Facets of the Dolphin

Objects in Delphinus
Objects in Delphinus

Dolphin Constellation

several objects

Location: The Bullaque – Ciudad Real – Spain

Date: 2013 – September – 01

Media: Graphite Pencil HB, torchon drawing sheet 1 and 130g

Inverted colors with GIMP 2.8

The Dolphin is a summer constellation modest, but can be very interesting for the amateur observer. Spend an evening full observation of its four most significant objects two planetary nebulae and two globular clusters, has been very rewarding.

When observed at the same time, are more striking differences between the two planets:
NGC 6905 is sees as a small disk, very bright and is easily distinguished in the field, and
NGC 6891 is quite the opposite, very small, very bright and compact, ie stellar appearance, difficult to distinguish from the other stars in the field.

The two globular clusters are very different concentration among them, but the different distances from us makes visual texture is very similar:
NGC 6934 (Class VII and 50,000.) Is bright, large, round, with denser center, feathered edges and mottled texture, and
NGC 7006 (Class I and 150,000 al.) Is less bright, somewhat smaller, round, with denser center, feathered edges and mottled texture.
A sample of observation is the sketch I made (picture above).

Finding NGC 6891 has been a challenge, stellar appearance has remained up to 200x and only from the 220x has started to show a very small round and compact disc.
The UHC filter and averted vision were needed in the localization and subsequent observation of nebulae.
For all objects have the best view obtained with the 220x. Good quality of the sky with a 21.41 SQM (roughly Male zone 6 was 6.2).

Greetings to all visitors of this page

Pedro Villamiel 09/04/2013

From Zucchius to Schiller

Zucchius, Schiller and environs

Zucchius, Schiller and environs

On the evening of September 16, 2013, I got the best view of the basin ring segment between young crater Zucchius (65 km.) and just the tip of large older crater Schiller (179 km.) The ring arc was more than a day beyond the terminator but perfectly illuminated to show its depth and smoothness.
Craters Weigel (36 km.) and Weigel B (37 km.) initially caught my eye as light was brightly glinting off the rims.
For an excellent image of this region see the LPOD for May 26, 2013
http://lpod.wikispaces.com/May+26%2C+2013
There were many fine crater showing nicely in this region at the time of the observation and sketch.
Sketching:
For this sketch I used: black Canson paper 9″x 10″, white and black Conte’
pastel pencils , and Conte’crayons, a blending stump, Pink and White Pearl erasers. Brightness was not altered but contrast was increased +3 using the scanner for this sketch
Telescope: 10 inch f/ 5.7 Dobsonian with 6mm (241x) eyepiece
Date: 09-17-2013, 02:00 – 03:45 UT
Temperature: 16°C (60°F)
Clear, calm
Seeing: Antoniadi II
Co longitude 53.8°
Lunation 11.42 days
Illumination 91.5%

Frank McCabe

Messier 67

Messier 67
Messier 67

Object Name : M67
Object Type : Open Cluster in Cancer
Location : Suppi-ryung Kunnam-myeon Chulwon-gun Gang won-do South.KOREA)
Date : 2013.2.8 Friday
Media : A4 paper, HB pencil
Equipment : 10′ dobsonian, XW 20mm
Observing conditions : clear sky(Excpet south sky)
This my first DSO sketch in my life.
Spent 1hour to sketch, 3:00 ~ 3:30

The Gigantic Face on the Yura Mountain Range

Yura Mountain Range
Yura Mountain Range

Although recently I have very much interested in Lunar horizon landscpe observation, and also it is a serious hard work that need preparationes, concentrations, patiences to acquire the most valuable results that nobody has seen yet .

So , for me, Lunar horizon observation time is limited , as a or two months of winter season in a year.

Then, other seasons, I useally observe others.

With a fairly good optics [like mine or better…], anyone can find out enormous amount of details on the face of the moon [also on the limb].

One night, very accidentally, I had just seen a much interesting feature in the binocular eyepieces attatched on my faithful 8 inches refractor on along the Yura Mountains range [= Montes Yuras ] , which very resembance to a human’s face … a giant’s face… !! . I was instantlly surprised at the view …. !!!

