 1868-7-28
Linne 1868 Jul 28 UT 20:00? Observed by Tacchini (Palermo, Italy)
"Shadow not so marked-had a light penumbra, indicated a feeble cavity.
Other craters had a black shad. On 29th appeared completely white.
Crater normal on 26th. (letter to Madler Sep. 16, 1868)." NASA
catalog weight=4 (high). NASA catalog ID #159.
2015-Apr-28 UT 00:40-02:17 Ill=69% Plato observed by Carle on 1952-2-5
On 1952 Feb 05 at UT 05:10 J.Carle (USA, 8" reflector, x180)
observed the following in Plato: "A shadow in a depression, or a
cloud, or an optical illus.? Oval dark area nr. center,
disappeared in 15m clear & prominenet at first then vanished. 4
of 14 spots nr. center continuously seen while remaining ones
seen only momentarily. (seeing?) Drawing includes sketch on
March 7. His sketch shows 18 spots, 13 same as here". The
Cameron 1978 catalog ID=549 and the weight=2. The ALPO/BAA
weight=2.
2015-Apr-28 UT 00:49-02:04 Ill=69% Tycho observed by Albert_J on 2010-8-19
On 2010 Aug 19 at UT 00:50-01:02 J.Albert (Lakeworth, FL, USA,
C11, Transparency 3, Seeing 7-8, 86F and very humid. Oberver
checking out repeat illumination condition appearence for Tycho
concerning LTP #468 in the 1978 Cameron catalog. Did not see the
effect from the original TLP report, but did see, immediately at
looking at Tycho a very faint hint of redness in a pencil thin
arc (< 1/4 circumference of the rim) confined to the top of the
rim of the well-lit north east wall. Coloured arc similar in
thickness to Rupes Recta, but not as sharply defined. The outer
(E) edge was perhaps sharper than the inner edge. The redness
was more on the inside of the top of the rim. The outside of the
rim was bright white. This effect was seen in three different
eyepieces, at 311x, 224x and 400x. Checked for the effect on
other craters nearby but could not see this effect anywhere
else. The colour had dissapeared by 01:02UT. The fade took about
1-2 minutes. Observation of Tycho continued until 01:06UT, but
all seemed normal. Quick checks were made again on Tycho
periodically until 02:50UT but the colour was not seen again.
ALPO/BAA weight=3.
2015-Apr-28 UT 01:38-02:15 Ill=69% Mare_Humorum observed by Dixon_M on 1989-2-15
On 1989 Feb 15 at UT 03:15-03:30 M. Dixon (Palenque Ruins, Mexico, 7x35
binouculars) observed a point of light that was very bright in or near
Mare Humorum. It was visible for 5 minutes then vanished. The Cameron
2006 catalog ID=353 and weight=1. The ALPO/BAA weight=1.
2015-Apr-28 UT 01:41-03:20 Ill=69% Plato observed by Reese_EJ on 1949-3-9
Plato 1949 Mar 09 UT 02:00-03:00 E.J.Reese (6" reflector x240)
and one hour later T.R.Hake (5" refractor x300) both unable to
see any detail on the floor of Plato, despite both being able to
see a "difficult to see" cleft near to the crater Connon. Reese
was able to see detail under similar illumination back in 1948
and 1947 and saw the floor craterlets in Plato clearly then.
ALPO/BAA weight=2.
2015-Apr-28 UT 01:54-03:29 Ill=69% Copernicus observed by Firsoff on 1955-7-28 *
Copernicus 1955 Jul 28 UT 20:20 Observed by Firsoff (Somerset, England,
6.5" reflector x200) "Great brilliance of the terraces in E(IAU?) wall
system(?) gets specular refl. (he gave 0820UT, but must have meant
2020" NASA catalog weight=4 (high). NASA catalog No. #600.
2015-Apr-28 UT 22:14-00:06 Ill=77% Proclus observed by Cook_MC on 1982-2-3
M.C. Cook (Frimley, UK) got an abnormally low brightness reading for
Proclus, despite nearby Censorinus being normal. Crater Extinction
Device used. The Cameron 2006 Extension catalog ID was 163 and the
weight was 3. The ALPO/BAA weight was 2 too.
