The Owl Nebula

Messier 97
Messier 97

Object Name: M 97 (NGC 3587)

Location: RA: 11h 15m 36.0s, Dec: +54° 01′ 08″

Magnitude: 11

Dimensions: 3.4 ‘x 3.3’

Constellation: Ursa Major

Type: Planetary Nebula. Class IIIa

Observing Location: Bonilla. Cuenca

Date: February 9, 2013.

Time: 23:58 T.U.

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

Telescope S/C 8″ Mount Cgt-5

Eyepiece: Hyperion Aspheric 31 mm; Magnification: 65x.

Conditions: NEML: 5.3 (Zone 4 Gem.) Temp.: -4º C, Humidity 72%, Slight breeze.

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

Rosette Nebula

Rosette Nebula
Rosette Nebula

Hi all!

I made an observation about Rosette nebula with my 10X50 binoculars. This is a digital drawing, but I hope you like it! 🙂

Date: 2012-01-05 20:33UT
Object: NGC2237-2238 (open cluster and nebula)
Location: Nagyvarsány/Hungary (N: 48°09’37” E: 22°16’46”)
Temperature: -2°C (windy)
My blog: www.viktorcsehdraws.blogspot.com

Clear skies!

Viktor

White Light and H-Alpha Sun from Polaris Observatory

White Light Sun - February 18, 2012
White Light Sun – February 18, 2012

Dear Asod,

I send you hereby my sketch made this Saturday at Polaris Observatory, Hungary. I used a 114/900 Skywatcher with Baader solar filter for white light sketch and a Lunt 35 for the H-alpha sketch.
The most intersting part is a solar prominence on the northern edge, which is was a very 3D something, biting in the sun-disk.

Equipments used: 114/900 SW (100x) & Lunt 35/400 H-alpha
Date: 18th February 2012, UT: 10:40 (white light) and 11:20 (H-alpha)
Place: Hungary, Budapest, Polaris Observatory
Media: graphite pencil used on white paper

Clear skies,
Judit

Mars – February 19, 2012

Mars - February 19, 2012
Mars – February 19, 2012

Object Name: Mars
Object Type: Planet
Location: Lombard, IL, USA, 41° 52′ 48″ N / 88° 0′ 28″ W
Date: 19 Feb 2012, 22:20-22:45 CST
Media: Pencil
Comments: This is Mars observed using my homemade 8″ f5.9 dob and Baader Hyperion 5mm, I had a pretty good seeing that evening. After scanning the picture, color balance was adjusted in Photoshop to better resemble observable Martian palette. The image to the right was generated by Stellarium for comparison.

Lunar Terminator – August 25, 2012

Lunar Terminator - August 25, 2012
Lunar Terminator – August 25, 2012

Hi,

I send my sketch of the Moon. The sketch was made on Aug. 25, 2012, by means of white watercolor and dry pastel. That night the moon was 8 days after the new moon. He was low on the horizon but still was strong in my telescope. This is my first picture of the moon.
GREETS

Date: 25th August 2012
Location: Pasry in Poland
Telescope: Newton 8 ”
Media: white watercolor and dry pastel, black paper

Gassendi Crater

Gassendi Crater
Gassendi Crater
Move cursor over image to view labels.

2012 06 01, 0238 UT – 0446 UT Gassendi
PCW Memorial Observatory, Texas, Erika Rix
www.pcwobservatory.com

Celestron Omni XLT 102mm, 24-8mm Baader Planetarium Mark III Hyperion, 2x Barlow, 250x
Temp 71° F, 60% humidity, S: Antoniadi II, T: 5/6
Eyepiece sketch black Strathmore Artagain paper, Conte crayon and pastel pencil, charcoal pencil
Phase: 45.8 deg, Lunation: 11.21 d, Illumination: 84.8%
Lib. Lat: +05:08, Lib. Long: -04:13
Az: +209:11, Alt: 41:03

Located on the northern border of Mare Humorum, crater Gassendi is an impact crater formed during the Nectarian period (-3.92 to 3.85 billion years ago) that later was modified after volcanic activity, becoming a fractured-floor crater. Gassendi is believed to have been filled with lava from the inside, raising its floor, creating stress fractures in the process. This would explain it being considered a walled plain with a shallow depth of 2.8 km. The central peaks (~1200 m high) remain and several rilles (called Rimae Gassendi) were formed on the lava-filled floor during the Imbrian geological period -3.85 to –3.2 billion years ago.

Crater Gassendi A was formed during the Copernician period (–1.1 billion years ago to the present day) and overlaps Gassendi’s northern rim. The pairing of Gassendi and Gassendi A resembles a diamond ring and makes a very striking feature to observe 3 days after first quarter or two days after last quarter of lunation. My observation was nearly three days after first quarter.

Gassendi’s southern rim was swallowed by the lava of Mare Humorum leaving only a thin crest line to support its circular shape. Dorsa ran from the southern rim to Gassendi O (11 km wide). The sharp ridge that defines the border of Mare Humorum to the SW of Gassendi adds to the crater’s unmistakable identification.

At the beginning of my session, Spica and Saturn lined up to align with the Moon. Spica was 2.08 degrees north of the Moon and Saturn was 6.9 degrees north of the Moon. Extending further north, Arcturus was nearly in line as well at 31.8 degrees north of the Moon