It’s real dimension , I measured from the diameter of 100 km Plato , must be about within 20 km in length.

Among the many moon sketches of mine , in which shows many curious, grotesque features.. and this gigantic human face is one of that.

Unfortunatelly, by interuption of front roof top, observing time is limited only as 15 minutes, that limits more details on this sktch.

——-[ Upside is the North of moon, Right side is West. ]—–

by K.S.Min

8 inches refractor x340- 500

white paper, graphite pencils, photographed under 300 watt white bulb

At backyard home, in South Korea

M84, M86 and More

M 84, M 86, NGC 4388, NGC 4402, NGC 4387
M 84, M 86, NGC 4388, NGC 4402, NGC 4387

Object Name: M 84, M 86, NGC 4388, NGC 4402, NGC 4387

Location: M 84: RA: 12h 25m 03.7s; Dec: +12° 53′ 13″

M 86: RA: 12h 26m 11.7s; Dec: +12° 56′ 462

Constellation: Virgo

Observing Location: Bonilla. Cuenca. SPAIN

Date: 13-14 April 2013.

Material used: graphite pencil on white paper. Inverted image and processed with Photoshop.

Celestron Telescope S/C 8″ Mount Cgt-5

Eyepiece: Hyperion Aspheric 31 mm;

Magnification: 65x.

Conditions: NEML: 5.9, Temp.: 10° C.

More information: http://astrodibujo.blogspot.com.es/

Jupiter’s Wondrous Red Spot

Jupiter's Great Red Spot
Jupiter’s Great Red Spot

This is the drawing I have made last year. ….
It represents the Great Red Spot of Jupiter.I have mentioned the details of the drawing below.Thank you.
Object Name : Jupiter
Object Type : Planet
Location : Pune, Maharashtra, India.
Date : 28 June 2012
Media : Canvass and acrylic colors

Thanks & Regards,
Amruta Sunil Pund

Eratosthenes

Eratosthenes Crater
Eratosthenes Crater

2011 10 07, 0330UT Eratosthenes

PCW Memorial Observatory, OH, USA, Erika Rix

www.pcwobservatory.com

Eratosthenes: Complex crater from Eratosthenian geological period (from –3.2 billion year to –1.1 billion years)

Lat: 14.5 deg N, Long: 11.3 deg W

Zhumell 16”, 21-7mm Zhumell, 257x, no filter

Temp14C, 89% increasing to 98% humidity, S: Antoniadi II, T: 6/6

Eyepiece sketch on Rite in the Rain paper, charcoal

Phase: 54.3 deg, Lunation: 9.68d, Illumination: 79.1%

Lib. Lat: -05:01, Lib. Long: +05:37

Az: +246:38, Alt: -07:34

Eratosthenian geological period includes fairly young, non-rayed fresh craters. I did notice a Copernican ray to the N of Eratosthenes and several patches of lightened areas within the surrounding areas. Eratosthenes has very steep, tormented walls and is approximately 60km x 60km wide. It has an elongated central mountain with several summits. Its morphology is very similar to impact crater Copernicus, but its rays most likely deteriorated from weather and age.

The distance of this crater from the terminator made it perfect for studying the floor and terraced walls. The western floor edge was difficult to differentiate from where the upslope began for its wall. It appeared to be more a lightening with a few darkened lines.

For comparison, here is an image from the Lunar Orbiter (through the Lunar and Planetary Institute site). My sketch is the eyepiece view from my telescope and will need to be rotated 180 degrees to match the Lunar Orbiter image.

Halley’s Comet

Comet 1P/Halley
Comet 1P/Halley

Hey Artists!

My sketch here, shows the famous comet Halley as seen at its best from Norway.
The bright coma had a drop-form, and a halo was seen in the outer coma to west.
In my 10 x 50 binos, the tail was narrow and 2 deg. long. Info on my sketch.
Halley returns in 2061, so good luck to the younger observers!
I used colour crayons on black paper.
Location : Trondheim, Norway.

Best wishes from : Per-Jonny Bremseth.