2015-Apr-29 UT 01:39-03:03 Ill=77% Plato observed by Davies_H on 1988-10-20
H. Davies (Llamandel, Swansea, (Scotland?), using a 3" refractor,
detected a short duration reddish hue along the inner NE-NW? rim
(4-7 O'Clock location. Sketch supplied to Foley (BAA coordinator)
No similar effect seen elsewhere. A.C. Cook (Frimley, UK)
detected spurious colour on several craters, including Plato
that night. Cameron 2006 Catalog Extension ID=337 and
weight=0. ALPO/BAA weight=1.
2015-Apr-29 UT 01:56-03:30 Ill=77% Mare_Crisium observed by Arsyukhin on 1981-6-12
Arsyukhin and others (Moscow, USSR), with naked eye and binouculars
saw three dark spots suddenly appear on Mare Crisium and disappear
approximately 30 minutes later. Cameron 2006 catalog extension ID=145
and catalog weight=4. ALPO/BAA weight=2.
2015-Apr-29 UT 01:56-03:30 Ill=77% Plato observed by Arsyukhin on 1981-6-12
Arsyukhin and others (Moscow, USSR), with naked eye and binouculars
saw TLP activity in Plato that Cameron thinks confirms what UK
observers saw later. Cameron 2006 catalog extension ID=145
and catalog weight=4. ALPO/BAA weight=1.
2015-Apr-29 UT 02:37-03:51 Ill=78% Alphonsus observed by Jenning on 1966-4-1
Alphonsus 1966 Apr 01 UTC(?) 03:00-03:20 Observed by Jenning, Harris
(Coral Estates, CA, USA, 12" reflector) "Red patch from c.p. to W. wall
(no confirm. from Corralitos obs. moon blink device & obs. at that
time)" NASA catalog weight=3 (average). NASA catalog ID #924.
2015-Apr-29 UT 03:28-04:25 Ill=78% Plato observed by North_G on 1980-7-22
On 1980 Jul 22 at UT20:08-21:50 G.North (Sussex, UK, 8" reflector, x144
and x207, seeing III-V and transparency fair) suspected an obscuration
on the north and north west wall. The effect came and went. May have
been due to seeing and image contrast? Cameron 2006 catalog ID=101 and
weight=1. ALPO/BAA weight=1.
2015-Apr-29 UT 21:10-22:20 Ill=84% Gassendi observed by Cook_AC on 1977-9-23
Gassendi 1977 Sep 23 UTC 21:15 Observed by Cook (Frimley, England, 6"
reflector x144, Seeing IV (Antoniadi)) "Prominent red dot seen at
central peak, also a hint of red on floor in N. quadrant of crater.
More likely to be spurious colour than TLP the observer feels"
2015-Apr-29 UT 21:14-23:10 Ill=84% Plato observed by Mobberley_M on 1982-6-2
Mobberley could not see the central craterlet on the floor of
Plato tonight. Foley notes that he could only just see
the central craterlet on nights of 2-5th Jun and it was
of reduced in brightness from normal. North reported
that the floor seemed nearly black, but brighter in
a green filter (x144 magnification used). All three
observers compared the Plato area to other areas for reference.
Cameron 2006 extension catalog ID 170 and weight=5.
BAA/ALPO weight=3.
2015-Apr-29 UT 23:21-23:40 Ill=84% Torricelli_B observed by Cook_MC on 1983-4-23
A blue tinge was seen inside and outside the crater
perimeter. The surrounding halo lost brightness that
was observed on 1993 Jan 29. Observed on Apr 19, 20 and 28th.
Cameron 2006 extension catalog ID=213 and weight=5.
ALPO/BAA weight=3.
2015-Apr-29 UT 23:30-01:21 Ill=84% Gassendi observed by Cook_AC on 1978-8-14
Gassendi 1978 Aug 14 UTC 21:22-21:35 Observed by Cook (Frimley,
England, 12" reflector x240, Seeing V (Antoniadi), Moon blink used)
"Blink reaction in filters seen in Gassendi. Spurious colour seen
without Moonblink in Gassendi and elsewhere. Moon at -18 deg in
Declination, hence very low and not suprised to see spurious
colour!". ALPO/BAA weight=1.
2015-Apr-30 UT 00:12-02:09 Ill=85% Torricelli_B observed by North_G on 1990-1-7
On 1990 Jan 07 at UT 20:20-20:58 G.North (Herstmonceux, UK) thought
that he detected dullness in Torricelli B crater - Cameron comments
that this cannot be shadow). The Cameron 2006 catalog ID=386 and the
weight=3. ALPO\/BAA weight=2.
2015-Apr-30 UT 04:10-05:20 Ill=85% Plato observed by Fauth on 1906-3-6
Plato 1906 Mar 06 UT 22:00? Observed by Fauth (Germany? 6" refractor)
"Color (brightness?) greatly enhanced as it was to be on the next
nite" NASA catalog weight=3 (average). NASA catalog ID #324.
2015-Apr-30 UT 04:19-05:20 Ill=85% Swift observed by Wilkins_HP on 1927-5-12
Peice A (Swift=IAU name?) 1927 May 12 UT 22:03 Observed by Wilkins
(England, 15" reflector) "Complete obscuration of crater. Saw no trace
of it. It was vis. May 11 & faint on May 13. 3x in 1948 Moore saw whole
area misty gray & devoid of detail, whereas surroundings were sharp &
clear. Birt also found it invis. at times in late 1800's" NASA catalog
weight=4. NASA catalog ID #394. ALPO/BAA weight=3.
2015-Apr-30 UT 04:22-05:20 Ill=85% Hyginus observed by Bradford on 1959-9-13
Near Hyginus 1959 Sep 13 UT Observed by Bradford (S.Shields,
England, 15"? reflector), Feist, Lovas (Hungary), Moore, Wilkins
(Kent, England, 7" refractor, x500) "Obliterated by a hovering
cloud (Feist disagrees). Budapest obs. saw a cloud at 21:02:30,
lasting 5 m . Moore & Wilkins saw burst of light & dust cloud at
21:02:35 (confirm.) Drawing by Lovas." NASA catalog weight=5 and
catalog ID #722. The ALPO/BAA weight=4.
2015-Apr-30 UT 04:22-05:20 Ill=85% Littrow observed by Bradford on 1959-9-13
Littrow, 1959 Sep 13 UT Observed by Bradford (S.Shields,
England, 15"? reflector), Feist, Lovas (Hungary), Moore, Wilkins (Kent,
England, 7" refractor, x500) "Obliterated by a hovering cloud (Feist
disagrees). Budapest obs. saw a cloud at 21:02:30, lasting 5 m . Moore &
Wilkins saw burst of light & dust cloud at 21:02:35 (confirm.) Drawing
by Lovas." NASA catalog weight=1 and catalog ID #722. The ALPO/BAA
weight=1.
2015-Apr-30 UT 04:36-05:20 Ill=85% Aristarchus observed by Weier_D on 1990-1-8
On 1990 Jan 08 at UT00:55 D. Weier (Sun Praire, WI, USA, 12.5"
reflector, x159) observed an "anomalous black bar across Aris. Nearly
digonal to terminator." The nearby crater Prinz had curious shadow
patterns, perhaps related to the rising sun projecting shadows from the
eastern rim and "reflected down"? "At 0224 W wall had a break in it & a
diffuse glow where it should not be. Manske thinks it was Earthshine
effect. At 0305 Weier saw Manske's bar - with diffused light and
flicker like an aurora - like a gas with electric charge. At 0325 saw a
strange glow in Aris. but may be due to atm. though thought it to be a
LTP. Darling had never seen such effects before (flickering implies a
medium in it)." The Cameron 2006 catalog ID=387 and the weight=3. The
ALPO/BAA weight=3.
2015-Apr-30 UT 21:09-21:19 Ill=90% Bailly observed by Miles_H on 1965-5-12
On 1965 May 12 at UT 22:20 H. Miles (UK) found a possible
obscuration in Bailly crater. Most of the region was as sharp as
normal, but the central area was greyish and blurred. Although
the observer concerned considered themselves a non-experienced
observer, another BAA Lunar Section observer saw the same
effect. ALPO/BAA weight=2.
2015-Apr-30 UT 21:09-23:59 Ill=90% Aristarchus observed by Baumeister on 1973-8-10 *
Aristarchus 1973 Aug 10 UTC 20:14 observed by Baumeister (48.63N,
9.25E, 110mm reflector, T=2, S=2) "Orange to red colours at the crater
floor dissappeared until 21:04" - Hilbrecht and Kuveler, Earth, Moon &
Planets, 30 (1984), p53-61. ALPO/BAA weight=2.
2015-Apr-30 UT 21:09-22:26 Ill=90% Vallis_Schroteri observed by Gray_R on 2004-11-24
Aristarchus Area 2004 Nov 22 UT 04:58-05:49 Observed by Gray
(Winemucca, NV, USA, 152mm f/9 refractor, seeing 4-5, trasparency 4-5,
x114, x228) "Blinked Herodotus with Wratten filters Blue 38A and Red
25. The illuminated west crater wall stood out brilliantly in blue
light, much more so than in white light. This was true also of
Aristarchus. Red light did not increase contrasts in Herodotus any more
than they were in white light. Shadows in Herodotus appeared as black
as the night west of the terminator and remained that way throughout
the observing period. No TLP seen in Herodotus tonight. A possible TLP
was seen to the west of Herodotus near the terminus of Schroters
Valley. It was noted at the beginning of the observing period that
there were four very bright spots of light, one near the end of
Schroters Valley, the other three grouped together a little farther
north. Although not far from the terminator they were definitely east
of it. It was noted that all of them nearly vanished in the Blue 38A
filter while Aristarchus and the rim of Herodotus gleamed brilliantly.
At 5:19UT it was noted that the most brilliant of the four lights, the
one near the terminus of Schroters Valley, had faded almost to
invisibility in white light. When first seen it had been brighter than
Aristarchus. It remained very dim after this through the remainder of
the observing period, and was unchanged at 7:35-7:49UT when I again
examined the area. The other three bright spots remained brilliant and
unchanged."
2015-Apr-30 UT 21:12-22:22 Ill=90% Aristarchus observed by Kidd_S on 2009-12-28
On 2009 Dec 28 at UT17:35 S. Kidd imaged a spot on the inner W
rim of Aristarchus. However he thinks that it is an artifact of
the software that he used to extract a sharp image out of the
acquired video AVI file. The ALPO/BAA weight=1 until we have
fully evaluated the situation.
2015-Apr-30 UT 21:15-23:59 Ill=90% Plato observed by Robinson_JH on 1973-8-10 *
Plato 1973 Aug 10 UT 22:45 observed by Robinson (Devon, UK).
Observer noticed that the lighter areas on the floor were more
distinct in red than in the blue filter. ALPO/BAA weight=1.
2015-Apr-30 UT 22:42-23:59 Ill=91% Herodotus observed by Hill_H on 1966-11-24
Herodotus 1966 Nov 24 UT 21:50 H.Hill (UK, 7.25" reflector,
x240), seeing 4-6/10, transparancy 4/5) sketched a central white
diffuse patch inside the floor of the crater, with a size of
about 1/7th the diameter of the crater. The eastern edge of the
white patch was encroached by the shadow of the eastern rim.
ALPO/BAA weight=3.
2015-Apr-30 UT 22:59-23:59 Ill=91% Encke_B observed by Blanco_J on 1990-9-1
Blanco, J. Vidal, of Gijon, Spain (3" refractor x72)
noticed an unfamiliar very bright center near to Encke.
Cameron suspects that this was Encke B crater
on the basis that it is a prominent small crater
near to Encke. Cameron 2006 catalog extension ID=410
and weight=2. ALPO/BAA weight=1.
2015-Apr-30 UT 23:03-23:59 Ill=91% Proclus observed by Bartlett on 1976-9-6
Proclus 1976 Sep 06 UT 02:00 Observed by Bartlett (Baltimore, MD, USA,
4.5" reflector 45-300x, S=3, T=5) "Nothing vis. on floor of 2deg
brightness. Usually floor ray & Proc. A are vis. at this col. & c.p. is
5 deg bright. (must have been 2 deg tonite)." NASA catalog weight=4.
NASA catalog ID #1450.
2015-Apr-30 UT 23:04-23:55 Ill=91% Torricelli_B observed by Cook_MC on 1983-4-24
All observers saw a blue tinge seen inside and outside the
crater. Marshall observed a bright spot in the middle of
the crater floor and thought perhaps that it was a central
peak. No central peak can be found on Lunar Orbiter images.
Cameron 2006 Catalog extension ID=214 and weight=5. ALPO/BAA
weight=4.
2015-Apr-30 UT 23:30-23:51 Ill=91% Aristarchus observed by Budine on 1964-2-25
Cobra Head, Aristarchus 1964 Feb 25 UT 02:37-02:38, 02:39-02:42
Observed by Budine (Binghamton, New York, USA, 4" refractor, x250, S=6,
T=4) "Red flashes" NASA catalog weight=3 (average). NASA catalog ID #
802.
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